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Massive elements can build up in celestial catastrophes like supernovae, with the rapid-, or r-process, producing neutrons at a high rate as elements much heavier than lead or even uranium emerge. But we’re learning that such events happen not just in supernovae but also in neutron star mergers, which are thought to occur only a few times per million years in the Milky Way. A new paper looks at meteorites from the early Solar System to study what the decay of their radioactive isotopes can tell us about the period in which they were created.

Such isotopes have half-lives shorter than 100 million years, but we can determine their abundances in the early Solar System through meteorite studies like these. What Szabolcs Márka (Columbia University) and Imre Bartos (University of Florida) have done is to study how two of the short-lived r-process isotopes were produced, using simulations of neutron star mergers in the Milky Way to calculate the abundances of specific radioactive elements. The simulations show that about 100 million years before the Earth formed, a neutron star merger occurred some 1,000 light years from the gas cloud that would become the Solar System.

This would have been a spectacular event, says Márka:

“If a comparable event happened today at a similar distance from the solar system, the ensuing radiation could outshine the entire night sky.”

Image: This is Figure 1 from the paper, which appeared in Nature. Caption: The path of r-process elements. When neutron stars merge, they create an accreting black hole (the accretion disk is shown red). Tidal (dynamical) forces and winds from the accretion disk eject neutron-rich matter. This ejected matter (ejecta, shown grey) undergoes rapid neutron capture, producing heavy r-process elements, including actinides. The ejecta reach the pre-solar nebula and inject the heavy elements that will remain in the Solar System. Credit: Szabolcs Márka / Imre Bartos.

Because a supernova can likewise produce actinides (elements from actinium to lawrencium — atomic numbers 89-103 — all of them radioactive), the authors use the same methods to analyze these. The evidence points to a neutron star event rather than supernovae explosions near the early Solar System, for the abundance ratio found via meteorite studies “…is well below the uniform production model’s prediction…” What the authors mean by ‘uniform production model’ is the fact that supernovae are orders of magnitude more frequent in the Milky Way than neutron star mergers, and their production rate can be approximated as being uniform in time:

By comparing numerical simulations with the early Solar System abundance ratios of actinides produced exclusively through the r-process, we constrain the rate of occurrence of their Galactic production sites to within about 1−100 per million years. This is consistent with observational estimates of neutron-star merger rates, but rules out supernovae and stellar sources. We further find that there was probably a single nearby merger that produced much of the curium and a substantial fraction of the plutonium present in the early Solar System. Such an event may have occurred about 300 parsecs away from the pre-solar nebula, approximately 80 million years before the formation of the Solar System.

The authors point out that working backward to reconstruct the abundance of another of the short-lived elements would help to produce a more complete picture of the neutron star merger.

Because I was having trouble with the distinction between actinides produced by supernovae and those from neutron star mergers, I asked Dr. Bartos for a clarification. He was kind enough to provide the following, explaining how supernovae can be ruled out (and many thanks to Dr. Bartos for his quick response!):

The difference between supernovae and neutron star collisions that we take advantage of is their relative rates. Supernovae occur a thousand times more frequently than neutron star collisions in the Milky Way. This means that the shortest lived isotopes would be regularly replenished if produced by supernovae, making them certain to be present at the time of the Solar System’s formation. For the less common neutron star collisions, the shortest lived isotopes are depleted soon after a merger, and stay depleted until the next. This means that it is probable that at the time of the Solar System’s formation, this isotope will be depleted. The observed abundances of the short lived Curium-247 and Iodine-129 isotopes in the early Solar System show this depletion, ruling out supernovae.

Dr. Bartos went on to explain the steps he and co-author Márka took to clarify the result:

An extra step is that we normalize the Curium and Iodine amounts found in the early Solar System with the amount of longer-lived r-process elements (Thorium-232 and Iodine-129, respectively). This is important because this way our results don’t depend on how much r-process a single event produces. The ratios stay the same.

We’re in the early era of using gravitational wave astronomy through observations from LIGO and the Virgo collaboration to make the call on the rate of spectacular events like the merger of two neutron stars, a rate that will be tightened further with continuing observation. Thus the Abadie et al. paper I reference below, tapped by the authors, which points to the rich observational fields gravitational waves help us explore. It was a scant five years after that paper that the first gravitational wave detection was made, and in the short time since, we are now producing catalogs of black hole and neutron star mergers.

The paper is Bartos & Márka, “A nearby neutron-star merger explains the actinide abundances in the early Solar System,” Nature Vol. 569 (2 May 2019). pp. 85-87 (abstract). The Abadie paper referenced above is Abadie et al., “Topical review: predictions for the rates of compact binary coalescences observable by ground-based gravitational-wave detectors,” Classical and Quantum Gravity 27, 173001 (2010). Abstract.

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Centauri Dreams’ resident movie critic turns his attention to a personal favorite from the canon of science fiction films. My own memories of The Thing from Another World go back to late Saturday night black-and-white TV, where I first saw the chilling tale as a boy. The scene where the team fans out on the ice as they try to figure out what it is that is frozen down there still puts a chill down my spine. Who knew at the time that The Thing himself was James Arness, early in his career arc toward Gunsmoke’s Matt Dillon? Larry gives us all the details, including reflections on the film’s significance in its time and the questions it raises about our attitudes toward the unknown. Don’t be surprised to find a collection of Larry’s Centauri Dreams essays making its way into book form one of these days.

by Larry Klaes

Ah, aliens. For some humans, they are the conquering interstellar warriors of some tyrannical Galactic Empire. To others, they are angelic saviors just waiting to uplift humanity into the wider Cosmos. To still more, they are aloof godlike beings who are completely indifferent to anyone unlike themselves. If an alien happens to be a member of the Star Trek franchise, the chances are very good they will look, talk, and act very much like a certain primate species of the planet Sol 3 (a.k.a. Earth), with perhaps some variations to the ears and nose.

In many science fiction stories dealing with extraterrestrial intelligences (ETIs), aliens can be all four of the types mentioned above. However, just as often our imagined cosmic neighbors can and do become little more than outright monsters: Creatures of the Id aimed at our basest fears who exist only to maim, extinguish, and sometimes consume unwary victims – while giving audiences visceral thrills designed to voluntarily release portions of their currency to these story makers multiple times.

This last category became the standout feature of many science fiction films, hitting their stride in the 1950s. The results range from great in a few notable cases down to quality levels that were found wanting for the majority of the rest.

One of the earliest and most memorable standouts of this genre from the mid-Twentieth Century was the science fiction/horror film titled The Thing from Another World (often referred to as just The Thing), Produced by the Winchester Pictures Corporation and released by RKO Radio Pictures, it premiered on April 27, 1951.

Given a cursory look, the main plot and overall trappings of this cinematic experience called The Thing can give one the impression of this motion picture being a standard, albeit classic, “monster movie.”

Or so it might seem…

Members of the United States Air Force (USAF) stationed at an air base in Anchorage, Alaska, are ordered to investigate a report by scientists at a remote Arctic research station of a possibly unusual aircraft that has crash-landed near the North Pole. Speculation on the craft’s identity ranges from the Canadians to the Russians, with the latter described as being “all over the pole like flies.” This is during the first decade of the Cold War, after all.

Image: The original film poster for The Thing from Another World.

The team of military airmen, the lead scientist of the research station, and a nosy journalist who is eager for a juicy story fly together to the reported crash site: They come upon not the expected terrestrial airplane in need of rescue, but instead a saucer-shaped alien spacecraft frozen in the Arctic wasteland! As the team attempts to remove the extraterrestrial vessel buried in the ice using thermite bombs, they accidentally destroy the entire ship in the process. However, the body of a lone occupant from the craft is found nearby, frozen in the ice.

The rescue/expedition team flies with their invaluable “prize” to the science research station just ahead of an approaching blizzard. There they crudely quarantine their confined “visitor”, only to have the alien being accidentally revived from its ice prison (by an electric blanket left on, no less).

Surprising the single guard on duty, the sentry uses his gun to shoot the alien multiple times, but without noticeable effect. The being subsequently escapes and proceeds to go on a rampage, injuring and killing both men and several of the station’s sled dogs.

Despite the creature’s violent and deadly behavior, which includes procuring the blood of its victims for both food and reproduction, the resident chief scientist perceives the alien as a highly evolved and therefore wiser and better being than his fellow humans: After all, this extraterrestrial life form arrived in a starship.

The scientist explains the alien’s hostile actions as a defensive response to its treatment by the equally hostile “alien” creatures from the station, along with their unwillingness to truly communicate with it. In stark contrast, the military personnel naturally and not without reason see this “thing” from outer space as a dangerous monster that threatens all their lives and possibly every other organism on Earth!

After attempting and failing to kill the alien intruder with bullets and fire, the airmen have one last plan to stop the creature before they are either slaughtered by the alien or freeze to death, as the alien has sabotaged the station’s furnaces. Their hope is to trap the alien in the generator room, where the humans are making their last stand, and electrocute the creature with a contraption rigged up along the floor.

Just as the alien enters the trap area, the lead scientist breaks ranks and rushes right up to the being, where he attempts to plead directly with the alien in order to reason with it to save its life so that the alien may in turn share its presumably superior knowledge and wisdom with humanity. The being responds by harshly knocking the scientist aside and continuing after the airmen.

The creature does step into the trap, where it is brutally electrocuted to the point of disintegration: The station and the world are saved by the menace from beyond the stars by a bunch of modern-day warriors wearing leather bomber jackets underneath their parkas.

Later on, having a news “scoop” beyond his wildest dreams, the reporter relays the events of the last two days to his very eager listeners. Ready to plunge in with the details, the reporter first gives his audience (and by proxy the film’s viewers) this warning and plea:

“Every one of you listening to my voice… tell the world. Tell this to everybody wherever they are: Watch the skies everywhere. Keep looking. Keep watching the skies!”

Roll credits.

Let us first acknowledge what should be the obvious: That The Thing is a film with a story and characters written by and for human beings of the planet Earth; in particular, American human beings from the mid-Twentieth Century in the midst of the Cold War era who were also in the thick of dealing with anti-communist “witch hunts”.

There was also a particular mindset in terms of social conventions at the time of how men and women should be and behave, especially towards anything that was different, even in ways that did not have to be literally alien to trigger certain responses.

The alien visitor in this story could have been friendly, or at least non-hostile, without sacrificing dramatic suspense and excitement in the process. This is what took place in the contemporary science fiction film It Came from Outer Space, released in 1953: The ETI in this story were also the victims of a spaceship that crashes on Earth, yet their only intentions were to repair their vessel and return to the stars. These aliens were explorers, not conquerors. They even informed the main human character, who happens to be an astronomer, that the two species were not yet ready to meet peacefully, for it was humanity which had a lot of maturing to do.

The aliens’ take on the situation was reinforced by the fact that an angry, armed mob of humans had been coming to destroy them, certain that these uninvited “guests” from outer space had only hostile intentions for the native terrestrials. Granted, the aliens had temporarily “possessed” certain townsfolk, which made them act unusual in the process, but this was only done in order to provide camouflage so that the distant voyagers could obtain the repair tools they needed in the nearby desert community as unobtrusively as possible. Had the aliens revealed their true physical appearance to the humans, they would have automatically terrified the local populace and created an even more immediate hostile response.

The resident scientist in It Came from Outer Space had been successful in quelling the mob from destroying the aliens in his story. The astronomer even kept the ETI from killing the humans that threatened them, which they reluctantly intended to do rather than be either captured or exterminated by these comparatively primitive and savage creatures.

This was not to be in the case with the “thing” in The Thing. The deck was stacked against this alien almost from the start. The very title of the film calls the alien a “thing”, even though the lead scientist, Dr. Arthur Carrington, emphasizes repeatedly the fact that the being came to Earth in a starship from another part of the Milky Way galaxy, stating that it therefore must possess at least some superior knowledge and wisdom (the alien is even dressed in a “civilized” fashion, wearing some type of manufactured coverall uniform).

Even the 1938 short story written by John W. Campbell, Jr., that The Thing is based on was titled “Who Goes There?” and the alien in that version was far more hideous, manipulative, and deadly to the trapped men of the Antarctic research station than the one of the 1951 film (the alien in the 1938 story was referred to only as the Thing, though).

The original cinematic plans for the physical appearance of the alien were more monstrous than the result that eventually arrived in the final film version. In a screenplay draft dated August 29, 1950, the first clear sight of the alien is described this way:

“He switches on his flashlight, and centers its beam on the ice-block. As Ericson said, the ice is now almost transparent. Through it, only partially distorted, can be seen an unearthly horror. It has a bulbous head, a tiny suck-hole for a mouth, multiple eyes, no ears. Its arms are extra-long, ending in thorny clusters, rather than hands. It stares malevolently through the ice.”

Despite this and other ambitious and creative concepts developed during production of The Thing, the filmmakers had neither the special effects technology nor the budget to make the alien look both so elaborate and convincing on screen. They finally settled on a being that bore more than a passing resemblance to the famous “monster” created by Victor Frankenstein in what is considered to be one of the first modern science fiction novels: Frankenstein; or, The Modern Prometheus, written by English author Mary Shelley (1797–1851) and first published in 1818.

Specifically, the alien bears definite similarities to the version which most people identify with Frankenstein’s creation, the one made for the iconic Universal Studios film, Frankenstein, released in 1931 and played by actor Boris Karloff.

This decision, intentional or otherwise, has its own allusions to our discussion theme. In the original Shelley novel, the “monster” was actually intelligent, articulate, and feeling. He only became hostile and murderous after relentless negative encounters with human beings who were frightened by his appearance. A similar situation took place with Frankenstein’s creation in the 1931 film (and initial sequels), although here the “creature” was portrayed as being less intelligent and verbose, though no less feeling. In fact, had the makers of this landmark horror film gotten their way, the “monster” would have been reduced to a purely instinctual killing machine, all for the sake of entertainment.

Image: Actor James Arness portraying the title character. Note the more than casual resemblance to the cinematic Frankenstein monster, and not just due to film production budget and contemporary FX technology restraints.

Nature versus Nurture, or You’ve Got to be Taught to Hate

As the alien was not terribly big on civilly “dishing” about itself during the film, the hapless humans trapped with it (and by proxy, the viewing audience) often had to make their own assumptions regarding the nature of their uninvited guest from the stars and its true intentions. Naturally human biases, instincts, training, and educational backgrounds play a big role in the numerous assumptions and reactions. This includes the thoughts and intentions of the script writers, both subconscious and conscious.

A big part of these guesses involve whether the alien was provoked into its hostile reactions, or did it indeed intentionally come to Earth to introduce its species as the new dominant life form for our planet. We know for a fact that the humans were already splitting off into their own camps of thought from the moment they realized that the craft which crashed in the Arctic was no terrestrial airplane, not even something exotic from their chief Cold War rival.

Image: The airmen and scientists discuss what to do with their unexpected visitor trapped in the ice – but soon their “guest” will force their hands in the matter.

When they found the alien in the ice and brought it back to the research station, the enlisted military men who were assigned to guard it repeatedly told the others how uncomfortable they felt just being near the creature, even though at first everyone assumed it was dead. This instinctual reaction led one of the sentinels to place an active electric blanket over the ice block containing the alien so he would not have to look at it – or have the being look back at him, which he swore it was doing. This event caused the frozen chunk of water to melt and subsequently release the alien – which turned out to be very much alive!

One item before we continue: It was stated in the Internet Movie Database (IMDB) Goofs section for The Thing that the heat from a working electric blanket placed directly upon a large amount of ice would produce a lot of liquid water, enough to short out the blanket early on. Of course the plot required an unintentional reason for the alien to be released and active, since the USAF officer in charge, Captain Patrick Hendry, refused to have the alien removed from the ice block for any reason until he heard back from his superiors for further instructions.

One wonders what might have happened if the alien had not only been placed under more competent security, but included being monitored by the station scientists? They were in a civilian scientific research station, after all, not a military base. Instead, the being was placed in an unheated store room (a window pane was broken to make the room even colder from the outside air) and watched by shifts of lower ranking airmen – men who were trained to respond to unknowns either defensively or offensively and only follow orders.

While certainly none of the humans in this story had ever encountered an actual alien being before, these members of the warrior class were probably the least advisable people to have watch over such a life form in such a situation (and why just one person at a time, for that matter?).

When the alien did become free of its ice prison, the first reaction from the guard was to shoot it with his gun, six times in fact. We later discover that the bullets had no lasting effect on the alien, at least in the physical sense. Soon after, as the being was attempting to escape from the station, it was set upon by three of the sled dogs. The alien also survived that encounter (and killed two of the dogs outright in the process, while injuring the third badly enough that it had to be put down on the spot), but it lost an arm during the attack. No doubt by that time, if the being had any thoughts of the natives of this planet being friendly or at least non-hostile, they were utterly extinguished.

Of course the audience already “knows” that the alien is going to react negatively towards any and all terrestrial life forms it encounters. Not only is it called The Thing in the film’s title (as opposed to, say, E.T. The Extraterrestrial, like that friendly and adorable little alien in the 1982 film co-produced by Steven Spielberg), we are told and shown in various ways via the 1951 film’s trailer and marque posters that we are going to see a horror flick. The Thing is not a balanced, scientific documentary on the subject of ETI thinking, behaviors, and intentions.

Despite being quite humanoid in appearance, the alien in The Thing is revealed to be even less like a human or even what most humans consider to be a “higher” life form: When the scientists analyze the arm ripped off the alien during its battle with the sled dogs, they discover it is composed of material more like a plant than an animal.

The mammalian humans present are clearly not easily able to wrap their minds around the idea of a thinking, walking plant in general, let alone one that can build and fly a starship. This combination of ignorance, fear, and bias only makes the extraterrestrial being even more alien to most of the station residents, heightening their concerns about their “guest”.

The reporter, Ned “Scotty” Scott, and Dr. Carrington have the following conversation during this revelation, which leads to one of the most infamous lines in the film:

Scotty: “Please, doctor, I’ve got to ask this. It sounds like, well… Just as though you’re describing some form of super carrot.”

Dr. Carrington: “That’s nearly right, Mr. Scott. This carrot, as you call it, has constructed an aircraft [!] capable of flying millions [!] of miles, propelled by a force as yet unknown to us.”

Scotty: “An intellectual carrot. The mind boggles.”

Dr. Carrington: “It shouldn’t. Imagine how strange it would have seemed during the Pliocene [!] age to forecast that worms, fish, lizards that crawled over the Earth would evolve into us. On the planet from which our visitor came, vegetable life underwent an evolution similar to that of our own animal life, which would account for the superiority of its brain. Its development was not handicapped by emotional or sexual factors.”

When the reporter tells the scientist that his readers would likely consider the notion of an “intellectual carrot” as too wild to be taken seriously, Dr. Carrington counters this attitude by asking one of his colleague to give several examples of real terrestrial plant species: One type, the acanthus century plant, can capture and consume a variety of small animals. The other flora mentioned is the telegraph vine, which is aptly named, as it can send signals to other members of its species many miles apart.

“Intelligence in plants and vegetables is an old story, Mr. Scott. Older even than the animal arrogance that has overlooked it.”

Dr. Carrington’s fascination and unabashed admiration for the alien only grows when they discover that the being reproduces by creating seed pods from its body:

“Yes. The neat and unconfused reproductive technique of vegetation. No pain or pleasure as we know it. No emotions. Our superior. Our superior in every way.

“Gentlemen, do you realize what we’ve found? A being from another world as different from us as one pole from the other. If we can only communicate with it, we can learn secrets that have been hidden from mankind since the beginning.”

Dr. Carrington betrays his own biases here. While he is likely the only human at the research station who does not want the alien either dead or at least sent somewhere very far away from them, the scientist also assumes that just because the being came to Earth in a technologically advanced spaceship, it is therefore morally and ethically superior as well, if such concepts can be applied to a species that evolved in a different manner on another world in another solar system.

The film also betrays its own stereotypical views when it comes to scientists: Dr. Carrington is deeply impressed, bordering on envy, over how the alien makes copies of itself. Since it does not involve sexual reproduction and all the “complicated” (read messy) physical and psychological baggage that process tends to bring, at least for higher intelligence species like humans, Dr. Carrington sees the alien’s method as essentially unemotional and therefore superior. This goes along with his character’s devotion to Science with a capital S and not the more mundane pursuits and behaviors most non-scientific human beings focus their lives on – like the airmen.

The film assumes a man like Dr. Carrington will be passionate about science but otherwise unemotional and certainly not one to have physical feelings – behaviors we witness all too well between Captain Hendry and Nikki Nicholson, Dr. Carrington’s secretary. This almost makes him the human equivalent of the alien: Mentally superior, highly intelligent, aloof, and therefore potentially just as much a threat to the station and beyond as the alien, since Dr. Carrington seems more than willing to sacrifice all their lives in his single-minded pursuit of what he sees as a much higher and therefore better life form.

As the cinematic representative of Science and its practitioners, this stereotype is no fairer to the field and its professionals than the automatic assumption that a being from the stars is on Earth only for conquest and destruction rather than exploration and contact. This also goes for the film’s representation of the Air Force men, who are portrayed as being much more average in intelligence and far more interested in the baser pleasures of life that Dr. Carrington undoubtedly disdains. Their baseness includes the almost instinctual response to anything unknown with lethal force, especially an actual alien.

Even when the airmen were first on their way to investigate the crashed flying craft, which they knew almost nothing about before finding it, their general consensus was that the vehicle was probably of Soviet origin. For Americans of the early Cold War era, this could mean little else than a potential threat to their nation, whether it was a spy plane or something more elaborate like an experimental weapon. Worse, the airmen generally tended to blend into one another in terms of having any prominent individual characteristics.

Image: Our predetermined heroes on their way to meet their destinies near the North Pole.

In essence, everyone in The Thing is one level of stereotype or another, including the character of the film’s title. While this may be expected from Hollywood cinema, especially back in the day to use a phrase, it does have ramifications in terms of making audiences think certain ways, even if it is just reinforcing their already preconceived notions about certain types of people and concepts. Thus Science is represented by a man who is devoted to it and little else, be it biological urges or his fellow humans.

Oh, Dr. Carrington is constantly emphasizing how he wants the presumably superior knowledge of their visitor from the stars for all of humanity, yet he is not unwilling to endanger the lives of all the humans at the research station in order to communicate with the alien, including his own.

Dr. Carrington said the following declaration in the 1950 script draft, which was retained in a watered-down version of the final released film:

“Two of our colleagues have died and a third is dying. Those are our losses – and the battle has only begun. There will be more losses. The creature X is more powerful, more intelligent than us. We are infants beside him. He regards us as soft, vulnerable earth worms important only for his nourishment. He has the same attitude toward us as we have toward a field of cabbages.

“A new world has come to devour us. Only science can conquer it. Our minds, gentlemen – the little muscle that thinks, observes, examines and finds answers. All other weapons will be powerless.”

We get to the core of the filmmakers’ take on science as an amoral force in pursuit of its own agenda at the sake of all others during the following scenes when it is learned that Dr. Carrington is secretly growing the seed pods from the alien in the station’s greenhouse.

We observe more indications of the airmen’s views on science as amoral or at least indifferent to the safety and concerns of the wider world with this next bit of dialog from the 1950 film script draft. These scenes contain some extra useful details that did not survive into the released film, yet neither detract from nor drastically change what was shown on screen.

Dr. Carrington: “A secret has come to us, greater than any secret ever revealed to science. It must not be destroyed! It must be studied – and learned.”

Captain Patrick Henry (later changed to Hendry): “I saw it, Carrington. It’s not something to put under glass – and examine. And there are thousands more of them hatching. They’ll reproduce like weeds. They’ll tear the world apart.”

Dr. Carrington: “That doesn’t matter!”

Henry: “It kind of matters to me.”

Dr. Carrington: “Knowledge is more important than life, Captain. We have only one excuse for existing – to think, to find out, to learn what is unknown.”

Lt. Eddie Dykes: “We haven’t a chance to learn anything from that pookey Martian, except a quicker way to die, Doctor.”

Henry: “I’m ordering you back, Carrington.”

Dr. Carrington: “It doesn’t matter what happens to us! We’re not animals. We’re a brain that thinks! Nothing else counts, except our thinking. We’ve thought our way into nature. We’ve split the atom – “

Dykes: “Yeah, and that sure made the world happy, didn’t it!”

[Stage direction] The mewing [of the newborn aliens raised in the greenhouse] out of the wall speaker increases.

Henry: “I’ve ordered you out, Carrington.”

Dr. Carrington: “We owe it to the brain of our species to stand here and die without destroying a source of wisdom! Captain, I beseech you. Science, government, the Army – civilization has given us orders.”

Henry: “They’re wrong order[s]. They come from people who don’t know what they’re talking about.”

Reporter Skeely (later renamed Ned “Scotty” Scott): “I’m with you there, Henry. In a pinch I always put my money on a little man – against all top brass.”

Dr. Carrington: “You set yourself above all human progress, above all science!”

Henry: “I set myself against an enemy, Carrington.”

MacAuliff: “Come on, Doctor. You’ve said your piece. This is one time when science doesn’t blow up the world… just to see what makes it tick.”

Note in particular the mention by Dr. Carrington about splitting the atom as one of science’s greatest achievements and the airmen’s reactions to it. The two sides were juxtaposing the benefits of atomic energy for running our technological civilization against the destructive reality of the atomic bomb. This latter item was often viewed by the general populace as a creation by science without either thought or safeguards as to whether or not it should be made – even though nuclear weapons came into existence in the United States at the demands of the government for the military: First to force the Axis powers of World War Two to surrender (and simultaneously beat them at developing such a weapon before the Allies could) and then to “balance” geopolitical power with the Soviet Union and their Iron Curtain allies.

There was also a quick comment early on in the film that Dr. Carrington is “the fellow who was at Bikini.” This is a reference to Bikini Atoll in the Pacific Ocean, which was used for conducting multiple nuclear bomb tests from 1946 to 1958. The atoll was left uninhabitable for humans due to the excessive amounts of radiation from these tests. Some of its numerous islands were outright obliterated from the powerful nuclear explosions.

These tests were performed as a major aspect of the Cold War: The nuclear weapons were, ironically, created and meant to prevent yet another global-scale war by making the possibility of a nuclear attack so devastating to Earth as to be untenable to any rational and ethical person or nation.

That the Thing looks so similar to Frankenstein’s monster as mentioned earlier only adds to the perception of science as an amoral force that delves into areas beyond where humans are considered capable of understanding or meant to be there. While the initial reasons for the alien ultimately resembling the Universal Studios film version of Mary Shelley’s monster were both technical and financial, the underlying message taken from it may have been consciously taken advantage of once the filmmakers saw the end result.

Both sides in The Thing have their points in their takes on the alien: The military men were already afraid of this being from another world even when it was presumed dead and encased in the Arctic ice when they first discovered it. That it came from another world in a vessel with unknown technologies and therefore abilities (including the underlying possibility of carrying weaponry with a similar bent) were reasons enough for them to be on alert for the worst possible scenarios of this unexpected and largely unplanned for situation. When the alien turned out to be very much alive and became free of its ice prison, their fears became confirmed and they immediately and instinctively went into warrior mode.

Dr. Carrington pointed all this out to Captain Hendry:

“Captain, when you find what you’re looking for, remember it’s a stranger in a strange land. The only crimes were those committed against it. It woke from a block of ice, was attacked by dogs and shot by a frightened man. All I want is to communicate with it.”

Captain Hendry: “Fine, provided it’s locked up.”

Of course we already know the deck is stacked against the alien being benevolent or even neutral, which makes the pleas and plans by Dr. Carrington seem naive at best and just as dangerous as a direct assault on everyone there at worst. However, it is not the scientist’s fault that he is unaware of what the filmmakers had in store for their characters.

It seems a bit much for such an intelligent man, no matter how excited he may be about coming upon what would be considered the most important scientific discovery in human history, responding to Hendry’s warning that the alien’s progeny will “reproduce like weeds” and “tear the world apart” by exclaiming “that doesn’t matter!” Unless Dr. Carrington’s illogical outburst was a combination of disdain for the Captain’s much lower level of scientific knowledge and words borne from exhaustion and an anxiousness not to lose such a unique intellectual prize. Nevertheless, it is still both excessive and irrational, especially if Dr. Carrington wants to reveal the supposedly superior wisdom and technology of the alien to the whole of the human race for their benefit. Getting his entire species wiped out in the process would rather defeat the purpose.

I think it is safe to say that Dr. Carrington’s personality is one that does not contain any serious levels of sadism, masochism, or megalomania. He has an obvious ego, of course, but this is borne of multiple earned achievements from a life-long career in science, including the Nobel Prize. As a further indication of Dr. Carrington’s overall character, it is interesting to note that someone of his stature and renown is still out working in the field – in the remote Arctic, no less – rather than a much more comfortable and perhaps even more profitable academia equivalent of a desk job, or in the corporate world, or even with the military, for that matter. His devotion to science is, if nothing else, certainly not for show but a genuine passion.

The words put into Dr. Carrington’s mouth by the scriptwriters show their biases on science and its practitioners in general. This reveals a genuine real world fear of what they don’t quite understand. In an ironic but hardly unexpected contrast for the era, the filmmakers turn to and lionize the ones whose main tasks are to monitor the region for (usually) terrestrial threats and to deal destruction and death when the situation calls for it – or even when told not to take the offensive in the particular case of this film.

These “regular Joes” are the kind our popular culture likes to measure by the “test” of who you would want to have a beer with. Whether you would want to drink beer or any other kind of liquid with either these airmen or Dr. Carrington and his cadre of scientists depends upon what kind of conversation topics and activities you prefer.

The other social hierarchy test portrayed in The Thing is who would prefer whom as a relationship partner. As the film takes place in late 1950, this naturally involves the designated Alpha Male (Captain Hendry) and the most prominent woman in the film, in this case Nikki Nicholson, who as a “bonus” happens to be Dr. Carrington’s secretary in terms of adding an extra layer of dramatic tension. Whole scenes are dedicated to establishing that the two have a form of romantic past together and will definitely upgrade to a serious relationship in the near future once this annoying ordeal with the asexually reproducing alien menace is over.

Ms. Nicholson shows definite signs of sympathy and respect for her work boss, as she constantly has to remind an increasingly frustrated Hendry that Dr. Carrington’s continually stubborn and life-threatening actions are due to his being both overexcited by the presence of an actual living ETI and very tired from lack of sleep over this major scientific discovery. However, in standard Hollywood tradition, it is made quite clear who is going to end up with whom by the time the film credits roll, though the scientist shows no non-work-related interest in Nikki or anyone else, from this planet at least.

One last point on this topic: I was made to wonder if there was originally going to be more of a romantic rivalry between Captain Hendry and Dr. Carrington over Nikki Nicholson when I read the following introductory description of the head scientist from the 1950 draft script:

“At a large flat-topped table in the room sits Dr. Arthur Carrington. He is a man of 43 with an alert, cheerful face. He is good looking, well built, soft spoken. His dominant characteristic is a smile that seems never to leave his lips. It is present always on his face like an extra feature. He is a genius of science and a man whose brain is focused like a microscope on the secrets of nature. But the intensity of his preoccupation with science is not to be heard in the easy tones of his voice. It will be seen in the things he does, in his point of view – but never in his manner. Outwardly, he seems only a good looking man full of child-like enthusiasm for a task and with a soothing, amiable way for his fellow man.”

“Captain Henry stands silently in the doorway, his eyes moodily on his scientific rival. The doctor is studying the indicator dials of a complex instrument on the table. Bill Stone greets the arrivals.”

The final result for Dr. Carrington created a character who was indeed a rival for Captain Hendry, but in a manner rather different from the usual thematic pattern.

Putting Things in Perspective

Just as the appearance and actions of the alien did with the airmen at the research station, the rapid pace of science and technology after the Second World War frightened the general public, many of whom did not really understand such concepts as nuclear physics, except to focus on the fact that one version of it could annihilate the world in large enough quantities with little warning.

They also often understood the practitioners of science even less, except for what they saw portrayed in their entertainment media. The Thing did its level best to make Dr. Carrington the catch-all example of scientists as a whole through a somewhat distorted and not entirely cloudless cultural lens.

Had The Thing been produced after October of 1957, when the Soviet Union lobbed the first artificial satellite into Earth orbit called Sputnik 1, then Dr. Carrington may have instead been turned into the true hero of the story.

That 184-pound silver ball with four radio whip antennae trailing off its sides shocked Americans into the realization that if the USSR could make an object circle the entire planet over and over with one of their rockets, then they could just as easily deliver a nuclear bomb to any part of the United States in a manner of minutes using the same technology.

American authorities at multiple levels felt it had fallen behind in educating its citizens in the sciences and technology, particularly in regards to space. Almost immediately an overhaul of the nation’s education system began with an emphasis on those subjects to close up what they perceived to be a serious gap with and lag behind the Soviet (and therefore Communist) system.

Thus my prediction that had The Thing been produced after 1957, Dr. Carrington’s high scientific knowledge and enthusiasm would have gone from being a suspicious hindrance and danger to the group to become the very qualities that literally save the day. In the actual 1951 film, he did mention multiple times how science was the only real tool that could “defeat” the alien visitor, at least in terms of understanding and communicating with the being to hopefully avoid the outcome that ultimately unfolded.

As will be discussed in more detail later on, even though Dr. Carrington would fail to sway the alien with his preferred methods, the scientific knowledge he and his colleagues did provide from their examination of the extraterrestrial did give the airmen the knowledge they needed to bring down their adversary after their more traditional weapons fell short due to the alien’s unconventional physiology.

The Thing itself may also have been turned into a more sympathetic character if the film had been released once the Space Age had begun in earnest, rather than a largely inhuman antagonist. One example of this theme was given early on in this essay with the 1953 science fiction film It Came from Outer Space. Another example comes from a 1967 episode of the original Star Trek television series titled “The Devil in the Dark”. The ETI in this case is a being called a Horta, a large silicon-based organism that is essentially a living rock.

In a future interstellar society called the United Federation of Planets (UFP), there exists far below the surface of an alien planet in its territory labeled Janus 6 a being that calls itself a Horta. This decidedly non-humanoid life form looks like a large blob of molten lava and can move through solid rock with ease thanks to a highly corrosive acid it produces from its body.

As we learn early on, this Horta has been attacking and killing dozens of the human residents of a Federation mining colony stationed on Janus 6 without seeming provocation. The being’s physical appearance and behavior has left the miners convinced that it is nothing less or more than a dangerous monster acting on instinct towards the humans which cannot possibly be reasoned with. Therefore, the creature must be exterminated before the mining facility has to be abandoned, losing access to the planet’s great stores of valuable mineral resources for the greater Federation.

Starfleet, the quasi-military organization that conducts both exploration and defense for the UFP, is called upon to stop this threat and save the miners and their operation. At first the officers of the starship assigned to handle this situation, the USS Enterprise, are led to similar thoughts about the native life form when they encounter it deep in the planet’s dim caverns. They too think the Horta is a purely destructive force that needs to be eliminated before they are all killed by it.

However, a series of events convinces the starship officers that this “living rock” is actually a highly intelligent and sensitive being. Eventually direct communications are established with the Horta. They learn that this alien is a mother who was defending her eggs, which are the thousands of silicon nodules found by the miners throughout the vast network of tunnels and chambers far beneath the surface of Janus 6. These spherical objects were being casually destroyed by the humans during their mining operations, as they did not recognize the nodules as the biological product of an ancient and highly intelligent organism – the last of its kind, in fact.

The mother Horta naturally viewed these strange alien bipedal creatures invading her world and killing her unborn children as monsters and acted accordingly.

An understanding is reached between the two species: The young Hortas who later hatched from those surviving nodules would help the human miners find all sorts of mineral deposits and with much greater efficiency, ensuring both the survival of the Horta and the continuation of the UFP colony and its importance to the galactic civilization that spawned it. Both sides also learned to tolerate and accept each other despite their initial mutually visceral reactions to the other’s wildly different physiologies.

This famous episode of the Star Trek series and many other entries from that franchise add further examples to the premise that when it comes to humanity encountering the unknown Other, the situation does not automatically have to turn into an Us-Versus-Them battle for survival with only one winner arising from the conflict. Most often it is when one of the groups make a genuine attempt to understand and communicate with the other that a non-lethal resolution has a chance to happen, while not sacrificing the entertainment demands for action and drama in the process. Writing such stories also gives our species one more roleplay example to practice with and learn from for the day when humanity finally does meet with real beings from other worlds.

Now That We’ve Got Them Just Where They Want Us

“Right, now that we’ve got them just where they want us.” – Captain James T. Kirk, quoted in Star Trek: The Motion Picture (1979)

You have read throughout this essay that The Thing from Another World was biased towards its alien (and potential ETI in general) being hostile and threatening not only to the hapless crew at the remote Arctic research station, but all life on Earth. So how did a small collection of military men and scientists, who before encountering the crashed alien starship and its lone occupant would have considered the idea of beings from other worlds to be science fiction at best, if they contemplated the concept at all, suddenly become experts on the motives of such a life form? In particular, one that the humans had destroyed its vessel through their hurried ignorance of the ship’s composition and was clearly in no mood to convey any information about itself or its actions to such comparatively primitive and violent creatures.

The answer would seem to come from human intuition, which in the case of the film’s characters, the non-scientists had the upper hand on. The airmen, being trained in the ways of military thinking and having participated in combat in World War Two just half a decade earlier were suspicious of the alien from the moment they learned that the “aircraft” the research scientists detected showed unusual flight behavior.

This was the early height of the Cold War. The airmen would have been stationed in Alaska as part of the United States presence to monitor the relatively nearby Soviet Union across the Bering Strait. They would also be there to dissuade their geopolitical rival from deciding to occupy such close American territory (Alaska had been part of the United States since its purchase from Russia in 1867, but it would not become an official state until 1959) or engage in even more elevated military actions on a larger scale.

The Korean War was also underway when The Thing took place: There is no mention of that conflict or that these men were directly involved with it. However, this early major “police action” of the Cold War heightened real world fears that things could expand beyond the Korean peninsula and trigger a nuclear response. Assuming this event was also occurring in the reality of the film, our military characters would be on alert to respond to any type of activity deemed suspicious – at least the terrestrial kind.

As noted earlier, the soldiers assigned to guard the alien while it is still in the block of ice are terrified of its appearance, with its “crazy hands and no hair” – although if the filmmakers had been able to make the alien look more like the description of the Thing in the founding 1938 story, they might have really had something to be terrified of. They can only assume anything which they see as frighteningly ugly is therefore also automatically dangerous with evil intentions.

Image: Dr. Carrington and his fellow scientists of Polar Expedition 6 studying how the Thing reproduces in the greenhouse of the Arctic research station.

Once the alien has responded to being shot by the guards and attacked by the sled dogs and then it is discovered that it uses blood for nourishment and can reproduce asexually via seed pods, it is Dr. Carrington’s secretary, Nikki Nicholson, who voices a theory as to why the alien has come to Earth in the first place.

Nikki has this discussion with her boss, which has been taken from the 1950 draft script as it adds some useful details which were left out in the final film version.

Nikki: “You’re not thinking of what’s happening in the greenhouse. You saw what one of them can do! Well, just imagine if there are a thousand, or a hundred thousand!

Carrington: “I have imagined it.”

Nikki: “And you won’t do anything?”

Carrington: “I’m doing all that can be done, Nikki – discovering its secrets.”

Nikki: “I know! And that’s quite wonderful. But what if that ship came here not just to visit the earth, but to conquer it! To start growing some kind of a horrible army. And turn the human race into – into food for it! And kill the whole world.”

Carrington: “There are many things threatening to kill our world, Nikki. New stars and comets shooting through space. Atmospheric changes. A sudden cooling of the sun. And even human wars – that may release deadly global gases.”

Nikki: “But those are theories, Arthur! This is an enemy – near us – and – “

Carrington: “There are no enemies in science. There are only phenomena to study. We are studying one.”

Nikki: “You’re not afraid?”

Carrington: “I’d be a traitor to human reason if I allowed my fears to destroy what has come to us – or let anyone else destroy it. I want you to believe in my way, Nikki – the way of the mind.”

In the dialogue where Dr. Carrington is describing other possible threats to humanity, he is more on target than they probably knew in 1950. We now know better than ever how dangerous a rogue comet or planetoid could be to Earth if one impacted our planet (the idea of one wiping out the dinosaurs 65 million years ago did not gain wide scientific acceptance until the early 1980s). Climate change and industrial pollution have certainly played a role in causing major changes to Earth’s atmosphere, not to mention the rest of our planet. If nothing else, it would be difficult for Nikki to casually cast off the idea of human wars creating deadly gasses and other weaponry that could threaten our species as just a theory, in both her time period and ours.

This dialogue also lends credence that while Nikki may be right about the alien at the research station being a real and immediate threat at least to them, in the wider context of the whole debate about the intentions of any actual ETI, natural objects in nearby space and certain real humans on Earth have much higher chances of causing disaster and death for us than beings for whom there is still no solid evidence of their existence, let alone their intentions.

In regards to Nikki’s declaration that the alien has come here to create “some kind of a horrible army” and use terrestrial life as a source of food, her response undoubtedly came from the fact that the alien can and did reproduce rather rapidly by producing seed pods from its body, then feeding the developing young inside them with human and dog blood.

The film bends us to think that Nikki’s speculation is the true intent of the alien. To take a page from Dr. Carrington calling upon real terrestrial examples of plant life that can seem to behave like animals, it could also be that the crash-landed and stranded alien might have been trying to preserve, if not its actual self, then its genetic material.

This scenario reminded me of an event that I personally witnessed when I once went salmon fishing with my family. I discovered that male salmon, when caught and pulled out of the water, do something which rather surprised me: The males shoot out a stream of sperm in what can only be described as a last ditch attempt to carry on its genes, desperate and hopeless as this gesture may otherwise seem (the things they do not tell you in most nature documentaries).

This action is very likely not a conscious response in the fish’s case, but rather an automatic survival reaction similar to the famous fight-or-flee response to danger. Perhaps the alien was doing something similar, even though of course it would have been aware of its purpose in producing seed pods. Highly intelligent and advanced or not, the alien still had basic instincts like all living creatures and acted upon them – with the survival of itself and its species no doubt being on the forefront of its list of important activities to conduct.

You could say this too is just speculation, but then again so is Nikki’s, lacking any direct confirmation or denial from the alien itself. Dr. Carrington was not wrong when he said communication is key to understanding.

Nikki, the lone major woman character in The Thing (there was one woman scientist at the research station, the wife of Dr. Chapman, but her role was small) had yet another collection of expressed thoughts in regards not just to their alien “visitor” but about the idea of ETI coming to Earth in general.

This conversation comes from the released film when the alien is still considered to be a dead specimen frozen in that block of ice:

Nikki: “What does that boogeyman in ice really mean?”

Hendry: “I don’t know, Nikki.”

Nikki: “Well, does it mean that we’ll have visitors from other planets dropping in on us? Do we have to return the call, or… Oh, jeepers.”

Hendry: “I know. Yesterday I’d said it was crazy.”

Nikki: “I’d say it’s crazy now.”

Hendry: “Forget it. Tomorrow it’ll all seem different.”

Nikki’s facial expressions and gestures during this scene make it clear that she is not very enamored of the idea that extraterrestrial beings may now be coming to Earth on a regular basis and that humanity might actually have to talk to and associate with them. The very idea itself is not one she or her companion Hendry ever took seriously until they personally found that alien ship and its living occupant in the ice. It is safe to say that these two and the rest of the non-scientists at the station have little interest in ever joining any type of Galactic Club, should one exist.

The scene itself seems mild, an almost casual conversation about a subject that would have been esoteric if not outright embarrassing for our two characters just the day before. That it is such a simple, short, and straightforward “evaluation” of the idea of ETI contact only makes it that much more palatable to the audience, who are continually conditioned to root for the “alien-is-bad” line of reasoning and its mouthpieces.

It is also interesting to note that it is Nikki who first comes up with the idea of how to dispatch the alien after bullets and even cruder methods have failed. While she and the airmen are speculating on how to stop their unwanted guest, someone asks what does one do with a vegetable. Nikki responds with: “Boil it. Stew it. Bake it. Fry it.”

This idea spark leads the men to attempt to burn it to death by dousing it in kerosene then setting it aflame. When that effort fails (in a scene that quite frankly looks like it had the potential to turn deadly for the cast and production crew in real life), they then try an electrical trap, which does succeed.

Image: The Thing as it is about to walk into what the human protagonists hope will be a successful trap to stop it from turning them all into dinner.

No one outside of Dr. Carrington even ventures the idea of communicating with the alien in any way; they only want the creature killed or otherwise destroyed by some method of brute force. The airmen did make some earlier vague suggestions about confining the alien after it escaped the ice block, which is what their superior officers wanted to be done with it, but even capturing the alien alive goes out the window once the danger of the situation escalates.

Another piece of speculation on the alien and its motives that was in the 1950 script draft but removed completely for the final film were its reasons for landing at the North Pole as opposed to anywhere else on Earth.

The scientists first speculate that the alien came from a world that was generally colder than Earth with a thinner atmosphere based on such things as its seeming lack of ears for hearing sounds (they guess that the being “receives magnetic impressions” rather than hearing and seeing as humans do, even though it definitely has eyes that appear and act like ours) and the way it can survive out in the Arctic snow storm even after it has been presumably injured multiple times and with only a thin type of coverall on its body. Also, in the final makeup form of the Thing, the being definitely has human-shaped ears located on either side of its head.

Then they and Captain Hendry come up with some ideas as to why the alien would choose to land in the frigid and desolate Arctic, presuming it did not arrive there by accident due to some technical issues with its ship:

Voorhees: “It ran out into the cold. I think our surmise that it requires a cold temperature is correct.”

Laurenz: “Obviously. That’s why the saucer tried to land in our Polar regions. They corresponded to the conditions of its own planet.”

Hendry: “There might be another reason. Its passengers could have wanted to keep their arrival secret.”

Note how the scientists are thinking about the alien’s motives based on its physiological needs first, as if it were here only to explore. Captain Hendry is thinking in terms of its strategic motives for conquering the planet. Of course the scientists could argue that the alien would want to remain hidden from humans in order to study us without causing any disruption, just like human scientists study animals in the wild using blinds and other means of camouflage in order to witness and record the true behaviors of their subjects.

On the other hand, the remote Arctic may not be the best place if the alien wanted to find a large quantity and cross-section of humanity. For that matter, the alien (and any cohorts aboard that spaceship) could have stayed in Earth orbit and monitored us remotely if exoanthropology were among its motives.

As The Thing takes place and was made years before the first human-made satellites were sent into space, attempting to watch our activities from hundreds of miles above our planet’s surface or more may not have been taken into serious consideration at the time, being thought of as too remote to learn anything useful.

In addition, the idea of sending unmanned vessels using Artificial Intelligence (AI) to explore space and other worlds, instead of ships with living, organic crews, would have been another fairly novel concept at the time. Yes, by 1951 several nations were using unmanned V-2 rockets captured from Nazi Germany at the end of World War Two to carry cameras and other basic instruments on brief forays to the edge of space. However, the idea of “marrying” a complex computer with a launch vehicle would have been difficult at best: A typical “thinking machine” circa 1950 was very expensive, had weight ranges measured in the tons, and filled up a large room. Miniaturizing computer technologies to fit inside a spacecraft on top of a rocket were another concept that would have to wait for the real Space Age to begin on Earth.

Of course the alien may have detected the electromagnetic signals (radio, television, and radar) being leaked from our civilization as a motive for coming to Earth. His species may also have been able to detect our planet’s multitude of biological life signs, which could be accomplished as far away as their home world using an advanced form of spectroscopy.

While we know the plot scales are tipped in favor of a malevolent reason for the alien being on Earth, the previous examples show it could still have come here for purely scientific exploration, its landing near the North Pole an accident as much as a planned place to study us without disturbing the natives.

Dr. Carrington may have taken the more rational and peaceful approach towards the alien, but that did not mean he was without his own biases. As we have seen multiple times over, the lead scientist insisted that because the alien arrived on Earth via a starship, it was therefore much more knowledgeable about science and technology and therefore it must be automatically wiser – with the implicit addition that the being was therefore also more ethical and moral. In addition, Dr. Carrington was rather swept away by the fact that the alien did not reproduce via “messy” sex. For him this was yet another sign that the alien came from a superior species.

As we have seen on Earth, a technologically advanced human society does not automatically indicate a kinder and gentler populace. As history has shown, it often means that the nation or culture with the better technology is simply more efficient at subduing and even wiping out any opposition. Either that or subjugating less powerful and sophisticated groups for their land, resources, and other items that might increase their position.

Even for species that do not possess any real technology, a higher-functioning brain does not therefore mean they will be necessarily more ethical or even just “nicer”. Dolphins are among the most intelligent creatures on Earth, with brains perhaps comparable to humans. Yet certain types often behave within their own species and others in ways that, were they members of human society, would immediately label them criminals.

This analysis does lead into questions of how one can (or should) judge a non-human species by human standards of behavior, especially when even humanity is often divided on what is considered to be moral and ethical, good and bad. If the alien in The Thing did come here to propagate its species on a new world, how is it different from all the organisms on Earth that have competed with other terrestrial creatures for dominance on this planet since their first microbial ancestors appeared over four billion years ago?

Imagine a situation where Earth was becoming uninhabitable for its native organisms: Would it be considered wrong for humanity to seek out another world in the Milky Way galaxy to continue ourselves and whatever other terrestrial life forms they could bring with them? What if they found a suitable world to colonize that was already occupied by its own flora and fauna, including species deemed intelligent enough to compare to humanity? What if the natives of that planet did not want any new neighbors, yet our species’ survival depended upon settling their world? Who would be in the right: The original occupiers of this planet? The would-be human colonists? Or the species that may end up best dominating that globe?

Suppose the alien in The Thing came to Earth because their world could no longer support them? Would they have any less of a right to inhabit our planet to survive than we would if we needed their world to sustain our species? Even if a species had deliberately wrecked their own world through neglect, greed, or war so that their only other choice was extinction?

Evolution is often thought of by the rule of survival of the fittest. If the species of the alien in The Thing is more suited for surviving in this Universe than humanity – and its ability to withstand extreme environmental conditions and various trauma that would dispatch a typical human in short order was witnessed multiple times – does its kind deserve to overtake the stars?

Humanity has certainly considered itself the predominant life form of Earth for ages, even to the point of proclaiming our species was divinely ordained to rule over the planet and utilize its other organisms and resources as it sees fit, since they were presumably placed there specifically for humanity. It is hardly impossible to imagine that such an egocentric view might not be unique to our species across the stars, as dominating cultures rarely think less of themselves as a whole or tend to shy away from gaining more territory and power when the opportunity arises.

If the plot situation in The Thing from Another World had been reversed, where a team of Terran military personnel found themselves on a starship that crash-landed on the world of the alien from the film: Who would the audience be rooting for as the humans undoubtedly would do their very best –indeed, whatever they had to do, if necessary – to survive on a world where the life forms would very likely react to their presence in a manner quite similar to how they reacted to the alien, especially once it had been revived and free in the Arctic research station?

Furthermore, if these humans went so far as to attempt to secure their survival by becoming the new dominant species on that alien planet, either subjugating the natives or snuffing them out, would not many consider them to be brave and audacious heroes, especially back in the era of The Thing’s first release. These humans would see the military men as warriors protecting and preserving the galaxy from dangerous aliens for our species.

That was certainly the theme in the 1997 film Starship Troopers, where a future fascist humanity is on a quest to rid the Milky Way of a nonhumanoid alien species they derisively nickname the Bugs. The few public calls to consider the situation from the Bugs’ point of view, including the possibility that we may have invaded their celestial territory first and thus their hostile response, are quickly dismissed and quelled. The leader of the Terran Federation, Sky Marshall Diennes, brings home the government’s position during a broadcast speech: “We must meet this threat with our courage, our valor, indeed with our very lives to ensure that human civilization, not insect, dominates this galaxy NOW AND ALWAYS!”

Here was Manifest Destiny taken to a stellar level. The film brings up the possibility that instead of an ETI civilization being the conquering aggressors bent on dominating the galaxy so often seen in science fiction, it could be humanity which becomes the “alien” invaders to be feared and despised by other societies across the stars.

This leads to another pertinent issue that was also tipped in favor of the human characters: Who and what would be considered either good or evil, or are these largely human judgement values that become increasingly parochial when compared on a literally cosmic scale? We naturally gravitate towards the idea that if something is beneficial to our species it is therefore good, whereas anything harmful is deemed bad or worse.

However, then how does one define something like a virus, which might be deadly to humans, yet we know that they act as they do with neither purposeful ill intent nor even a consciousness. They exist to make copies of themselves, just like virtually all known species do, just on a much more rudimentary – although certainly highly efficient – level.

Now take this perspective to a galactic scale: What if humanity or other similar types of intelligent biological life forms that may attempt to colonize the Milky Way galaxy are perceived by ETI of a very different makeup or are similar to a Kardashev Type 3 civilization, one that spans and utilizes the resources of an entire stellar island like the Milky Way, just as we generally look upon viruses.

We would not tend to see our interstellar expansion as a spreading disease because we have yet to become fully and truly conscious as a culture of the literally much wider picture. After all, humanity and the single planet it currently occupies at present are virtually microscopic in comparison to the rest of the Cosmos. Yet such a lack of cosmic awareness may not spare us from the more advanced ETI’s response to what they may well see as a form of virus infecting their society’s “body”.

Recall the quote at the beginning of this section from the 1979 science fiction film Star Trek: The Motion Picture: That first cinematic installment of the Star Trek franchise dealt with the mostly-human crew of the starship Enterprise encountering a vast alien being calling itself V’Ger. This ETI hailed from (though not originally) a planet occupied by “living machines”, also known as Artilects, or artificial intellects.

As a result, V’Ger perceived the Enterprise as a fellow living being, albeit much smaller and far less sophisticated, whereas the multiple organic creatures it found inside the vessel were labeled as “carbon units” and therefore were “not true lifeforms” so far as V’Ger was concerned. The artificial alien further thought these carbon units were actually infesting the starship like a disease, keeping it from properly functioning and undoubtedly a threat to its overall existence.

Obviously the scenario with V’Ger is a fictional one, but how often have humans dispatched other organisms they do not consider to be their equals – which is just about everything else on this planet – not only with little to no consideration, but also with the thinking that their duty to remove creatures they consider to be harmful or worse to their fellow humans.

For that matter, how often have humans committed acts of genocide against other human beings, often due to little more than minor differences in appearances and customs? There is usually a justification made for such aggressions; even slim ones can be enough to behave in ways that on an individual scale would be considered nothing less than assault and murder.

Image: The human denizens trapped in the Arctic research station prepare for their final confrontation with the Thing.

Now imagine how contemporary humanity might respond to beings that are truly alien to our world in virtually every way, and vice versa. The results may well be what we have seen in The Thing, with fear and aggression winning out over reason, logic, and overtures of peace, or at least neutrality.

At the end of The Thing, with the alien threat safely eliminated, we find the reporter Ned “Scotty” Scott finally able to broadcast his incredible story to the outside world via radio. Here he beseeches his listeners to tell “everybody wherever they are: Watch the skies everywhere. Keep looking. Keep watching the skies!”

While one can appreciate this warning from the reporter in the context of his reality’s encounter with an ETI, one may also imagine the heightened levels of paranoia and fear that will now be growing in that human society over anything foreign appearing in Earth’s skies. Authorities will be flooded with reports of unidentified flying objects beyond the already voluminous amounts of such sightings that already existed at the time: Some sighting stories will be legitimate and useful additions to the UFO database, but many more will be either misidentifications or outright hoaxes. Throw in a Cold War that was also a hot one in certain parts of the globe, and it will likely be only a matter of time before someone shoots down a non-hostile terrestrial aircraft, mistaking it for yet another alien invader.

Then there is the possibility that the next visitors to Earth will be either peaceful or at least neutral explorers, or have other motives for traveling here that may either benefit humanity or cause no real harm, if nothing else. All that may change and become a self-fulfilling prophecy if the military panics and attacks them without provocation. Or civilians could fall victim to a mob mentality and conduct equivalent harm on anyone who is not a terrestrial native, or at least attempt to cause their demise. This attitude could even extend to other humans who show any form of support or even sympathy for those do not come from Earth.

This is why we should not and cannot leave the “discussion” about alien life and its possible motivations to science fiction media, be it from over half a century ago or now. I have often said that the general public gets its “education” about the world and various concepts from the films, television programs, and written works produced by our cultures. They often tend to take these messages to heart, whether they are accurate or not.

Some try to dismiss such media as merely harmless entertainment designed purely for profit – “it’s just a movie,” as they like to say. Yet if one is presented with a work that involves thousands of people and multiple industries to create, costs many millions of dollars to produce, and has numerous deliberate messages implanted throughout for its audiences, then it is most definitely not mere entertainment.

The Thing from Another World falls squarely into this category, despite looking like a more-or-less typical monster horror film of its day. That The Thing does look so “harmless” on its surface makes the fact that it is so biased against rational science over a more warlike stance all the more problematic. How many could honestly walk away from this film and not sympathize and side with the protective and friendly airmen over the emotionally aloof Dr. Carrington and his cold logic, even though most of his scientist colleagues at the research station did not share his fanatical attitude towards the alien, no matter where your preferences usually lie?

This is why the professional science community needs to really ramp up both their science education and outreach with the general public on the subject of alien life and the possibilities for and consequences of contact. While we cannot know how, when, where, or exactly why this event may occur one day, we can at least attempt to prepare ourselves and our species.

Being armed with knowledge and not just weapons may make all the difference, especially since it is just as plausible that our first real experience with an ETI may not resemble what Hollywood and other science fiction works have come up with – which in many cases is a good thing for our species, seeing how often they focus on malevolent aliens.

Should the science community fall short in providing the public and non-scientific authorities with guidance in this arena if a contact scenario goes awry due to the actions or inactions of either parties, scientists may find themselves being thought of and reacted to in the same way the airmen and the film audience did with Dr. Carrington.

The science community also needs to work together and push for improved methods to detect extraterrestrial life in all its possible forms. This means both an increase in SETI and METI efforts and exploring other star systems directly with interstellar vehicles. Breakthrough Starshot has made notable opening efforts in all of these areas, bringing awareness, respectability, and proper funding to fields that were often treated as either mere academic exercises or ridicule by much of the professional community.

Nevertheless, we need to be cautious about any singular organization being representative of the whole arena. Until the late 1990s, most American SETI efforts were dominated largely by radio astronomers with only token responses allowed from other fields, including ones that should have been equally as prominent considering the subject matters involved.

As a result, SETI projects in those otherwise pioneering days were focused on listening for radio transmissions from beings dwelling on Earthlike exoplanets circling yellow dwarf stars. Interstellar travel was largely dismissed as either very difficult or impossible to achieve, discrediting the concept of UFOs as alien vessels in the process. In other words, they were looking for versions of ourselves, even though other authorities and other nations involved in the SETI effort, like the Soviet Union, said that the evolutionary odds of alien beings resembling and behaving like us were slim.

Hollywood went on to reinforce this notion of aliens either appearing or at least acting like humans, often if for no other reason than the early science fiction films and television series could neither afford nor do expensive and elaborate nonhumanoid costumes and makeup.

For the fascinating and often otherwise untold history of SETI and astrobiology, please read this online thesis by Mark A. Sheridan:

http://www.daviddarling.info/encyclopedia/S/SETI_critical_history_contents.html

The Moment of Dr. Carrington

Throughout most of the events in The Thing, Dr. Carrington has been made to come across either as a naive fool at best (he and his fellow scientists were described as acting “like kids drooling over a new fire engine” in their initial reactions to the alien) or tantamount to working with the Thing against the best interest of his own species.

Even near the end, when the airmen had set up a way to electrocute the alien into oblivion, Dr. Carrington attempted to stop them by shutting off the station’s generator powering the trap and threatening them all with a revolver if they tried to turn it on again. The scientist was quickly subdued and hustled into another room for his own safety as much as theirs.

Then the unexpected occurs: Just as the alien is walking towards the airmen, brandishing a long wooden board as a weapon for the final standoff, Dr. Carrington suddenly emerges from behind them, bursting through the group and running straight towards the alien!

The scientist moves right up to the alien and stares into its face. Probably as astonished as the airmen are by this brazen act, the intruder stands still long enough to hear Dr. Carrington plead the following directly to it:

“I’m your friend. I have no weapons. I’m your friend. You’re wiser than I. You must understand what I’m trying to tell you. Don’t go farther. They’ll kill you. They think you’ll harm us. But I want to know you, to help you. Believe that. You’re wiser than anything on Earth. Use that intelligence. Look and know what I’m telling you. I’m not your enemy. I’m a scientist who’s trying – “

Whether the alien truly understood anything Dr. Carrington was saying to it is debatable. However, it may not have mattered, as the alien decides it has had enough of this babbling member of a race that has done nothing but try to kill it: With one swing of its arm, the alien violently knocks the scientist across the corridor, where Dr. Carrington lands on the floor unconscious.

The Thing continues on its menacing path. As the alien steps into the trap, the airmen now give their own “speech” to the intruder: Thousands of volts of electricity, which burn into the being from three different angles. Screaming and flailing about, the alien slowly shrinks until it is nothing but a pile of smoldering ash. The research station – and humanity – are saved from the menace from outer space. This time.

Image: The Thing meets its shocking end at the hands of the United States Air Force.

After this it is clear that the airmen and the reporter now have a new level of respect for Dr. Carrington that before was only inclined towards his higher education and intellect compared to theirs, along with his prestigious reputation in the scientific community. Right or wrong, the scientist had proven that he was willing to put his own life on the line for what he believed in, doing something none of the others would have dared to attempt unless cornered – and certainly not unarmed!

When Scotty is giving his news report to the listening world via Anchorage, he informs his audience that “Dr. Carrington, leader of the scientific expedition, is recovering from wounds from the battle.” The scientist had received “a broken collarbone and a headache” from his one and only direct meeting with the alien. Captain Hendry gave his tacit approval by quietly responding with “Good for you” to Scotty.

This is a strong contrast to what the filmmakers had originally planned for Dr. Carrington’s final scenes. In the 1950 draft script, the climactic action and dialog largely parallels the released cut, including Dr. Carrington running up to the alien unarmed and attempting to appeal to the being’s presumably superior and therefore better nature.

However, when he pleads “I’m not your enemy – I’m a scientist – a scientist!” the following occurs:

“The Creature has paused before Carrington’s tirade as if studying him. Now, without haste, it lifts one arm, and flicks its hand at Carrington’s throat. Carrington falls to the floor almost decapitated, his last words still gurgling in his throat. The Creature steps over Carrington’s corpse and enters the tunnel. It advances five or six steps.”

In the draft script, the alien is destroyed by the electrical trap, disintegrating in essentially the same manner as it would be shown on screen. The surviving humans’ reactions regarding Dr. Carrington, however, are something rather different:

Nikki: “Dr. Carrington – what happened to him?”

Hendry: (quietly) “He’s dead.”

Skeely (Scotty the reporter): (to Henry. Kneeling over Carrington’s remains) “A clean sweep, Captain. Both monsters are dead.”

In this earlier version, Dr. Carrington is killed outright by the alien, and rather gruesomely at that. Instead of being considered brave and therefore receiving a degree of new understanding, respect, and forgiveness for his previous actions and words, the scientist (and by proxy his profession and field) is lumped in with the alien as just another type of dangerous and non-human creature in need of destruction by the brave, relatable, and very human American airmen.

Not only does this alternate turn of events leave an unpleasant feeling, especially if you were not anti-science, anti-rational, and anti-ethical to begin with, but it removes any chance of even a glimmer that The Thing was not entirely on the side of the military and their warrior stance. I will even go so far as to say that had those scenes of and about the demise of Dr. Carrington been filmed and left in the final cut, they would have diminished the opportunity for The Thing to rise above being a straightforward Grade B horror flick.

Thankfully, someone decided that Dr. Carrington was not a monster, at least certainly neither a real nor metaphorical one. As a result, not only did they give the scientist a chance to show that he was a brave and determined warrior in his own way, but also that there was at least some room for more than one viewpoint when it comes to encountering the unknown.

Dr. Carrington’s on screen life may also have been saved because the graphic nature of his initially planned demise may have been deemed too brutal for 1950 audiences. Or that they did not have the special effects budget for it. Or both.

That The Thing left the door open a bit for the scientific angle of humanity dealing with alien life is good. Science is going to be at on the front lines in any event when the day comes that our world does discover extraterrestrial beings, no matter what fashion that historic occasion takes. Civilian and military authorities, and certainly the general populace, will be turning to science and its practitioners for answers to satisfy their curiosity, but even more so to alleviate their fears.

Should the alien(s) turn out to be hostile or otherwise nonbeneficial to the welfare of life on Earth, science will be necessary to provide solutions on how to deal with the threat(s). In The Thing, it was the scientific examination of the alien’s severed arm by the research station scientists that determined the physical makeup of the being and ultimately how to defeat it. The scientists also helped the airmen and reporter overcome their incredulousness at the concept of an intelligent plant capable of conceiving, building, and flying a starship.

This is why in the end it made sense that the chief scientist would be the one to confront the Thing from another world directly, and in a manner decidedly different from the quite predictable ones the airmen had set up for the being. There had to be at least some balance and fair play at some point; otherwise, what the 1950 film draft wanted would have left all of the human characters no more redeemable than the alien who was made to be a monster from the start.

Here is a what-if thought: What if the alien had really listened to Dr. Carrington and heeded his words, stopping his attack on the station personnel? Would the airmen have also stood down? Would the alien have waited for the authorities to arrive and gone with them, probably to be intensely questioned and examined before being detained indefinitely?

In light of what we already know about The Thing, these alternative scenarios all seem rather unlikely, but they are interesting to ponder just the same. If they did happen, we would have had a very different film, perhaps even a sequel at that. Even more importantly, we would have had a form of roleplay for the possibility of dealing with an actual ETI coming to Earth to learn from our species and vice versa, something science fiction can be rather good at, when its various authors can remember to keep at least some legitimate science in their plots. We might also have had a relatively rare chance for an early example of truly thoughtful and even literate science fiction cinema, from a Hollywood “monster” movie no less.

Doesn’t Every Alien Drive a Flying Saucer?

The Thing from Another World reflects another perception of alien life that evolved in the post-World War Two and early Cold War era: The surge of reports on Unidentified Flying Objects (UFOs), also known as flying saucers. The latter term came from comments made by Kenneth Arnold, the man who is credited with the first modern era UFO sighting in 1947.

After that landmark and widely-publicized event, sightings of strange craft seen moving about the sky and even more elaborate related stories increased exponentially. It soon became accepted on a cultural level that these objects were the vessels of highly intelligent alien visitors coming to Earth to study and interact with humanity, despite having primarily just eyewitness accounts for evidence.

There were so many UFO sightings in those days, in fact, that the USAF set up a department to document and study this phenomenon. What would one day become best known as Project Bluebook, which lasted from 1952 until 1969, originated as Project Sign in 1947 and then evolved into Project Grudge just two years later.

Project Sign’s final estimate on the UFO phenomenon was officially stated as inconclusive, although it had initially determined that these objects were real and likely extraterrestrial in origin. Air Force officials rejected those first claims on the basis of a lack of physical evidence and dissolved Sign. Its replacement study, Project Grudge, determined that most reported UFOs were either hoaxes or misunderstood natural phenomenon, although they admitted a certain percentage could not be explained conclusively.

Image: The moment the humans realize the crashed “aircraft” was not a product of their species.

The time period that events in The Thing take place – November 2 and 3, 1950 – put them smack in the middle of the Project Grudge era. There is a scene when the alien has first been found in the Arctic ice and the airmen are putting it aboard their airplane that one of them informs Captain Hendry – with full irony given their current situation – that a recent bulletin from the Department of Defense (DoD) declared that…

“The Air Force has discontinued investigating and evaluating reported flying saucers on the basis that there is no evidence.”

“The Air Force said that all evidence indicates that the reports of unidentified flying objects are the result of:

“One: Misinterpretation of various conventional objects. Second: A mild form of mass hysteria. Third: That they’re jokes.”

Dramatically, this sets up the audience to react based on the general public’s tendency to be suspicious of and often outright reject certain declarations from those figures in authority. Even the airmen, who are trained to obey their military superiors, make more than a few disparaging remarks about the capabilities of their higher ranking officers and the Air Force organization in general throughout the film. The airmen also have a level of disdain for the authority of science, particularly with Dr. Carrington as their chief representative science scapegoat.

This attitude ties in with the earlier theme in this essay about the built-in biases of the film regarding science’s take on alien life and how the response from the military in the form of our airmen heroes is made to be the “right” one. It is a reflection of our base fears of the unknown and how our more instinctual emotions take over and tell us how to respond to them.

The scene is also very likely an ironic comment on what happened when the film’s co-producer, Howard Hawks, asked the Air Force for assistance in making The Thing. They were turned down, as the head officials felt that their public cooperation with the film would contradict the military branch’s official stand on UFOs, which thanks to Project Grudge meant that they were anything but spacecraft from other worlds with alien occupants, friendly or otherwise.

These aspects of ourselves have not changed despite progress in other areas of science, technology, and cultural awareness since The Thing was released. The film also shows how the cinema can both reflect and influence our thinking and that such media are more than “just a movie.”

As for the film’s comment that the USAF no longer had any interest in UFOs and related phenomenon, the truth in our reality is that they continued to investigate them officially through 1969 with the aforementioned Project Bluebook.

The original intent of this study was to determine just what UFOs were and why they were acting as they were reported. The Air Force also wanted to know if these objects posed any threat to the United States. There was also an underlying motive that if some of these things were actual vessels of some sort, be they of Soviet origin or elsewhere, that the continual study or even acquisition of one of them could be a boon to our knowledge in the fields of technology, engineering, and physics – with perhaps some biology thrown in as a bonus.

Project Bluebook would eventually conclude the following:

1. No UFO reported, investigated, and evaluated by the Air Force was ever an indication of threat to our national security.

2. There was no evidence submitted to or discovered by the Air Force that sightings categorized as “unidentified” represented technological developments or principles beyond the range of modern scientific knowledge.

3. There was no evidence indicating that sightings categorized as “unidentified” were extraterrestrial vehicles.

If you think these statements from the USAF made in 1969 ended the public interest in UFOs or the view that they are the vehicles of alien visitors from beyond Earth, guess again. The plot elements of an alien being arriving on Earth in a flying saucer-shaped interstellar spacecraft certainly did not stop with The Thing, as both the real UFO phenomenon and this genre of science fiction both fed off each other and grew. Whether it helped or clouded the issues surrounding extraterrestrial intelligences and their motives can be debated, but they are a prominent part of the equation for human thinking on the subject nonetheless.

Image: The only real glimpse we get of the Thing’s mode of interstellar transportation, before the starship is inadvertently destroyed during its recovery effort.

The Thing from Another World was certainly not the only science fiction film influenced by the growing UFO phenomenon in that era. Just five months after The Thing was delivered to theaters, another effort called The Day the Earth Stood Still made its debut.

This film involved a humanoid alien named Klaatu and his robot “companion” Gort, who came to Earth in a silvery flying saucer starcraft, landing on a baseball field in Washington, D.C.. Like The Thing, the alien was shot by a panicky human soldier shortly upon leaving his vessel. However, this time a bloodbath did not promptly commence and Klaatu was promptly taken to Walter Reed General Hospital as it was known until 1951 to recover.

The Day the Earth Stood Still further veered away from its predecessor when it is revealed why Klaatu and Gort were sent to our planet: They are part of “an organization for the mutual protection of all planets – and for the complete elimination of aggression. A sort of United Nations on the Planetary level….” This is quoted from the revised final draft of the film dated February 21, 1951.

This interstellar organization has devised a system of sophisticated robots such as Gort which patrol the galaxy and respond decisively to any barbaric societies that might take their aggressive ways into space. Humanity has been recognized as one of these potentially dangerous species, thus Klaatu’s mission to Earth to warn its primate inhabitants that while they do not care what humans might do to each other or their home planet so long as they stay there, if we “threaten to extend your violence, this Earth of yours will be reduced to a burned-out cinder.”

Klaatu leaves humanity with these words:

“Your choice is simple. Join us and live in peace. Or pursue your present course – and face obliteration. We will be waiting for your answer. The decision rests with you.”

This time it is not the aliens who are the aggressors, except in potential self-defense, but the humans who have not ended their tribal warlike ways and now possess the ability to send nuclear weapons into space. Whereas The Thing was primarily a cheerleader for the American side of the Cold War and its warrior caste, The Day the Earth Stood Still is a blatant warning to stop the very real concept of Mutually Assured Destruction, or MAD, before it is too late.

That The Thing was more successful at the box office in 1951 in terms of financial earnings perhaps speaks more to the desire of general moviegoers to prefer what was perceived as relatively light entertainment compared to a film with a bigger production budget, a more sophisticated plot, and an Important Message to Humanity, rather than suspect the public would want warfare over peace. Or so one may hope.

Yet another counterexample of a science fiction film from the 1950s with a flying saucer starship was Forbidden Planet, released in 1956.

This time the flying saucer belongs not to the expected aliens of either malevolent or benevolent stripes but to humans of the 23rd Century as their interstellar vehicle of choice to explore and patrol the Milky Way galaxy at the behest of the United Planets. However, the intended good and bad guys of the film are more in line with the characters in The Thing: The crew of the hyperdriven starship designated just C-57D consists of a military style hierarchy on a rescue mission to Altair 4 to retrieve some research scientists presumably stranded on that remote alien world twenty years ago. There they encounter only one surviving scientist, a fellow named Dr. Morbius, his daughter, Alta, and their robot servant, Robby.

Morbius has found the still-functioning technological remains of an ancient and long-extinct civilization which called themselves the Krell. Far more advanced in virtually every way than even this future human society, the scientist refuses to relinquish control of all that he has learned from the Krell to any members of his fellow species, as he considers the rest of humanity neither ready for nor worthy of such superior knowledge.

Tensions mount as the scientist increasingly rejects the standing orders of the United Planets officers to bring back to Earth any survivors from Altair 4. They also have the unexpected complication of dealing with a strange and powerful alien technology and the need to report this discovery to their superiors.

Ultimately, the situation goes sour when Dr. Morbius unconsciously uses the Krell technology against the C-57D crew to force them to leave the planet or else. The alien instrumentality turns Morbius’ subconscious primitive thoughts into a deadly material reality, producing a literal monster from the id portion of his brain that kills several crewmen and threatens to destroy them all. The human warriors are forced to defeat Morbius and his godlike powers at the cost of almost everything, including the very planet of the Krell itself.

As with The Thing, the heroes and “good guys” in Forbidden Planet are the exclusively white, male, and American officers and crew of the C-57D. Anyone and anything else that does not fall into lockstep with these men and their ideals is labeled naive and delusional at best and a dire threat at worst. This includes the Krell, who destroyed themselves when they allowed their quest for knowledge and power to go unchecked. The starship’s captain, J. J. Adams, even “gets the girl”, Alta, in the end as his “reward”, just like Captain Hendry and Nikki in The Thing.

If you want to learn much more about Forbidden Planet, please read my two-part essay on Centauri Dreams starting here:

https://www.centauri-dreams.org/2017/09/11/creating-our-own-final-frontier-forbidden-planet/

and here

https://www.centauri-dreams.org/2017/09/12/creating-our-own-final-frontier-part-two/

As an interesting comparison, the starship that the Thing arrived in from the original short story “Who Goes There?” resembles an unadorned submarine rather than the flying saucer design from the 1951 film and its much later cinematic remakes.

“Something came down out of space, a ship. We saw it there in the blue ice, a thing like a submarine without a conning tower or directive vanes. 280 feet long and 45 feet in diameter at its thickest.”

Campbell’s story was published nine years before the modern UFO “flying saucer” era. If you look at the science fiction artwork and story descriptions of spaceships in the decades before 1947, such vessels often had much in common with real aquatic submersibles. This makes sense in that a submarine and its crew traveling through the ocean has definite parallels with a manned spaceship moving through space. Submarines would have been the closest vessel type to a spaceship for those artists and authors to have a comparison with in the pre-Cold War and Space Age eras.

It is interesting to see how a cultural mindset on a particular subject can change almost wholesale, and in such a relatively short period of time.

What About Those Other Things?

You may have noticed that I have given little mention of the other film versions of The Thing in this essay. This is largely due to the fact that while the 1982 version has become rightly praised on multiple fronts, not the least of which includes the fact that it follows the original 1938 science fiction story much more closely than the 1951 film when it came to the design and actions of the alien, director John Carpenter’s vision is not nearly as focused on the deeper themes found in its cinematic predecessor and inspiration.

In essence, Carpenter’s take on The Thing is largely a successful horror film with a shapeshifting alien creature as the protagonist whose primary motivation appears to be sheer survival. The human characters trapped with it in the isolated Antarctica research station are far more focused on not being absorbed and taken over by this truly monstrous intruder and their growing paranoia over who is actually the alien in disguise.

As for the 2011 film “prequel”, it is mostly an inferior copy of its 1982 predecessor. The only real difference in terms of items and information from the other films is that the prequel created the interior of the alien’s starcraft and gives its own explanation why the vessel impacted on Earth: The ship belonged to an advanced nonhumanoid ETI species that was exploring the Milky Way galaxy to collect biological specimens for later scientific study.

One of the organisms they found and took onboard during their expedition was the Thing, which eventually broke free of its containment unit and attacked the ship’s crew while they were in the vicinity of Earth. In an attempt to destroy the alien, the ship was deliberately crashed into the planet’s southern polar continent, obviously without success.

For those of you who may still want to salvage these later cinematic takes on The Thing from the pit of straight horror entertainment with an attempt at speculation on the further motives of the alien, you are in luck.

Just one year before The Thing prequel was released into theaters, Canadian science fiction author Peter Watts took on the task of giving us the alien’s perspective on its existence and its encounters with the handful of human and canine residents of Antarctica. Titled “The Things” and both published and made into a podcast in 2010, we learn that the Thing is not some mindless feeding monster, but was instead…

“…so much more, before the crash. I was an explorer, an ambassador, a missionary. I spread across the cosmos, met countless worlds, took communion: the fit reshaped the unfit and the whole universe bootstrapped upwards in joyful, infinitesimal increments. I was a soldier, at war with entropy itself. I was the very hand by which Creation perfects itself.

“So much wisdom I had. So much experience. Now I cannot remember all the things I knew. I can only remember that I once knew them.”

The Thing soon learns from its initial encounters with these strange terrestrial creatures that they actively do not like and do not want to be “communed” with, for they are individual and largely independent entities with minds confined to one localized area of their bodies rather than throughout every cell of their beings like the Thing. This leaves the alien “ambassador” both shocked and repulsed by these “thinking cancers” as it first labels humans.

Having barely escaped being destroyed at the research station after its numerous efforts to commune with the dogs and humans there and now trapped on Earth in an ice-laden wasteland, the alien eventually empathizes with its attackers and the lonely and lifespan-limiting fate that evolution has dealt them, which it now refers to as “the things”.

As The Thing buries itself in the polar ice for preservation to await release by future discoverers, the being determines its new purpose is to bring the wondrous uplifting qualities of communing to all terrestrial organisms, for their benefit.

The alien in Watts’ story is based on the being from the 1982 film and is of course entirely from his own imagination: We are never given such a perspective in the Carpenter film. Just like the USAF airmen in the 1951 version, the men of the Antarctic research station only want to kill the alien: They have no desire to communicate with it (they would likely consider it pointless anyway) and they do not want to understand the intruder beyond acquiring the knowledge of how to eradicate it.

This is especially ironic in that about half of the men in the cast are portraying scientists. At one point a young assistant biologist named Fuchs protests the destruction of several organic samples of the alien on scientific grounds, but is quickly overruled. Most of the dialogue in the 1982 version is often too colloquial and clipped to contribute any real substance to the discussions regarding ETI for this essay.

In terms of science, primarily what one could take from the Carpenter film is to add one more cultural data point that most human beings placed in lethal danger by unknown forces will respond with paranoia and hostility that will easily turn into a mob mentality if they are facing such a threat as a group.

This lack of internal revelation is disappointing, as it would have added some very interesting and unexpected layers to the Thing, rising it and the plot above the purely horrific monster we were given. Exploring these depths might also have added some substance to the real world debate about whether or not to contact ETI and how to deal with alien life once it is found, as that type of science fiction often does.

This is why the 1951 cinematic version has more intellectual value and depth in certain respects despite dovetailing from the original Campbell story in key places and having the least emphasis on special effects for the alien due to budget and special effects technology constraints. Even with the built-in bias towards the alien being a threat to all Earth life, the opposing viewpoints shown between the scientists and the military genuinely contribute to the popular-level scientific debate found in The Thing from Another World.

You may read “The Things” story in full at either of these following Web sites, or listen to the audio/podcast versions, if you prefer:

http://escapepod.org/2011/06/23/ep298-the-things/

http://clarkesworldmagazine.com/watts_01_10/

One Last Thing…

“I hate war, for it spoils conversation.” – Bernard Le Bovier De Fontenelle (1657 – 1757), French author and member of the French Academy who wrote one of the first popular accounts about alien life and the heliocentric theory: Conversations on the Plurality of Worlds, first published in 1686.

You may read the 1803 English edition online here:

https://openlibrary.org/books/OL6981190M/Conversations_on_the_plurality_of_worlds

Fontenelle also once said:

“Nothing can be more destructive to ambition, and the passion for conquest, than the true system of astronomy. What a poor thing is even the whole globe in comparison of the infinite extent of nature!”

We shall one day see if such a grand perspective does indeed stem the aggressive sides of intelligent species both on this world and beyond.

References

The following hyperlinks take you to places of information for your further appreciation of the film The Thing from Another World. You will find several other reference links throughout the essay. These links were functional at the time of this essay’s publication.

Here is the 1938 science fiction story that started it all…

http://www.goldenageofscifi.info/ebook/Who_Goes_There.pdf

Although the author of “Who Goes There?” was listed in the August, 1938 issue of the magazine Astounding Science Fiction as Don A. Stuart, his real name was John W. Campbell, Jr., who had just become the publication’s managing editor. Campbell is considered to be one of the primary shapers of modern science fiction, with a heavy emphasis on the science aspect of the genre. This is evident throughout the story, with lots of real science tidbits on a variety of subjects thrown in along the journey.

In this story, the alien had crash-landed its starship on Antarctica roughly twenty million years ago and became frozen in the surrounding ice, not the day before as in the 1951 film. Both versions have the Thing’s vessel being destroyed accidentally when its human discoverers attempt to remove it from the ice using thermite bombs.

After the Thing is found and brought to the research station for study, some of the characters in Campbell’s work actually take the time to debate whether the alien could be dangerous/evil or not. They initially conclude that a human cannot adequately judge the expressions and features of a truly alien being to determine its thoughts and emotional states.

Other characters immediately assume upon first seeing the creature that it is evil and full of hatred and fury based on the baleful gaze it projects from its three red eyes, which are surrounded by blue wormlike tentacles on its head and over its body, like the snakes of Medusa from ancient Greek mythology. They also determined at one point that the alien evolved on “a hotter planet that circled a brighter, bluer sun they came.”

Of course it turns out that the alien is very hostile and apparently hate-filled. It is also telepathic and can project thoughts to others. Once it escapes from the block of ice it was encased in, the being has no qualms completely taking over (and therefore killing) any terrestrial life forms it comes across down to the cellular level. When the Thing is finally destroyed, the survivors discover the alien had gotten quite far in building an atomic-powered anti-gravity device that would have allowed it to escape beyond Antarctica.

In 2018, a box of manuscripts donated by Campbell to Harvard University were found to include a much longer version of this story titled Frozen Hell. A very successful Kickstarter campaign made it possible for this novel to be published, first digitally as an E-book in January of 2019 with a later goal of hardcopy printed versions.

The original theatrical trailer:

https://www.youtube.com/watch?v=eLqm-YcQQd8

The complete original 1951 film online at Archive.org:

https://archive.org/details/TheThingFromAnotherWorld_201712

This is a straight transcript of the released 1951 film. Sadly none of the dialog is labeled in terms of who said what and there are no stage directions:

http://www.script-o-rama.com/movie_scripts/t/thing-from-another-world-script.html

A Web page celebrating the sixtieth anniversary of the release of The Thing from Another World in 2011. A nice plot summary and lots of good stills and behind the scenes images:

https://johneaves.wordpress.com/2011/04/28/the-thing-from-another-world-the-60th-anniversary/

Although this Web site is mainly focused on the later film versions of The Thing, in particular the John Carpenter version from 1982, some information may be found on the 1951 film. This includes the complete August 29, 1950 draft script:

https://www.outpost31.com/

If you want to read a detailed yet fascinating yet anything-but-dry analysis of alien life in all its potential forms, behaviors, and motivations that uses science fiction characters as its jumping off points, you cannot do much better than this Web site:

http://www.projectrho.com/public_html/rocket/aliens.php

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99942 Apophis: The Value of a Close Approach

The approach of the asteroid 99942 Apophis in April of 2029 offers an opportunity to study a sizeable asteroid through both radar and optical telescopes. Marina Brozović, a radar scientist at the Jet Propulsion Laboratory, points out that radar studies of the object might resolve surface details that are no more than a few meters in size. No surprise, then, that Apophis is the subject of much discussion at the 2019 Planetary Defense Conference in College Park, Maryland.

This is the same conference at which NASA Administrator Jim Bridenstine warned about the critical nature of planetary defense, noting the Chelyabinsk event in 2013 that delivered some 30 times the energy of the Hiroshima bomb. NASA has contracted with SpaceX to provide launch services for its Double Asteroid Redirection Test (DART), which is expected to launch in 2021 via a SpaceX Falcon 9 and test asteroid deflection through high-speed collision.

DART’s target will be the tiny moon of an asteroid called Didymos, which it will reach by solar electric propulsion in October of 2022, when the asteroid closes to within 11 million kilometers of Earth. Bridenstine pointed out that the NASA plan to detect and characterize 90 percent of near-Earth objects measuring 140 meters in diameter and above is “only about a third of the way there,” adding that events like Chelyabinsk are expected roughly every 60 years.

So it’s heartening to see missions like the Japanese Hayabusa2 and NASA’s OSIRIS-REx probing the nature of these objects, even as we look toward the Apophis opportunity in 2029. Numerous small objects on the order of 5-10 meters have been found passing as close to the Earth as Apophis, but the latter is substantial, a 340-meter asteroid that will be widely studied as it approaches to within 31,000 kilometers of the surface. The asteroid will become a naked eye object in the night sky over the southern hemisphere on April 13, 2029.

Image: This animation shows the distance between the Apophis asteroid and Earth at the time of the asteroid’s closest approach. The blue dots are the many man-made satellites that orbit our planet, and the pink represents the International Space Station. Credit: NASA/JPL-Caltech.

You may recall that following its discovery in 2004, early calculations showed a 2.7% chance that Apophis might impact the Earth in 2029, but follow-up observations have ruled that out. Now we can take advantage of the close passage to study Apophis’ size, shape and composition. A key question: Can we use the flyby to learn more about the asteroid’s interior?

“We already know that the close encounter with Earth will change Apophis’ orbit, but our models also show the close approach could change the way this asteroid spins, and it is possible that there will be some surface changes, like small avalanches,” said Davide Farnocchia, an astronomer at JPL’s Center for Near Earth Objects Studies (CNEOS), who co-chaired the April 30 session on Apophis with Marina Brozović.

Apophis’ passage in 2029 will take it within the distance some spacecraft orbit the Earth, and there remains the possibility of a mission to the object. As to future collision risks, the trajectory of Apophis is well established, but gravitational interactions between asteroid and Earth make it necessary to continue to recalculate the orbit. As we assemble the catalog of potentially hazardous objects, the need for missions like DART — and others testing a range of mitigation strategies — is clear. Because if we ever do find an asteroid of this size that presents a danger to our planet, we need to know what we’re going to do.

You can watch video from the 2019 Planetary Defense Conference here.

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Corridor of Ice Identified on Titan

What an interesting thing Titan’s atmosphere turns out to be. A fine haze produced by sunlight breaking apart methane molecules settles continuously to the surface, leaving organic liquid and solid sediments. Titan also has large lakes, but these contain about a third of the necessary methane, available through evaporation, to replenish that atmosphere, which should be depleted over geological time scales. What produces Titan’s supply of methane?

It was to answer that question that Caitlin Griffith (University of Arizona Lunar and Planetary Laboratory) and colleagues embarked on a study of cryovolcano activity on Titan. Cryovolcanoes erupt not with molten rock but volatiles like water or methane, and thus could provide an answer if they are venting methane found in subsurface reservoirs. A feature on Titan’s surface called Sotra shows cryovolcanic features that imply past icy flows.

Image: A giant of a moon appears before a giant of a planet. Titan, Saturn’s largest moon, measures 5,150 km across and is larger than the planet Mercury. Credit: NASA/JPL-Caltech/Space Science Institute.

Thus the need for a study of Titan’s surface focusing on potential cryovolcano candidates. But this is tricky work, with weaker spectral features difficult to tease out because of the moon’s dense atmosphere. The work draws on tens of thousands of spectral images produced by Cassini’s Visible and Infrared Mapping Spectrometer. The team developed a principal components analysis (PCA) which allowed a more fine-grained breakdown of surface ice and sediments at the four wavelength bands that most clearly view Titan’s surface from orbit.

Out of this came the detection of an icy linear feature, a ‘corridor’ in Griffith’s words, and one that raises questions:

“This icy corridor is puzzling, because it doesn’t correlate with any surface features nor measurements of the subsurface. Given that our study and past work indicate that Titan is currently not volcanically active, the trace of the corridor is likely a vestige of the past. We detect this feature on steep slopes, but not on all slopes. This suggests that the icy corridor is currently eroding, potentially unveiling [the] presence of ice and organic strata.”

Based on the settling of sediments from the atmosphere, scientists expect the surface of Titan to be an ice bedrock coated with organic materials. What the team has found is that water ice is unevenly exposed in Titan’s tropical latitudes. The exposed icy materials do indeed appear as a long, linear corridor that stretches 6,300 kilometers, with the aforementioned Sotra region especially rich in water ice, and positioned roughly in the middle of the icy corridor.

Image: Three orientations of Titan’s globe: the icy corridor is mapped in blue. Credit: NASA/JPL-Caltech/Space Science Institute.

All of this relates to the methane question, because the distribution of organic sediments on the surface is, the researchers believe, related to the history of Titan’s interior. We seem to be seeing evidence of a past, geologically active period. As Griffith notes, the icy feature does not correlate with topography as measured by Cassini’s radar measurements, nor does it seem to correlate with gravitational field anomalies likewise noted by Cassini, which offer a limited measure of subsurface composition. Just when did it appear, and how? From the paper:

The linearity of the icy corridor over a global scale presents the question of whether tectonic processes shaped this feature, thereby manifesting the processes that mould Titan’s surface and subsurface on a global scale. However, we find no evidence that Titan is geologically active, consistent with Titan’s long-wave topography and gravity field, which indicate a thick ice shell that is conductive rather than convective.

The answer may lie in the past, with methane surging up from below:

Measurements of the 13C/12C ratio in Titan’s atmosphere indicate that methane was injected into the atmosphere not more than 0.5–1 billion years ago. This age is consistent with the volume of dunes that would have accumulated since then, and suggest, consistent with evolution models of Titan’s interior, that a major cryovolcanic event occurred several million years ago. Potentially the topography that established the steep slopes of the icy corridor is a remnant of the time when Titan was geologically active. One example is the Sotra region, which displays cryovolcanic features, the steep terrain of which exhibits the strongest water-ice features.

Thus a past cryovolcanic event could explain Titan’s methane, with the ice corridor a telling reminder of these processes. Icy features in other parts of Titan are found only in local regions exposed by erosion or cratering, which suggests that if cryovolcanism remains an active process on Titan, it is not widespread. The team plans to use the same techniques to examine Titan’s poles, where the moon’s methane seas are prominent, to explore these ideas further.

The paper is Griffith et al., “A corridor of exposed ice-rich bedrock across Titan’s tropical region,” Nature Astronomy 29 April 2019. Abstract.

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Refined Parameters for an Expanding Universe

When it comes to matching what we know of the early universe, as seen in the Cosmic Microwave Background (CMB), with what we see today, astronomers have their work cut out for them. Edwin Hubble could demonstrate that the universe was expanding by studying the redshift of galaxies as they receded, but the rate of that expansion has been controversial. Now we have new work based on data from the Hubble Space Telescope as well as the Araucaria Project (about which more in a moment) that is helping us refine the Hubble constant (H0) to tighten the parameters on how the universe’s expansion is accelerating.

The result: The universe is expanding some 9 percent faster than we would expect based on observations by the European Space Agency’s Planck satellite, which mined data from the CMB from 380,000 years after the Big Bang. Exactly what drives this accelerated expansion — an enhanced interaction between matter and something we have yet to detect, ‘dark’ matter, or the as yet unknown form of energy likewise called ‘dark’ — no one knows.

Nonetheless, our cosmos is doing something that we need to explain. Nobel laureate Adam Riess (Johns Hopkins University and Space Telescope Science Institute) is lead researcher on this work. Riess’ Nobel came in 2011, shared with Saul Perlmutter and Brian Schmidt for demonstrating that the expansion of the universe was accelerating. We now firm up that discovery yet further. Riess says the chances of this observation being in error have dwindled from 1 in 3,000 to 1 in 100,000, adding “This disparity could not plausibly occur by chance.”

“This is not just two experiments disagreeing,” Riess added. “We are measuring something fundamentally different. One is a measurement of how fast the universe is expanding today, as we see it. The other is a prediction based on the physics of the early universe and on measurements of how fast it ought to be expanding. If these values don’t agree, there becomes a very strong likelihood that we’re missing something in the cosmological model that connects the two eras.”

Image: This illustration shows the three basic steps astronomers use to calculate how fast the universe expands over time, a value called the Hubble constant. All the steps involve building a strong “cosmic distance ladder,” by starting with measuring accurate distances to nearby galaxies and then moving to galaxies farther and farther away. This “ladder” is a series of measurements of different kinds of astronomical objects with an intrinsic brightness that researchers can use to calculate distances. Credit: NASA, ESA, and A. Feild (STScI).

Riess is working with a team called SHOES, for Supernovae, H0, for the Equation of State, which analyzed the light of 70 Cepheid variable stars in the Large Magellanic Cloud. Cepheid variables are ‘standard candles’ that brighten and dim at predictable rates, making it possible to measure the distance between galaxies. On the immediate level of data acquisition, the team was able to sharply reduce the time normally required for studying a Cepheid with Hubble (one star for every 90 minute orbit). Using a technique called Drift And Shift (DASH), Hubble can take quick ‘point and shoot’ images, considerably speeding the process.

With the Hubble data in hand, Riess combined them with observations from the Araucaria Project, which is an international collaboration studying the calibration of extragalactic distance, with considerable attention to Cepheid variables, RR Lyrae stars and other potential distance markers. The group has used eclipsing binaries to tighten our distance estimates to the Large Magellanic Cloud. The combined data helped refine the true brightness of the Cepheids.

Image: This is a ground-based telescope’s view of the Large Magellanic Cloud, a satellite galaxy of our Milky Way. The inset image, taken by the Hubble Space Telescope, reveals one of many star clusters scattered throughout the dwarf galaxy. Credit: NASA, ESA, Adam Riess, and Palomar Digitized Sky Survey.

We get a new estimate of 74.03 kilometres per second per megaparsec for Hubble’s constant, which means that for every 3.3 million light years further away a galaxy is from us, it appears to be moving 74 kilometers per second faster. This is a result of the expansion of the universe, and as mentioned above, is a figure 9 percent higher than the Planck observations of the early universe. The latter pegged the Hubble constant at 67.4 kilometres per second per megaparsec.

Consider the values we’ve determined for the Hubble constant in recent decades. A factor of two separated estimates of the constant in the days before the Hubble Space Telescope was available. By the late 1990s, the Hubble Space Telescope Key Project on the Extragalactic Distance Scale refined the value to within 10 percent. By 2016, with the discovery that the universe was expanding faster than previously calculated, the uncertainty dropped to 2.4 percent. What Riess and team have done is to reduce that figure down to 1.9 percent.

“The Hubble tension between the early and late Universe may be the most exciting development in cosmology in decades,” says Riess. “This mismatch has been growing and has now reached a point that is really impossible to dismiss as a fluke.”

And where do we go from here? From the paper (note the reference to gravitational waves, as well as to the supernovae used to extend distance measurements deeper into the cosmos):

A new feature in the dark sector of the Universe appears increasingly necessary to explain the present difference in views of expansion from the beginning to the present… Continued pursuit in precision in the determination of H0 is also needed to transition from the discovery of a difference to a diagnosis of its source. Additional observations of giants and pulsating stars in more hosts of SNe Ia [supernovae] are underway and should further refine H0. Less predictable but highly sought are contributions from gravitational wave sources as standard sirens (Schutz 1986; Abbott et al. 2017; Chen et al. 2018). Improvements in parallaxes from future Gaia data releases are also expected to continue to increase the precision of the distance ladder in the near term.

The paper is Riess et al., “Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics Beyond LambdaCDM,” accepted at the Astrophysical Journal (preprint).

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Probing Parenago: A Dialogue on Stellar Discontinuity

The publication of a paper called “New Features of Parenago’s Discontinuity from Gaia DR1 Data” by V. V. Vityazev and colleagues brought us a new look at an unusual observation. Parenago’s Discontinuity refers to the fact that red, cooler stars move faster in the direction of galactic rotation than blue, hotter stars, based on Hipparcos data. But is the phenomenon just a chance, local observation? Fortunately, a much larger dataset from the Gaia mission has now become available, and it is this that the Vityazev paper addresses in terms of Parenago’s finding. The following dialogue between Greg Matloff and Alex Tolley goes to work on the Vityazev document. Dr. Matloff has pointed to the Discontinuity as a possible marker of consciousness among low temperature stars, where molecular bonds can form.

Could motion be a matter of agency in such stars? Greg explored the idea in his book StarLight, StarBright. Now Alex digs into the Vityazev paper and questions whether Greg is right that his controversial theory can be falsified given our data. Various mechanisms for stellar motion are explored, ranging from coronal mass ejections to possibilities that are downright Stapledonian. How exactly would a civilization go about moving stars? I am preserving the dialogue format of the original correspondence as a case in point of serious differences being discussed in a way that both disputants have found valuable.

By Greg Matloff and Alex Tolley

Alex: Greg, in your 2012 Centauri Dreams post Star Consciousness: An Alternative to Dark Matter, you made the claim that there was an alternative explanation to dark matter for the velocity of stars around the galactic center. Your hypothesis was some sort of psychokinesis effect generated by consciousness, even if a primitive one. You used the Parenago Discontinuity (PD), which showed that velocity was related to star type, to suggest that fast stars were cool and that these cool stars could have chemistry, allowing some sort of consciousness. The 2015 Centauri Dreams post Greg Matloff: Conscious Stars Revisited further elaborated on this hypothesis.

The first problem I have with the data you used is that there was no plateau of velocity, but rather a peak, unlike the classic Parenago Discontinuity, which showed a plateau. This would imply that star types reach a peak velocity, then decline. Why would there be such an effect if consciousness was the driver of some psychokinetic effect? A possible explanation could be the amount of material that could be expelled to propel the stars.

The issue was left on whether the Parenago Discontinuity was purely a local, rather than galactic effect. We awaited the Gaia data.

The Vityazev paper using Gaia data confirmed that the Parenago Discontinuity was indeed non-local and that the peak effect around B-V of 0.7 seen with the earlier data you presented was indeed correct. As you had hung the hypothesis on the Parenago Discontinuity, this confirmation with the larger data did not falsify the interpretation that stars might be conscious.

The Hipparcos satellite measured the distances to hundreds of thousands of stars. It also measured the magnitude of each star through two filters:

A blue filter, yielding a B (for “blue”) magnitude

A greenish filter, yielding a V (for “visual”) magnitude (the human eye has highest sensitivity in the green)

Now, astronomers call the difference between the B and V magnitude of a star its (B-V) color, or sometimes just “color” for short. Remember how magnitudes work: large numbers mean “faint”, and small numbers mean “bright”. What is the “(B-V) color” of a hot star?

Figure 5 in the Vityazev paper seems to offer the basis for the more likely explanation of the PD results.

The figure 1b graph (left) shows the PD with the Gaia data. The figure 5 chart (right) shows that the PD effect is correlated with stellar age, rather than stellar temperature. The cooler stars in the sample are actually younger than G stars at the age peak. The shape of the B-V vs age graph matches the B-V vs azimuthal velocity (V) graph. This seems to me to suggest that velocity is therefore related to age, and more likely due to some physical factor related to time.

This seems to me to be the most parsimonious relationship and should be chosen by Occam’s razor. The stellar conscious hypothesis has to account for this age relationship and explain why the coolest stars that should have good consciousness and can, for unknown reasons and unknown mechanisms, chase around the galaxy faster than large, hotter stars, nevertheless go more slowly than G-type stars.

Why stars increase velocity with age still needs elucidation and modeling. However, the Vityazev paper has broken down the many components of stellar kinematics. This should provide a nice set of constraints for validating computational models.

Greg: The fact that Parengo’s Discontinuity is apparently non-local supports my hypothesis and does not support density waves. I have gone through the Messier, Herschel, and NGC Catalogues and reported my results in several publications. No known diffuse nebula in our galaxy or the Clouds of Magellan is large enough to drag along stars over a ~1,000 light-year radius sphere. The fact that stars seem to move faster along the direction of galactic motion as they age is very interesting, but it does not bear upon my original hypothesis that the discontinuity occurs at the point where molecules come in to stellar spectra. It is in my data as well as the data in the paper, so I presume that it is correct. I had originally ignored it because it does not bear on the original hypothesis. I presented in my original letter to Paul and others the causes I could think of to explain this phenomenon. But please, don’t hesitate to present others.

I am pretty happy right now because I predicted a non-local Parenago Discontinuity and this has apparently been verified. No one else, to my knowledge, had made this prediction. The local alternative explanations are now extinct. But science works by constructing alternative explanations for a phenomenon and testing them. Please do so. Try your hand at galaxy-wide possible alternative explanations. I can think of a few that won’t work. I am very interested in what you and others come up with and look forward to a dialogue of competing ideas.

Alex: The chart below is a rough conversion of the B-V values to age (from Figure 5) and the velocity from figure 1b. This seems to show that the Parenago Discontinuity might be a phenomenon based on using a variable (stellar type) that isn’t really related to the star’s velocity. Using age provides an approximately linear trendline with an R-squared of 0.93.

I accept that this velocity might be hard to explain (I am certainly not able to comment on this) but the relationship of age to velocity does seem to point to a simpler explanation for V based on natural forces, rather than requiring agency.

This older reference looked at A and B stars and examined the velocity differences based on age. There were clear differences based on age, rather than stellar type. While this doesn’t invalidate your hypothesis, they do have a physical explanation on why age impacts star velocity. To my mind, such approaches should be examined further before resorting to more exotic explanations. With the Gaia data, astronomers involved in kinematics studies now have a trove of high-quality data to test their models. I would be looking amongst that cadre for cutting-edge modeling.

Greg: Nice analysis! What I tried to do is put all the cards, as I see them, on the table. I am not and never have been an advocate for psychokinesis. But science seems willing to accept the Multiverse, which can perhaps not be verified. It accepts dark matter and invokes many properties for this stuff even though it remains hidden. I have discussed PK and the Geller/Randi controversy with people on both sides and find nothing wrong with their arguments. So I believe, with David Kaiser of MIT and others, that the case should be reopened. If a weak PK force can be demonstrated to the satisfaction of the scientific community, it should be considered an option.

I also believe that the stellar age variation has little to do with Parenago’s Discontinuity. Why does the discontinuity appear at the same place where molecules come in to stellar spectra?? And why indeed is it a discontinuity instead of a smooth curve? Invoking strange (and unknown) stellar variability to explain it is certainly an exotic explanation!

One of the problems with what we are discussing comes from the fact that I was checking the metaphysics of Olaf Stapledon, a sci-fi author and philosopher, and attempting to see if there is something scientific behind his discussion in Star Maker. If I were starting afresh, I would title my work (as I have done in subsequent papers) “A Test of Self-Organization on the Galactic Scale?”, since astrophysicist Erich Jantsch uses “self-organization” as a possible explanation of consciousness. Alternatively, I might go with the terminology of philosophers such as David Chalmer and title my papers “Is Panpsychism a Science?”

I think that the work that you have done on (B-V) vs. star age from the Gaia Release 1 sample is invaluable and should be included in our published dialogue. I hope very much that our debate leads to further work with future Gaia data releases.

Alex: Let me give you a perspective from a biologist’s point of view. The Parenago Discontinuity might have an analogy to living vs non-living, where living things can be observed to grow, move (or have tropisms), reproduce, etc. Let us assume that cooler stars have some sort of motility which is driven by a “need”, perhaps acting something like a bacterium. Bacteria can be observed to move faster in their medium if they have flagella. A biologist would ask “what is the evolutionary advantage of movement given the cost” and might hypothesize that this leads to faster food discovery, or a phototropism, or evasion of larger predators. In the case of cool stars, I would be asking similar questions. Why is V (azimuthal velocity) the key variable, rather than a different direction (U, W)?

Given that V is affected by star type, what is the advantage of moving faster in one direction? One might hypothesize that this facilitates sweeping up of neutral gas clouds more effectively, but this would be even better if the stars moved in the opposite direction. Are the stars perhaps self-organizing into “flocks” and what we are seeing is the movement of the flock which is currently going in the V direction? With bacteria, we know that it is flagella that allow movement through the medium. With stars, one mechanism is with a Shkadov drive to asymmetrically create thrust. Another might be directed coronal mass ejections (CMEs). In the former case, it is not the star that is sentient, but more likely a separate intelligence, a more Stapledonian idea.

Therefore another hypothesis is that stars are being driven by a galactic wide intelligence[s] to reach a certain unified velocity for some reason. The age relation to velocity then makes sense if the Shkadov drives need billions of years to reach the needed velocity. For what purpose?

One idea might be to facilitate more frequent stellar encounters allowing biological civilizations to disperse more easily among the stars. On the other hand, if the galaxy is an organism or superorganism, perhaps the Parenago Discontinuity is some process to organize older stars for some equivalent of a cellular process.

An obvious question suggests itself. If cooler stars are somehow able to direct their velocity, shouldn’t very cool stars, i.e. red dwarfs and brown dwarfs, also have that behavior? We don’t have enough examples of BDs to determine this, but it would provide another datum. One might extend this to gas giant planets too. While the ones we know about are bound to their stars, is it possible that planetary migration is a related phenomenon? Are “hot Jupiters” exhibiting similar behaviors?

Clearly one can speculate endlessly. If the relevant variable is time rather than stellar type, then this constrains mechanisms to those that require both time and a reason for the more uniform direction. With such a constraint, looking for a natural process that requires billions of years would seem to be the most fruitful direction. That velocity W (fig 1c) is fairly constant, but U (fig 1a) declines with stellar type suggests to me that physical forces are somehow directing the movement into the W direction, whether those forces are natural or artificial. The direction is apparently translating from U, towards the galactic center, to V, a transverse direction, rather like the Coriolis forces operating on weather patterns that “shape” the velocity profile.

If time is the relevant variable, then looking for young, cool stars should be the best way to test the hypothesis. If they are fast, then stellar type is the key variable, but if slow, then time. The Vityazev paper also has limited data for red giant stars. If anything, the G, K and M red giant stars have more uniform V than main sequence stars, i.e. they seem to conform more closely to the classic PD plateau. Whatever the mechanism, size is clearly not a variable as they have velocities comparable to the oldest G stars. Creating an age chart for these stars might also be instructive.

Unfortunately, even if age is the relevant variable, it doesn’t falsify your hypothesis. The mechanism of acquiring a high V might simply require time, whether a natural, external force or an inner, self-directed one. Just as with determining which animals are conscious (e.g. using the mirror test), we need a better test to be able to falsify your hypothesis. We may be in the position of trying to determine sentience of a herd of buffalo from a still photograph when what we need is video or many photographs over time.

PS: A back-of-the-envelope calculation shows that a star could attain the necessary velocity by directing its radiant energy (e.g. Shkadov drive), but not by directed coronal mass ejections. (calculation for our sun).

Greg: Wonderful! My feeling has always been that stars need not have a high level of consciousness–they could be like slime-mold amoeba or developing cells in embryos.

I suspect that Vityazev et al could not use the red giant Gaia data for the same reasons the Burnham’s validation of Parenago for giants looks so fluffy. Since most of these stars are very distant, astrometric parallax is impossible with Hipparchus and the early Gaia data.

Spectroscopic distance estimates using the HR diagram are accurate to 10% or less. Also, what is the local reference standard when the subject stars occupy a sphere thousands of parsecs in radius? Hopefully, future Gaia data releases will offer the possibility of greater accuracy.

Also, I have been thinking about your suggestion regarding unknown forms of stellar variability. My suggestions in the earlier emails–EM radiation anisotropy and unidirectional jets in mature stars–are two of these. Perhaps there are others!

Greg: The Shkadov thruster could of course be a form of anisotropic EM emission from the star. But could such a thruster develop in a purely materialistic setting not requiring a Kardashev Type 2 civilization in that star’s system or volition on the part of the star?

It is so strange that we are encountering so many fascinating intellectual insights at the same time that national governments are failing. Last Sunday we attended a talk by Tyler Volk, a biologist at NYU. He has constructed a geometric/architectural model of self-organization from the quark to universal levels. Tyler suspects that we are moving towards the planetary phase of our civilization and this is the use of apparent political dysfunction. I hope he is correct.

Alex: Greg, you write: “The Shkadov thruster could of course be a form of anisotropic EM emission from the star. But could such a thruster develop in a purely materialistic setting not requiring a Kardashev Type 2 civilization in that star’s system or volition on the part of the star?”

I would be skeptical about EM emission asymmetry as I would have thought this would be detectable. A Shkadov drive with mirrors would definitely have some observable effects. Even just some “magical” control over EM emissions should be detectable.

While CMEs are not energetic enough, a small star with large CMEs that are accelerated to c might just work. But again, I would think such a beam would be detectable. I agree with you that such EM or particle control would need K2 civilizations to manage. With so many stars that would be exhibiting such high V’s, just by chance we would detect some anomalies, and solve the SETI question too.

It also occurs to me that since our galaxy has experienced a collision with another galaxy or satellite in the remote past, with a corkscrew effect on velocities, is there any chance this might in some way be responsible for the Parenago Discontinuity?

Let me refer to a post here on Centauri Dreams titled Gaia Data Hint at Galactic Encounter. I could imagine that an old collision with another galaxy or similar massive object accelerated stars which retained their higher velocities while younger stars maintain the velocities of birth in a more stable galaxy post-collision. To get the age-related relationship, it suggests that the collision must have had its impact on velocity over billions of years. Perhaps the values of U, W and V can be used to determine the likely form of the collision?

Greg: Regarding the Shkadov thruster discussion, have you read the Benford/Niven novels Bowl of Heaven and Shipstar? These discuss an advanced version of this concept. I have given some thought to a galactic collision producing Parenago’s Discontinuity. According to the computer simulations done at Cornell (and likely other places), when the Milky Way collides with Andromeda to form Milkimedia (what a horrible name!), there will be widespread disruption of diffuse nebulae. This might result in a Spiral Arms Density Wave effect drawing lower-mass stars along faster than their more massive colleagues.

But the same simulations indicate that the combined galaxies lose their spiral shapes after merger. The ultimate result is a giant elliptical with few nebulae and a very low rate of star formation. Since this has clearly not occurred for the Milky Way galaxy (which is a nice barred spiral), it is reasonable to conclude that such a galactic merger did not happen. From what I understand, galactic cannibalism (where a big galaxy gobbles a smaller one) has less disruptive effects–the big guy retains its shape (which might be an argument for self-organization on the galactic scale.

Alex: From an engineering point of view, I think controlling the solar wind might be a lot easier than deflecting the EM with a solid mirror. I would envisage surrounding the star in a charged, superconducting “mesh” to trap the protons. These would be funneled to electromagnetic accelerators to emit the protons in a unified direction at near c velocity. That might be enough to accelerate the star over the needed timescales. The advantage is lower mass requirements and no impact on the star’s light emissions or spectrum. However, I would expect that the proton beam emitted would be detectable. Think of this drive as a giant ion engine coupled with a ramscoop that captures the protons from the star, rather than from the interstellar medium as in a Bussard ramjet.

The Centauri Dreams link I provided was for a proposed “impact” with a dwarf galaxy (the Sagittarius dwarf galaxy). Much smaller than M-31, and if there was an impact, it certainly hasn’t disrupted the shape of our galaxy. What is interesting is the analysis technique that teased out the spiral shape of the velocity-position phase space that was too subtle to visualize with pre-Gaia data. This sort of analysis might offer a better way to understand the stellar type/age vs velocity relationship. Figure 2 in the paper referenced in the article shows the structure in the azimuthal (V) direction vs the radius (I cannot interpret if this has any possible bearing at all on the Parenago Discontinuity, but the same analysis teasing out stellar type might well do. It might be worth contacting the principal author regarding this approach. Paper attached)

[The paper Alex is referring to is Antoja et al., “A Dynamically Young and Perturbed Milky Way Disk,” Nature 561 (2018), 360-362 (abstract / preprint).]

Greg: Nice paper! Thanks for it. But can this effect bear on an apparent near-linear relationship between galactic revolution velocity and star age? I think that such dwarf galaxy absorptions by the Milky Way are rare events. Regarding the Shakdov thruster, you are (I think) correct. But could we detect a proton flow necessary to increase V by ~1 km/s over a 10 billion year time interval? Certainly fuel for thought.

Alex: Given the large numbers of stars in the sample, I was thinking that the stellar type vs velocity relationships could be plotted for locations on the galactic disc. If they are all the same, that would tell a different story than if they differed in shape. There is a hint of this in the Vityazev paper where they plot thin vs thick disk stars that show differences. In other words, given the large sample size, it should be possible to show more granularity based on location than with the averaging that Vityazev computes.

Incidentally, I came to the same conclusion with regards to CMEs. However, even for our sun, the CMEs are within a single order of magnitude if they are accelerated to c. As the solar wind produces more protons overall than CME, the same approach might work. However, this approach has to work for all stars, so the mass loss of protons/star mass has to increase for cooler stars for this mechanism to describe the PD observation.

I am not aware of the idea of moving stars by trapping and accelerating the solar wind and flares, so possibly it is novel. I also wonder if it is possible to direct solar flares by manipulating the surface magnetic fields of the star so that they break and cause a flare in desired positions. As the star rotates, the magnetic field is broken when the alignment is correct, releasing the flare. The flare material still needs to be accelerated to have the desired thrust, so electric fields could do that, or something more like a linear particle accelerator. Definitely K2 or even K3 level engineering…or just maybe some phenomenon than a “living” star could manage.

Greg: The differences between disc star velocities and others in the Antoja et al paper is fascinating. I don’t think it bears on Parenago unless somehow large diffuse nebula were created in the galactic merger. These could have perhaps caused differential velocities between massive and less massive stars. But such nebula would have to be perhaps an order of magnitude larger in radius than those in today’s galaxy to encompass a stellar sphere with a radius in excess of 1,000 light years. A further problem is that these structures would have to dissipate in less than 1 billion years, leaving no trace.

But your suggestion of using future Gaia data releases to dig deeper in stellar kinematics is excellent. I hope that someone will check if Parenago’s Discontinuity works for a star sample at a distance, say, of 10,000 light years.

I have done some rough calculations to see if a directional stellar wind or directional coronal mass ejections (CMEs) could accelerate a Sun-mass star by about 1,000 m/s in 1 billion years. Both seem to fail by a few orders of magnitude. But it is most intriguing that stellar flares (and presumably CMEs) are more common in less massive red dwarfs than in Sunlike stars.

Alex: BoE calculation for thrust of solar wind:

For our sun, redirecting the solar wind to a single direction would only result in the sun traveling ~3 m/s after 1 billion years. However, if the particles were accelerated by 3 orders of magnitude to c, that increases the velocity to 3 km/s. Over 5 billion years, that gets you to 15 km/s, which is in the range of the V needed for the Parenago Discontinuity graph. So physically possible. My first thought is that this would be an engineering solution, rather than a natural one – that is K2 – K3 civilizations. The bias in my thinking is that only human engineering can create craft that can travel at supersonic and hypersonic speeds. Birds cannot even manage 0.1 km/s, while our engineering can propel craft in air 1-2 orders of magnitude faster.

I do have a question about the relative emissions of EM and particles from different stellar types. Isn’t the mass loss vs initial star mass going to be the basically the same for all stellar types? If so, wouldn’t all stellar types reach the same velocity by the time they reach the end of their main sequence period? The Parenago Discontinuity relationship suggests mass or age is important, which implies that the acceleration must be approximately constant for all stars. This would imply, naively perhaps, a force more like gravity, that is exerted over the age of the star. It cannot be a point source outside the galaxy; otherwise the rotation of the galaxy would keep changing the direction of the force. Could it possibly be invoked by the [dark] matter in or surrounding the galaxy? Can this force be computed to suggest a possible cause?

Greg: Very interesting speculation. It’s so funny–we needed Gaia to get beyond a few hundred light years. And this early paper of Gaia results (and I am sure many others) will inspire people to generate designs for even more capable space observatories. It seems that every question we investigate and answer results in hundreds of new questions.

I would hesitate to invoke dark matter. It seems to be a catch-all for everything not understood in the universe. I will check out mass loss rates for distant star types. But I don’t know if we have reliable data.

Alex: What is relevant is whether the acceleration is related to stellar type or not. A large, hot star may lose a lot of mass, but it has to accelerate a more massive object. If a star loses X% of its mass over its lifetime, and if the wind speed is fairly uniform across such stars then the final velocity should be much the same for all star types over their lifetimes. The PD requires that this is not the case.

Greg: I just did a Google for “Mass Loss from Main Sequence Stars”. Apparently, this quantity directly depends upon star surface temperature.

I think our dialog has been very fruitful. When I submitted my first paper on the subject to the Journal of the British Interplanetary Society, I had to contend with 4 reviewers. Some of these favored the concept of stellar volition but argued about the inclusion of psychokinetics as a possible explanation. I am neutral regarding this topic, as I have discussed but I am still impressed by the vehemence of the arguments pro and con decades after the Geller/Randi affair. So the fact that accelerated CMEs can provide acceleration of G-type stars (as I agree after a few calculations) indicates that there is an alternative option. I will at some point write up my work on accelerated CMEs and send you the results.

Late this afternoon, weather permitting, we will journey to the Hayden Planetarium, which is hosting a Dutch astronomer who will talk about the latest Gaia results on galactic stellar kinematics. I suspect that Parenago’s Discontinuity is not on the agenda, but I will let you know.

Alex: I note that the Gaia data include all the information needed to create samples of stars within a radius of a position. This could be used to explore the type/mass vs V graphs at the higher granularity that I suggested, particularly radius from the galactic center. This would help confirm that the Parenago Discontinuity is truly global within the dataset and not some averaging, or whether there is spatial structure to the distributions. It may take some computational effort, but it might shed light on possible natural explanations of the PD observation. Sample sets would be easy to crunch on a PC, and the results compiled as a map. For example, the slope of V vs type or mass as a color-coded map.

I was also thinking about the gravity solution. It may work if a point object makes continual passes in the galactic plane. Older stars would experience more passes and if V is due to gravity dragging the stars along during a pass, then this would account for their higher V. A prediction would be that the slope of V would depend on how far from the source the stars are. Dare I say a denser clump of dark matter in a highly elliptical orbit about the galactic center? Data and some modeling would be needed to test this idea.

Out of this discussion, Greg Matloff incorporated many of Alex Tolley’s contributions and produced the short essay below looking at how stars could be accelerated to account for the Parenago Discontinuity.

Physical Methods of Effecting Main Sequence Star Acceleration

Greg Matloff, Nov. 16 2018

Using the Gaia DR1 dataset, Vityazev et al. have investigated Parenago’s Discontinuity for a sample of 1,260,071 main sequence stars [1]. The minimum mean distance for O-k stars in this data release is estimated as 0.15 kiloparsecs, which indicates that the diameter of the sphere containing the subject stars equals or exceeds 1,000 light years. Local explanations for Parenago’s Discontinuity clearly fail.

The analysis reveals that Parenago’s Discontinuity is real. Stars redder than (B-V) about equal to 0.6, which corresponds to spectral class F9 or G0 move faster in their orbits around the center of the Milky Way galaxy than hotter, more massive, bluer stars. Their results are in substantial agreement with the results from Allen’s Astrophysical Quantities and Hipparcos data for a much smaller stellar sample (with a diameter of about 500 light years) presented by Matloff [2].

But Vityazev et al. discuss for the first time a feature present in both data sets. Main Sequence stars apparently speed up in their galactic trajectory as they age. This velocity increment amounts to an increase of about 2 km/s in 8 billion years. The acceleration is approximately equal to 8 X 10-15 m/s2. For a solar-mass star (2 X 1030 kg), the average force exerted on or by the star during the 8 billion year time interval is 1.6 X 1016 N.

Reference 2 presents a number of possible causes for the discontinuity in galactic stellar orbital velocity around (B-V) = 0.6. The analysis presented here considers possible mechanisms that a star might employ to maintain a constant acceleration over a multi-billion year time interval.

1. Acceleration by Nonisotropic Stellar Electromagnetic Emissions

Consider here the possibility that a minded star can control the direction of its electromagnetic emissions. The solar luminosity (Lsun) is 3.9 X 1026 W [3]. Modifying Eq. ((7.2) of Ref. 4, the maximum stellar-radiation pressure acceleration for a Sun-mass star (Msun) is Lsun/ (Msun c) for a unidirectional stellar wind, where c is the speed of light in vacuum (3 X 108 m/s). Substituting in this equation, the maximum solar acceleration from this process is about 7 X 10-13 m/s2.

This acceleration is about 100 times the required stellar acceleration to effect the 1 km/s during a 1-billion year time interval. But if the Sun accelerates using this process, the Solar Constant might vary on an annual basis by up to 1%. Solar Luminosity has been measured to vary by a much smaller amount during the Sun’s 11-year activity cycle.

But the Sun and other main sequence stars generate neutrinos as well as photons as they convert hydrogen into helium deep in the solar (stellar) interiors [3]. Neutrinos have linear momentum as well as very small mass. The solar momentum flux is hard to study because of the very low cross-section of neutrino interactions with detectors. Perhaps stellar neutrino fluxes are not isotropic.

2. Acceleration by Nonisotropic Solar Wind

From Ref. 3, p. 427, the average solar wind velocity is 500 km/s (5 X 105 m/s) and the solar wind carries about 2 million tons of solar matter per second (2 X 109 kg). If all of this material were concentrated in a unidirectional jet, the force exerted on the Sun or Sunlike star is 1015 Newtons. This force is 1/16 the force required for stellar acceleration. This proposed method of stellar acceleration therefore fails.

3. Acceleration by Coronal Mass Ejections

Coronal mass ejections (CMEs) are generally associated with solar flares. Their frequency varies with the solar activity cycle. On average, the mass ejected by CMEs in a Sunlike star amounts to a few percent of the mass ejected in the solar wind and the velocity of a typical CME varies from a few hundred km/s to a few thousand km/s [5]. Unidirectional flares therefore fail as a stellar accelerating mechanism.

4. Acceleration by an Accelerated Solar Wind

Consider next the possibility that a minded Sunlike star can apply its magnetic field to accelerate a unidirectional solar wind to 0.1c (3 X 107 m/s). For the solar wind mass listed above, the kinetic energy of the jet is approximately 1024 W, which is less than 1% of the solar constant. If all of the solar wind is in the jet, the approximate force on the star is 6 X 1016 N. This is about 4X greater than the average force required to accelerate the star.

5. Might the Gravitational Constant of Galactic Mass Vary With time?

Elementary physics students learn that the velocity of an object orbiting a central body varies directly with the square root of the product of the central body’s mass and the Universal Gravitational Constant G. It might be argued that increases in galactic mass or G over billion-year time scales might account for the higher galactic-orbital velocities of older stars.

Surprisingly, as reviewed in an on-line essay by Rupert Sheldrake, experimental measurements of G show some variation [6]. But according to Lorenzo Iorio, such variations are likely caused by experimental errors because the orbits of solar system planets seem relatively constant [7].

A recently published study based upon the Gaia data set demonstrates that within the last 900 million years, at least one dwarf galaxy has passed through and possibly merged with the Milky Way [8]. So it is safe to conclude that the mass of our galaxy may not be constant over multi-billion-year time scales.

But it seems unlikely that either of these two variations can account for the reported increase in stellar galaxy-orbiting velocity with star age. After all, stellar birth nebulae orbit the Milky Way galaxy’s center as do the stars. Infant stars will therefore be accelerated in the same fashion as mature stars by such variations.

6. Conclusions

We see that several of the above suggestions succeed as possible methods of main sequence star acceleration. Perhaps the most intriguing, and the one that might inspire future research, is the possibility that stellar neutrino emissions need not be isotropic.

Psychokinetic (PK) effects have not been considered in the above treatment. Although it is unwise to eliminate PK from consideration for this application and others, it is wise to keep a distance until/unless it can be demonstrated in the laboratory in experiments that can be replicated by other researchers, including skeptics.

Acknowledgement

I greatly appreciate communications and interactions with Alex Tolley. His spirited comments and criticisms were instrumental in preparation of the above discussion.

References

1. V. V. Vityazev, A. V. Popov, A. S. Tsvetkov, S. D. Petrov, D. A. Trofimov and V. I. Kiyaev, “New Features of Parenago’s Discontinuity from Gaia DR1 Data”, Astronomy Letters, 44, 629-644 (2018).

2. G. L. Matloff, “Olaf Stapledon and Conscious Stars: Philosophy or Science?”, JBIS, 65, 5-6 (2012).

3. E. Chaisson and S. McMillan, Astronomy Today, 6th ed., Pearson/Addison-Wesley, San Francisco, CA (2008).

4. G. L. Matloff, Deep Space Probes, 2bd. ed., Springer-Praxis, Chichester, UK (2005).

5. P. Odert, M. Leitzinger, A. Hanslmeier, and H. Lammer, “Stellar Coronal Mass Ejections I. Estimating Occurrence Frequencies and Mass-Loss Rates”, arXiv:1707.02165v2 [astro-ph.SR] 31 Jul 2017.

6. R. Sheldrake, “How the Universal Gravitational Constant Varies.”, www.sheldrake.org. Also in R. Sheldrake, Science Set Free, Deepak Chopra Books, NY (2012).

7. L. Iorio, “Does the Newton’s Gravitational Constant Vary Sinusoidally with Time? Orbital Motions Say No”, arXiv:1504.07233v2 [gr-qc] 16 Dec 2015.

8. T. Antoja, A. Helm, M. Romero-Gomez, D. Katz, C. Babuslaux, R. Drimmel, D. W. Evans, F. Figueras, E. Poggio, C. Reyle, A. C. Robin, G. Seabroke, and C. Soubiran, “A Dynamically Young and Perturbed Milky Way Disk”, arXiv:1804.10196v2 [astro-ph.GA] 24 Sep 2018.

———

The Vityazev et al. paper is “New Features of Parenago’s Discontinuity from Gaia DR1 Data,” Astronomy Letters, Volume 44, Issue 10 (October 2018), pp 629–644 (abstract).

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An Earth-sized Planet for TESS

If Kepler’s task was to give us a first statistical cut at the distribution of exoplanets in the galaxy, TESS (Transiting Exoplanet Survey Satellite) has a significantly different brief, to use its four cameras to study stars that are near and bright. Among these we may hope to find the first small, rocky planets close enough that their atmospheres may be examined by space telescopes and the coming generation of extremely large telescopes (ELTs) on Earth.

Thus the news that TESS has found its first planet of Earth size is heartening, even if the newly found world orbiting HD 21749 is in a tight 7.8 day orbit, making it anything but clement for life. What counts, of course, is the demonstrated ability of this mission to locate the small worlds we had hoped to find. Diana Dragomir is a postdoc at MIT’s Kavli Institute for Astrophysics and Space Research, as well as lead author on the paper describing the latest TESS planet:

“Because TESS monitors stars that are much closer and brighter, we can measure the mass of this planet in the very near future, whereas for Kepler’s Earth-sized planets, that was out of the question. So this new TESS discovery could lead to the first mass measurement of an Earth-sized planet. And we’re excited about what that mass could be. Will it be Earth’s mass? Or heavier? We don’t really know.”

Image: NASA’s Transiting Exoplanet Survey Satellite (TESS), shown here in a conceptual illustration, will identify exoplanets orbiting the brightest stars just outside our Solar System. Credit: NASA’s Goddard Space Flight Center.

Dragomir considers the new planet around HD 21749, some 52 light years from Earth, a milestone in being the mission’s first planet of Earth size, though the expectation is for at least a few dozen more among the nearest and brightest stars as TESS continues sweeping the sky in overlapping sectors. This is a two-year mission that has already discovered 10 planets smaller than Neptune, four of which now have estimated masses. We’re in the early days of this mission, and that’s a good sign. As noted in the paper, “All of these discoveries are based on only the first two sectors of TESS data, suggesting many more are to be found.”

The star is a K-class dwarf in the southern constellation Reticulum that is known to host a second planet, recently confirmed, that is about three times the size of Earth. The paper reports on the discovery and confirmation of HD 21749b and the discovery of HD 21749c, but it is the latter, given its small size, that is receiving the lion’s share of coverage.

The paper notes that spectroscopic and photometric data have made the confirmation of the larger planet possible, while the Earth-sized HD 21749c would be a challenging observation for radial velocity confirmation, if possibly feasible with a dedicated campaign using the combination of the Very Large Telescope (VLT) and the ESPRESSO spectrograph. But density measurements of both planets should be useful. From the paper:

…the density of HD 21749b indicates that it is likely surrounded by a substantial atmosphere. By measuring the density of these two planets (and other similar planets that TESS may find) more precisely, we can begin to observationally constrain the maximum core mass a planet can reach during its formation before accreting a volatile envelope.

The paper is Dragomir et al., “TESS Delivers Its First Earth-sized Planet and a Warm Sub-Neptune,” Astrophysical Journal Letters Vol. 875, No. 2 (15 April 2019. Abstract.

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New Planet Detected in Circumbinary System

The transit method has proven invaluable for exoplanet detection, as the runaway success of the Kepler/K2 mission demonstrates. But stars where planets have been detected with this method are still capable of revealing further secrets. Consider Kepler-47. Here we have a circumbinary system some 3340 light years away in the direction of the constellation Cygnus, and as we are now learning about circumbinaries — planets that orbit two stars — the alignment of the orbital plane of the planet is likely to change with time.

Let’s pause for a moment on the value of the detection method. Transits detected in the lightcurve have helped us identify 10 transiting circumbinary planets, with the benefit of allowing astronomers to measure the planets’ radius even as variations in the duration of transits and deviations from the expected timing of the transits establish the circumbinary orbit.

At Kepler-47, we’re looking at the only known multi-planet circumbinary system. Moreover, the orbital period of the binary stars is in the range of 7.5 days, making this the shortest known orbital period for any known circumbinary system. The first two Kepler planets were detected in 2012, but San Diego State University astronomers now find a middle planet between these, Kepler-47d, its strengthening transit signal the result of orbital plane adjustment. In fact, the transit depth for the hitherto undetectable world has become the deepest of the three planets.

Jerome Orosz (SDSU) is the paper’s lead author.

“We saw a hint of a third planet back in 2012, but with only one transit we needed more data to be sure. With an additional transit, the planet’s orbital period could be determined, and we were then able to uncover more transits that were hidden in the noise in the earlier data.”

And according to co-author and SDSU colleague William Welsh, this planet defied expectations by showing up not exterior to the previously known planets but between them. “We certainly didn’t expect it to be the largest planet in the system. This was almost shocking,” said Welsh.

Image: Artist’s impression of the third planet in the Kepler-47 circumbinary system. Credit: NASA/JPL Caltech/T. Pyle.

So what we see at Kepler-47, at least at this juncture, is an inner planet 3.1 times the size of Earth, in an orbit taking 49 days around this G-class star orbiting an M-dwarf. The other planets here are, respectively, 7 times Earth-size on an 187-day orbit (Kepler-47d), and 4.7 Earth-size with a 303 day orbit. Remember that we are talking about planets orbiting two stars, in a system compact enough to fit inside the Earth’s orbit of the Sun.

Kepler-47’s system may be telling us something interesting about planet formation. From the paper:

This is the first detection of a dynamically packed region in a circumbinary system, and it further confirms suspicions that planet formation and subsequent migration can proceed much like that around a single star, at least when far from the binary (Pierens & Nelson 2008, 2013; Kley & Haghighipour 2014, 2015). We also find that, although they are close to having integer commensurate periods, the middle and outer planets are not in a mean-motion resonance–and yet they are gravitationally interacting and exchanging angular momentum, as indicated by their anti-phased oscillations in inclination and eccentricity.

The authors find the planetary configuration dynamically stable for at least 100 million years, adding:

This nearly circular, co-planar, packed configuration is unlikely to have arisen as an outcome of strong gravitational scattering of the planets into their current orbits. Rather, the observations suggest that the planetary configuration is the result of relatively gentle migration in a circumbinary protoplanetary disk.

Image: This is Figure 28 from the paper. Caption: The conservative (dark green) and optimistic (light green) habitable zone regions are shown for the Kepler-47 system. The red circle shows the critical stability radius (Holman & Wiegert 1999), interior to which planetary orbits are most likely unstable. Credit: Jerome Orosz/William Welsh et al.

On the matter of habitability, there is little reason to expect life here. These are low density worlds, all three being less dense than Saturn, which implies substantial hydrogen and helium atmospheres. The outer planet receives an average insolation from its two stars that is 86.5 percent of what the Earth receives. But while that puts this world within the boundaries of the circumbinary habitable zone, the density implies a world somewhere in the range between Neptune and Saturn. The newly discovered middle planet skirts the inner edge of the habitable zone, but again its density makes life unlikely.

The paper is Orosz et al., “Discovery of a Third Transiting Planet in the Kepler-47 Circumbinary System,” Astronomical Journal Vol. 157, No. 5 (16 April 2019). Abstract / Preprint.

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Huge White Light Flare on a Tiny Star

About 250 light years away there is a faint object that is on the borderline between brown dwarf and star. Only a tenth of the radius of our Sun, ULAS J224940.13-011236.9 was actually too faint for most telescopes to observe until a huge flare lit it up, turning this L dwarf, among the lowest mass objects that can still be considered a star, 10,000 times brighter than it was before. Very cool compared to the average red dwarf, L dwarfs emit radiation primarily in the infrared.

But this story also has to do with visible light, and the question of how such a small object can produce such a powerful explosion. This was a ‘white light’ flare, a type of flare that displays associated brightening in the visible light spectrum. Astronomers believe flares are driven by magnetic energy, the sudden release of which can cause charged particles to heat plasma. In this case the resulting optical, ultraviolet and X-ray radiation was copious.

James Jackman, a PhD student in physics at the University of Warwick (UK) and lead author of the paper on these observations, points to the rare nature of this flare:

“The activity of low mass stars decreases as you go to lower and lower masses and we expect the chromosphere (a region of the star which support flares) to get cooler or weaker. The fact that we’ve observed this incredibly low mass star, where the chromosphere should be almost at its weakest, but we have a white-light flare occurring, shows that strong magnetic activity can still persist down to this level.”

Image: A superflare on an L-dwarf. Credit & Copyright: University of Warwick/Mark Garlick.

And note this from the paper on this work, on the unusual strength of some L dwarf flares:

While seen regularly on GKM stars, observations of white-light flares on L dwarfs remain rare, with only a handful of stars showing them to date (e.g. Paudel et al. 2018). However, those observed have included some of the largest amplitude flares ever recorded, reaching up to V ≈ −11 (Schmidt et al. 2016). This shows that white-light flaring activity persists into the L spectral type, despite previous studies of L dwarfs showing their chromospheres and magnetic activity to be diminished compared to those of late M dwarfs.

So a borderline brown dwarf/star is giving us an interesting lesson, perhaps on the difference between the two, because we may be able to determine whether flares like these are limited to actual stars, learning at just what point the activity ceases. Are there other tiny stars, like ULAS J224940.13-011236.9 about the same size as Jupiter, that mark the limits of such flares, below which none occur? Whatever the case, few L dwarfs have produced a flare of this magnitude.

Embedded in future work will surely be the question of how tiny stars like this one store energy in magnetic fields, and their level of chromospheric activity. From the paper:

Ultracool dwarfs are also known to exhibit auroral activity…, which may account for observed Hα [hydrogen alpha] emission [when a hydrogen electron falls from its third to second lowest energy level], in these systems. It is expected that the transition from predominantly chromospheric to auroral Hα emission occurs during the L spectral type… Many ultracool dwarfs that show activity such as radio emission and flaring also tend to be fast rotators, with rotation periods on the order of hours. However, neither the L1 dwarf SDSSp J005406.55−003101.8 (Gizis et al. 2017a) nor the L0 dwarf J12321827−0951502 (Paudel et al. 2018) showed any sign of rapid rotation when observed by K2, despite showing large amplitude white-light flares. Consequently, we do not attempt to predict whether ULAS J2249−0112 is a fast rotator. Regardless of this, studies of white-light flares such as from ULAS J2249−0112 can aid in understanding exactly how far into the L spectral type chromospheric activity persists.

The J224940.13-011236.9 data come from the Next Generation Transit Survey (NGTS) facility at the European Southern Observatory’s Paranal Observatory, with further data from the Two Micron All Sky Survey (2MASS) and Wide-field Infrared Survey Explorer (WISE), a total observation period of 146 days. The flare occurred on 13 August 2017, with an energy equivalent of 80 billion megatonnes of TNT, surpassing the largest flare (the Carrington event of 1859) ever observed on the Sun.

The paper is Jackman et al., “Detection of a giant white-light flare on an L2.5 dwarf with the Next Generation Transit Survey,” Monthly Notices of the Royal Astronomical Society: Letters Vol. 485, Issue 1 (May 2019), L136-L140 (abstract).

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Chinese Mission to an Earth Co-Orbital

This morning’s entry resonates with Jim Benford’s recent work on objects that are co-orbital with Earth (see A SETI Search of Earth’s Co-Orbitals). You’ll recall that Benford argues for close study of co-orbitals like Cruithne (3753), a 5-kilometer object with closest approach to Earth of 0.080 AU, and 2010 TK7, which oscillates around the Sun-Earth Lagrangian point L4. A number of other such objects are known in a 1:1 orbital resonance with Earth, but they are seldom studied or even mentioned in the literature.

Calling for SETI observations at radio and optical wavelengths, as well as lighting up the objects with planetary radar, Benford gives a nod to Ronald Bracewell, who speculated that one way for an extraterrestrial intelligence to study a stellar system would be to plant a probe within it that could inform the home civilization about events there. The Earth co-orbitals are made to order for such observation, so why not give them a look with all the tools in our SETI arsenal?

Now we learn that China plans to explore the near-Earth asteroid 2016 HO3, along with a main-belt comet designated 133P. An interesting move — 2016 HO3 is the closest, most stable quasi-satellite of Earth, with a minimum distance of 0.0348 AU. Also known as Kamoʻoalewa — a Hawaiian word for an oscillating object in the sky — 2016 HO3 has a minimum orbital intersection distance of 0.0348 AU (5,210,000) km, which is 13.6 times as far away as the Moon, although it seldom comes closer than about 38 lunar distances from us. The Center for Near Earth Object Studies (CNEOS) calculates this one has been in a stable orbit of our planet for about a century and will remain in its orbital pattern for centuries.

Image: Orbit of 2016 HO3. Credit: James Benford.

According to Liu Jizhong, director of the Lunar Exploration and Space Program Center of the China National Space Administration (CNSA), the current plan is to study 2016 HO3 from space before landing on it to collect samples for return to Earth. Following delivery of the sample return capsule, the probe is to proceed to comet 133P by means of gravity assists at Earth and Mars, in a mission lasting on the order of 10 years.

China is now soliciting proposals for eight types of scientific instruments for the mission among universities, research organizations and private companies both in China and abroad, according to a CNSA news release. Among the instruments needed, Liu says, are a color camera with an intermediate field of view, thermal emission spectrometer, visible and infrared imaging spectrometer, multispectral camera, detection radar, magnetometer, charged and neutral particle analyzer and dust analyzer. Quoting from the news release:

[Liu] said there might be two forms of onboard schemes. One possible scheme is to carry an independent detector on the rocket. After China’s main probe enters the orbit, the onboard detector will separate from the rocket and then perform independent tasks. Its mass should not exceed 200 kg. The other possible option is to let China’s main probe carry the onboard detector to the near-Earth asteroid or the main-belt comet and then release it. The detector could either perform independent scientific exploration or coordinate with the main probe.

If the onboard detector does not separate with the main probe, its mass should not exceed 20 kg. If the detector separates from the main probe near the asteroid, its mass should be no more than 80 kg. If it separates from the main probe near the comet, its mass should not exceed 20 kg.

The deadline for proposals is August 31, 2019, with those interested asked to contact CNSA.

Image: An animation of 2016 HO3’s orbit around Earth 2000-2300. Credit: Phoenix7777 – Own work. Data source: HORIZONS System, JPL, NASA. CC BY-SA 4.0.

This will not be China’s first experience with an asteroid mission. In December of 2012, its second lunar probe, Chang’e-2, made a close approach and flyby of asteroid 4179 Toutatis after completing its primary mission, approaching to within 3.2 kilometers and returning images. Now we have an ambitious mission to give us a close-up look at an Earth co-orbital, with comet operations to follow. We should learn a lot, for right now even the size of 2016 HO3 is not firmly established, though it is believed to be between 40 and 100 meters, depending on assumptions about its albedo, and we do know that it is a fast rotator.

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