Centauri Dreams

Imagining and Planning Interstellar Exploration

HD 7449Ab: Choreography of a Planetary Dance

Given this site’s predilections, it’s natural to think of Centauri A and B whenever the topic of planets around close binary stars comes up. But systems with somewhat similar configurations can produce equally interesting results. Take what we’re finding around the G-class star HD 7449, some 127 light years from our Sun. In 2011, a planet of roughly eight times Jupiter’s mass was found orbiting the star in an orbit so eccentric that it demanded explanation. A highly eccentric orbit can indicate another object in the system that is affecting the planet.

Exactly what has now been determined. “The question was: is it a planet or a dwarf star?” says Timothy Rodigas (Carnegie Institution for Science), who led the work on the discovery. Rodigas’ team went to work using the Magellan adaptive optics system (MagAO) on the Magellan II (Clay) instrument at Las Campanas in Chile. MagAO allows sharp visible-light images to be acquired, with the instrument capable of resolving objects down to the 0.02 arcsecond level.

The object near HD 7449 was quickly spotted and we learn that the system has a second star, an M-class dwarf. So now we have HD 7449A and the dwarf secondary, HD 7449B, along with the gas giant HD 7449Ab. HD 7449B is a tiny object with about one-twentieth the Sun’s mass, and it’s close enough to the primary (18 AU) to evoke that Alpha Centauri comparison I made above — Centauri A and B move between 11.4 and 36.0 AU as they orbit. I’ll grant that the comparison is strained by the fact that Centauri B is a K-class dwarf, while HD 7449B is a far smaller M-dwarf. Moreover, we have nothing like planet HD 7449Ab in the Alpha Centauri system.

What we’re seeing in HD 7449Ab is a planet that in the words of Rodigas is “‘dancing’ between the two stars.” The gravitational influences at work here evidently go back millions of years. The system, in fact, may be showing us the so-called Kozai mechanism at work. First described by the Russian astronomer Michael Lidov and later by Japanese researcher Yoshihide Kozai, the Kozai mechanism is one factor that can shapes the orbits of multiple-star systems. We see an oscillation between the planet’s orbital eccentricity and its orbital inclination, the ‘dance’ that Rodigas refers to. Have a look at the team’s visualization of the effect.

Image: This animation shows the Kozai mechanism at work in the HD 7449 system. Credit: Carnegie Institution for Science.

From the paper:

If the planet and outer companion were initially on mutually-inclined orbits of at least 39.2°, then the planet’s eccentricity and inclination would oscillate with oppositely-occurring minima and maxima (Holman et al. 1997). Based on the nominal parameters for the planet and M dwarf companion, the length of a Kozai cycle would be ? a few hundred years, which is certainly short enough to be plausible given the age of the system (? 2 Gyr).

The Kozai mechanism is not the only explanation for the planet’s eccentric orbit, but the paper argues that it is the most convincing:

Another explanation for the planet’s large eccentricity is planet-planet scattering in the inner parts of the system (e.g., Rasio & Ford 1996). In this case, one or more planets may have been ejected from the system, leaving behind the eccentric HD 7449Ab. This scattering scenario would require both the surviving planet and the scattered planet to be relatively massive (7–10 MJ ) and the eccentricity damping of the original circumstellar disk to be small (Moorhead & Adams 2005). Given the “smoking gun” (the nearby M dwarf companion), it seems more likely that Kozai cycles are responsible.

The paper calls for continuing monitoring of this system by both radial velocity and direct imaging methods, the latter important because it can provide further constraints on the planet’s orbital eccentricity and inclination, allowing for a more accurate estimate of its mass. The dwarf star is itself interesting, the paper noting that it can become a benchmark object for studies of stellar structure. What this system gives us is a rare case of an M-dwarf with a measurable age (via the primary) and a mass that will be measured by astrometric means. Spectroscopic follow-up should constrain metallicity, improving structure models for similar cool stars.

The paper is Rodigas et al., “MagAO Imaging of Long-period Objects (MILO). I. A Benchmark M Dwarf Companion Exciting a Massive Planet around the Sun-like Star HD 7449,” accepted at The Astrophysical Journal (preprint). Thanks to Dave Moore for alerting me to this story.

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Globular Clusters: Home to Intelligent Life?

I can think of few things as spectacular as a globular cluster. Messier 5 is a stunning example in Serpens. With a radius of some 200 light years, M5 shines by the light of half a million stars, and at 13 billion years old, it’s one of the older globular clusters associated with our galaxy. Clusters like these orbit the galactic core, stunning chandeliers of light packed tightly with stars. The Milky Way has 158 known globulars, while M31, the Andromeda galaxy, boasts as many as 500. Giant elliptical galaxies like M87 can have thousands.

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Image: The globular cluster Messier 5, consisting of hundreds of thousands of stars. Credit: ESA/Hubble & NASA. Via Wikimedia Commons.

Given the age of globular clusters (an average of ten billion years), it’s a natural assumption that planets within them are going to be rare. We would expect their stars to contain few of the heavy elements demanded by planets, since elements like iron and silicon are created by earlier stellar generations. And indeed, only one globular cluster planet has been found, an apparent gas giant that accompanies a white dwarf, both orbiting a pulsar in the globular cluster M4.

A team led by David Weldrake (Max-Planck-Institut für Astronomie) reported on its large ground-based search for ‘hot Jupiters’ in the globular clusters 47 Tucanae and Omega Centauri in 2006, finding no candidates. So should we give up on the notion of planets in such environments? Rosanne Di Stefano (Harvard-Smithsonian Center for Astrophysics) thinks that would be premature. She presented the research at a press conference at the ongoing meeting of the American Astronomical Society, which this year occurs in Kissimmee, Florida.

Working with Alak Ray (Tata Institute of Fundamental Research, Mumbai), Di Stefano points out that we have found low-metallicity stars known to have planets elsewhere in the galaxy. And while we can couple the occurrence of Jupiter-class planets with stars that have higher metallicity, there seems to be no such correlation when we’re dealing with smaller, rocky worlds like the Earth. Perhaps, then, we shouldn’t dismiss planets in globular clusters.

Di Stefano also argues that while stellar distances are small within a globular cluster, this may not work against the possibility of habitable planets, and may actually be a benefit for any civilizations that do emerge there. Most of the stars in these ancient clusters are red dwarfs with lifetimes in the trillions of years. The habitable zone around such small stars is close in, making potentially habitable worlds relatively safe from disastrous stellar interactions.

So let’s imagine the possibility of life evolving in ten billion year old globulars. In our comparatively sparse region of the Milky Way, the nearest star is presently some 4.2 light years away, a staggering 40 trillion kilometers. Within a large globular cluster, the nearest star could be twenty times closer. Imagine a star at roughly 15000 AU or somewhat less, about the same distance from our Sun as Proxima Centauri is from Centauri A and B. Then open out the view: Imagine fully 10,000 stars closer to us than Alpha Centauri, the night sky ablaze.

I would see this as a powerful inducement to developing interstellar technologies for any civilization that happened to emerge, and Di Stefano agrees, according to this CfA news release. The ‘globular cluster opportunity’ that she identifies would play off the fact that broadcasting messages to nearby stars would presume round-trip travel times not a lot longer than it took to get letters from the United States to Europe in the 18th Century by sail.

As to this site’s own idée fixe, Stefano sees further good news:

“Interstellar travel would take less time too. The Voyager probes are 100 billion miles from Earth, or one-tenth as far as it would take to reach the closest star if we lived in a globular cluster. That means sending an interstellar probe is something a civilization at our technological level could do in a globular cluster.”

That does give me pause — imagine one of our Voyagers already a tenth of the way to another star. If civilizations can develop inside globular clusters, they could be just what Di Stefano says, “the first place in which intelligent life is identified in our galaxy.” The problem for our current exoplanet methods is that even the closest globular cluster is a long way from us — both M4 and NGC 6397 are approximately 7200 light years out. Gravitational microlensing may produce some planetary finds, and perhaps new transit efforts could be effective, though we would be working on the outskirts of the cluster and small rocky worlds would be a tough catch.

Even so, it’s a breathtaking prospect, because my imagination is fired by the possibility of intelligent life looking out on a sky packed with stars from the center of a globular cluster. I also take heart from the fact that there is much we don’t know about such clusters. M5, for example, dates back close to the beginning of our universe, yet we know that along with its ancient stars, it also has a population of the young blue stars called ‘blue stragglers.’ Explaining their formation should help us better understand the dynamics of this dazzling environment.

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Stellar Age: Recalibrating Our Tools

Making the call on the age of a star is tricky business. Yet we need to master the technique, for stellar age is a window into a star’s astrophysical properties, important in themselves and for understanding the star in the context of its interstellar environment. And for those of us who look at SETI and related issues, the age of a star can be a key factor — is the star old enough to have produced life on its planets, and perhaps a technological civilization?

Until recently, luminosity and surface temperature were the properties that helped us make a rough estimate of a star’s age, which gives insight into how challenging the problem is. These are factors that, while they do change over time, give us only approximations of age. More recently, researchers have learned to study sound waves deep in the stellar interior, a method that is confined to bright targets and cannot help us with vast numbers of dimmer stars. Called asteroseismology, this method has helped our estimates of stellar ages among old field stars.

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Enter gyrochronology. Within the last decade, we’ve learned that stellar rotation rates can help us with a star’s age, for a star’s spin is slowed due to the interactions between its magnetic field and its stellar wind. The latter, a flow of charged particles moving away from the star, helps to inflate the ‘bubble’ in our system we know as the heliosphere. But these gases also become caught in the magnetic field as they spin outward, causing changes to the star’s angular momentum.

Thus a star’s magnetic field can over time brake its spin rate. Assuming we know the rotation rate and mass of the star, we can use the method to calculate its age. Now we have new work out of the Carnegie Institution for Science that should be helpful at refining this technique. What Jennifer van Saders and team have discovered is that our models for predicting the slowdown have been off. The braking action of the magnetic field becomes weaker as stars get older, becoming much less accurate for stars more than halfway through their lifetimes.

Image: Solar image courtesy of NASA’s Solar Dynamics Observatory.

Appearing in Nature, the paper is based on data from the Kepler spacecraft, which makes it possible to test gyrochronology for a large number of stars older than the Sun. Kepler gives us a significant sample of stars whose rotation rate is measurable and whose asteroseismic properties are now known.

If, as appears the case, there is a change in the way the magnetic field interacts with the stellar wind as a star ages, then we need to find out the nature of this change and when it occurs. In any case, we have hard data that stars more evolved than the Sun rotate more rapidly than our models predict, a fact that limits the usefulness of gyrochronology in these populations. Our own Sun could be approaching the age when its magnetic field loses some of its braking power.

Bear in mind that we are talking about astronomical timescales here, so whatever transition occurs may not happen for hundreds of millions of years. Moreover, the changes to the magnetic interactions are likely to take place over a long period. But the speed of the change and the process behind it point the way to future work as we try to unwrap the riddle of stellar ages. “Gyrochronology,” says van Saders, ” has the potential to be a very precise method for determining the ages of the average Sun-like star, provided we can get the calibrations correct.”

The paper is van Saders et al., “Weakened magnetic braking as the origin of anomalously rapid rotation in old field stars,” published online in Nature 4 January 2016 (abstract). Be aware as well of van Saders er al., “Rotation periods and seismic ages of KOIs – comparison with stars without detected planets from Kepler observations,” published online by Monthly Notices of the Royal Astronomical Society 11 December 2015 (abstract). This one deals with using Kepler Objects of Interest to calibrate gyrochronology, concluding that planet-hosting stars show rotational patterns similar to that of stars without any detected planets.

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‘A City Near Centaurus’

Let’s start the year off with a reflection on things past. Specifically, a story called “A City Near Centaurus,” set on a planet circling one of the Alpha Centauri stars. Just which star is problematic, because our author, Bill Doede, describes it as a planet circling ‘Alpha Centaurus II.’ I’m sure he means Centauri B, but the story, which appeared in Galaxy at the end of Frederick Pohl’s first year as editor, is less concerned about nomenclature and setting than the conflict between a humanoid alien called Maota and the timeless city he lives in.

Michaelson, our human protagonist, looks out upon this long deserted metropolis:

He gazed out from his position at the complex variety of buildings before him. Some were small, obviously homes. Others were huge with tall, frail spires standing against the pale blue sky. Square buildings, ellipsoid, spheroid. Beautiful, dream-stuff bridges connected tall, conical towers, bridges that still swung in the wind after half a million years. Late afternoon sunlight shone against ebony surfaces. The sands of many centuries had blown down the wide streets and filled the doorways. Desert plants grew from roofs of smaller buildings.

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Maota is a humanoid who, fortunately for the reader and Michaelson, speaks English, evidently one of the few who remain half a million years after whatever has caused the disappearance of a once great civilization. If anything, this should remind you of Bradbury’s The Martian Chronicles, whose ancient cities shaped many a young imagination, but Doede’s story likewise has a bit of J. G. Ballard in it, this at a time when Ballard was being introduced to America by Cele Goldsmith, the brilliant editor of Amazing Stories and Fantastic. The early 1960s were truly fecund years for science fiction.

Disturbing a Living Past

I introduce Doede’s story today as a bit of a jeu d’espirit, but also out of genuine curiosity. I had thought I had read every story or novel dealing with the Centauri stars at one point or another. And indeed, I know for a fact that I read the October 1962 issue of Galaxy, for reasons I’ll explain in a moment. But when I stumbled across “A City Near Centaurus” over the weekend, it was by way of a chance encounter on Project Gutenberg, where the tale, its copyright never renewed, is now available. I therefore read it with fresh eyes.

We’re asked to swallow a lot if we’re dealing with humanoids on an alien world, although bear with the tale. To my mind, it’s spritely done and could easily be imagined as a TV script for Rod Serling’s Twilight Zone, a tale plucking at a kind of moral lesion in what it means to explore and encounter not just the alien but the past. Maota wants Michaelson to leave the city alone, fearing his amateur archeology will disrupt the spirits of the dead.

“What difference does it make?” Maota cried, suddenly angry. “You want to close up all these things in boxes for a posterity who may have no slightest feeling or appreciation. I want to leave the city as it is, for spirits whose existence I cannot prove.”

For his part, Michaelson is as clumsy as Schliemann at Troy, but he wants to know what made this culture tick. The tension is heightened by the fact that these two are alone in the deserted city.

Along the way we encounter an ancient book that seems to communicate telepathically. We also learn that Michaelson possesses a technology that allows teleportation, in the form of a small implant behind his ear that lets him be more or less wherever he chooses to be. Inevitably, although Maota is old, he and Michaelson fight both verbally and physically, and the book is destroyed. The old man then reveals what happened to the civilization once here:

Maota smiled a toothless, superior smile. “What do you suppose happened to this race?”

“You tell me.”

“They took the unknown direction. The books speak of it. I don’t know how the instrument works, but one thing is certain. The race did not die out, as a species becomes extinct.”

Michaelson was amused, but interested. “Something like a fourth dimension?”

“I don’t know. I only know that with this instrument there is no death. I have read the books that speak of this race, this wonderful people who conquered all disease, who explored all the mysteries of science, who devised this machine to cheat death. See this button here on the face of the instrument? Press the button, and….”

“And what?”

“I don’t know, exactly. But I have lived many years. I have walked the streets of this city and wondered, and wanted to press the button. Now I will do so.”

It would be churlish to give away what happens next, but it’s clear that the city lives, and that the tension between inevitable change and the urge to preserve what has been infuses even our encounter with beings from another star. Reading “A City Near Centaurus,” I became intrigued enough to look for information on Bill Doede. Biographical data didn’t emerge, though the The Internet Speculative Fiction Database did reveal that he published four other tales between 1960 and 1964, all in Galaxy save one for Fred Pohl’s fledgling Worlds of Tomorrow in early 1964. Clearly, he was an H. L. Gold discovery who managed a working relationship with Pohl after the editorial handoff of Galaxy in 1961.

Riffing on the Future

Some of us keep old magazines and collect others because the pleasures of science fiction from this era were so intense, and in any case, we all gravitate to the better memories of our childhood. I mentioned that I was sure I had read the issue of Galaxy that “A City Near Centaurus” appeared in, and that’s because the lead story in the issue was Cordwainer Smith’s “The Ballad of Lost C’Mell.” I envy those who haven’t made an acquaintance with Smith’s work — he was actually a well-traveled diplomat (and sometime spy) named Paul Linebarger, who led a life fully as interesting as some of his astonishing fiction.

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I remember where I was when I read most of Cordwainer Smith’s fiction for the first time, and though I don’t remember Bill Doede, I’m pleased to have recovered another story dealing in some way with our nearest stars. On a broader note, I was thinking this weekend, as I listened to a Bobby Hutcherson album while reading Doede, that jazz and science fiction have much in common. Whether keying off chord changes or moving in a modal direction (as in Miles Davis’ wonderful work from the same era as the Doede story), jazz gives musicians ways to explore sound, with no two performances representing the same idea. Listen to Davis, for example, doing the classic “Milestones” on the album of the same name and then compare the performance with his take on the same piece on Miles Davis In Europe.

It’s the same composition, but taken in entirely different directions — the accelerated tempo of the latter, recorded at the Antibes Jazz Festival, pushes the piece to its limits. Like jazz, science fiction shapes its materials — elements of emerging science — and plays speculative changes with and against them. We invent a future and explore it, tweak it and explore it again, a riffing of ideas that helps us see possible directions for our species. As we begin 2016, I ask myself what changes we’ll play off in the coming year, secure in the knowledge that there is no terminus. In some ways we are always, as David Deutsch would say, at the beginning of infinity.

Addendum: Jon Lomberg passed along the beautiful artwork below, his visualization of Earthport, from Cordwainer Smith’s “Ballad of Lost C’Mell,” by way of letting me know he’s also a great fan of the author’s work. Jon also sent a scrupulously detailed chart of Smith’s fictional universe that I couldn’t get to display well due to the limitations of the format here, but have a look at Earthport. Jon’s art can be viewed in considerably more detail at http://www.jonlomberg.com/.

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Can Social Insects Have a Civilization?

I first encountered Michael Chorost in his fine book World Wide Mind (Free Press, 2011), which looks at the relationship between biology and the machine tools that can enhance it. Mike’s thinking on SETI has already produced rich discussion in these pages (see, for example, SETI: Contact and Enigma). In today’s essay, he’s asking for reader reactions to the provocative ideas on insect memory and intelligence that will inform his next book. While it does not happen on Earth, can evolution invent — somewhere — a social insect society capable of long-term memory and civilization? A nearby planet evidently hostile to our kind of life offers fertile ground for speculation.

by Michael Chorost

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I’ve admired Paul Gilster’s Centauri Dreams for many months and I’ve always been impressed by the quality of the comments. Paul graciously allowed me to write a guest entry to test one of my book-in-progress’s ideas on a smart audience — you.

This book-in-progress will be my third book. My first two books were about bionics and neuroengineering, respectively titled Rebuilt (Houghton Mifflin, 2005) and World Wide Mind (Free Press, 2011.) I’ve also published in Wired, New Scientist, Slate, Technology Review, the Chronicle of Higher Education, and Astronomy Now.

The book is about communication with extraterrestrials. Not by radio but in person, with us visiting their planet and looking at their mugs (or whatever they have instead of mugs). How should we begin trying to communicate? What could we safely assume — and not assume — about how minds think? What knowledge could we bring to bear from evolutionary theory, linguistics, cognitive science, and computer science?

Of course, direct contact anytime soon is unlikely in the extreme. That’s why, below the surface, the book is about a deeper set of issues: What are the universals of thought and language? Can intelligent minds be so different as to render communication impossible? What kinds of advanced cognition can an evolutionary process invent? The book gets at these ideas by using alien communication as a vehicle.

So here’s the idea I want to test on you all. I asked myself, “Would it be possible for social insect colonies on some other planet to evolve to have language and technology – in other words, a civilization?”

Of course, the idea of swarm intelligence, or hive-mind intelligence, has been around forever in science fiction. To give but one example, Frank Schatzing’s The Swarm posits an undersea alien made of single-celled, physically unconnected organisms that collectively have considerable intelligence. But I need to examine the idea with much more rigor than can be done in fiction.

I refined the question by deciding that, as on earth, the individual insects would have brains too small for serious cognition. The unit of analysis would not be individual bugs but colonies of bugs. The intelligence would have to emerge from their interaction.

After much thought, my answer to the question is “No – but…”

Let me explain both the No and the but. It is these explanations on which I want your feedback.

To start with the No. I don’t think it’s possible for physically separate units to form a collective that supports high intelligence. The reason is straightforward: physically disconnected units have no way of permanently storing large amounts of discrete information in a way that is available to the collective. More succinctly, they can’t support long-term memory.

Of course, information can be manipulated by collectives even when the units have no permanent connections among them. If you’ve read Douglas Hofstadter’s “Ant Fugue” you know how ant colonies collectively find and consume food. A forager comes across food and lays a pheromone trail while returning to the nest. Other workers follow that trail and lay down pheromones of their own. When the food is gone the returning ants stop emitting pheromones, and the ants move on to other things. From a global perspective it looks as if the colony has a “memory” of the food source. Insect colonies have many mechanisms of this sort, which go under names like “stigmergy” and “quorum sensing.” They are brilliantly described in the literature, especially by Thomas Seeley. [1] But all of them yield only short-term memory. As soon as the insects disperse and the pheromone evaporates, the information vanishes.

That is a problem, because language and other forms of advanced cognition need long-term memory. Language requires storing a large number of primitives (e.g. words) plus state information related to a conversation (the identity of the interlocutor, the situation, information about past and future, and so forth.) Not only that, the method of storage has to be both stable and easily changeable. If it can’t be changed, an intelligence can’t keep up with changing events in the world.

Let me pause here to define what I mean by “intelligence” and “language.”

I like the definition of intelligence offered by Luke Muehlhauser in his book Facing The Intelligence Explosion. [2] He defines it as “efficient cross-domain optimization.” Cross-domain optimization refers to being able to exercise intelligence in multiple domains. Consider that IBM’s Deep Blue program is very smart at chess but can’t play checkers, let alone want to learn how. It has intelligence in one domain, and only one. Or take honeybees, who are outstanding at communicating the location of food but have no way of asking humans to move that food closer, or change it. In order to cross domains a mind needs not just cognition but metacognition, the ability to think about thinking. When I speak of intelligence I mean the kind that can reflect upon its own actions, make plans, describe things that don’t exist, and so forth. This is the kind of intelligence that is required to build a civilization.

Now language. I like Steven Pinker’s definition of it: Language is a finite set of primitives that when combined yield an infinite number of possible statements. [3] By this definition, language is open-ended. It can be used to say anything. Contrast that to, say, referee signals in baseball. They are a communication system but not a language. A referee can precisely say whether a pitch is a ball or strike, but he can’t use the repertoire of signs to talk about taxes, or explain that the pitcher has just become a free agent. Likewise, a honeybee can precisely state where food is but can’t use its waggle dance to discuss the weather with a human. Animals such as honeybees, birds, chimps, dolphins, parrots, and dogs all have communications systems, some of which are very sophisticated, but they are closed-ended; they do not rise to the level of language.

Now that I have defined intelligence and language, please note that both of them simply have to have long-term memory. Without long-term memory, no intelligence, no language. And I don’t think there is any way at all that a social insect colony can get long-term memory if its units are physically disconnected. It has no physical medium in which it can store information in a way that is both permanent and easily changed.

So, Conclusion A: Social insect colonies do not have the memory mechanisms to support language, therefore no bug civilizations.

Now let’s get to the “but.” After working out Conclusion A I asked myself, “Could insect colonies acquire, through an evolutionary process, a mechanism of long-term memory?” I think the answer to that question is yes.

Consider how mammalian brains store long-term memory: in collections of synapses. A synapse is a physical gap between the axon of one neuron and the dendrite of another. Depending on the strength of an incoming signal and the synapse’s threshold, neurotransmitters either flood into that gap or they don’t. If they do, they are picked up – essentially “smelled” – by chemoreceptors on the dendrite’s side. Then the signal continues to the body of the next neuron, which uses it as an input for its own decision-making process.

Each neuron in a mammalian brain has thousands of synaptic connections to other neurons – it is part of an immense network of physically connected units. By changing synaptic configurations and thresholds, neurons can encode immense amounts of discrete information. That information is both stable and easily changeable.

So for an insect colony to gain long-term memory, it has to invent the equivalent of the synapse. Not in the brains of individual insects – they already have plenty – but on the level of the colony as a whole, using interactions between insects.

This is obviously tricky because insects move around. But there are insects in colonies that don’t move around: the larvae. Even better, in flying insect colonies they are generally stored in honeycombs that keep them in place. And better still, they’re loaded with chemoreceptors. The ends of antennae and feet are the “noses” by which insects pick up smells.

Imagine, then, the antennae and feet of developing larvae thrusting their way through the waxen walls of honeycombs and making contact with the antennae and feet of their neighbors. Right there you have the basic elements of synaptic connections. If the larvae can send signals and adjust synaptic thresholds, they could form a network.

Of course, there has to be an evolutionary reason why such a network would ever come into being. There would have to be accidental variations that create primitive networks, and they would have to confer fitness and reproduction benefits.

So consider this story of an evolutionary process. It so happens that in some kinds of colonies, the larvae perform a digestive function for the colony. The workers bring them the food that they can’t digest, and the larvae break them down into compounds the workers can eat. [4] So the larvae are effectively the colony’s stomach. The food needs of workers vary depending on temperature and season and so forth. Larvae that could exchange information with other larvae about digestion could produce better food, and that benefit would tend to be conserved and amplified. Over many generations, then, colonial stomachs could evolve into colonial brains. Each larva would be a large neuron with many connections to other larvae, and the synaptic configurations between them would store long-term memories.

This is, of course, a just-so story – but then evolution is full of just-so stories of evolutionary adaptations that seem spectacularly improbable. For example, insect wings are thought to be adapted legs. [5] And insects have often evolved to look like leaves and twigs for camouflage. Nature is astonishingly inventive at reshuffling its building blocks. I am not trying to convince you that my larvae-to-brains story is likely, only that it is possible.

There is one more piece to the puzzle. Long-term memory is metabolically and spatially expensive. Clearly, on Earth insect colonies have seen no need to develop it; they’ve done well for millions of years without it. So you need to have an environment in which it would confer fitness advantages.

Consider the planet GJ832c.

GJ832c is a rocky planet of 5.4 Earth masses orbiting a red dwarf star sixteen light-years away. Happily, it’s in the star’s habitable zone. Since a red dwarf is very dim the habitable zone has to be very close to it, and accordingly GJ832c has a year just 36 days long. [6]

We don’t know much about GJ832c. We don’t know its density, so we don’t know its surface gravity. But I’ve guessed that it’s 78% as dense as Earth, which would give it a surface gravity of 1.5 gees. We don’t know its rotational period, but since it’s so close to its star it would probably be gravitationally locked. Mercury has a 3:2 spin-orbit resonance, which means that it rotates three times every two years. So let’s say that GJ832c also has a 3:2 spin-orbit resonance.

We don’t know its axial tilt, but gravitational locking tends to stabilize axial tilt near zero – Mercury’s is just two degrees, and the Moon’s is 6.6 degrees, compared to the Earth’s 23 degrees. So let’s say its axial tilt is zero. But we do know its orbital eccentricity, .18, which is very eccentric by our solar system’s standards.

If you put these facts and guesses together you can compute how much solar exposure each point on such a planet gets, like so:

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Astonishingly, on such a planet the climate is determined as much by longitude as latitude. Yes, longitude. Some longitudes are in daylight for long periods, while other longitudes never see the sun at all – including a few points on the equator. The planet looks like a tennis ball with burns on opposite sides (red), a temperate zone ringing the burns (yellow), and ice everywhere else (blue). [7]

To be sure, the temperature extremes would be moderated by the atmosphere. My guess is that you would see Hadley cells centered on the hot zones, since the hot air would rise and cold air would come in underneath it. Since the planet rotates so slowly, you wouldn’t see much Coriolis force to shear the atmosphere sideways. So there would probably be steady winds moving toward the center of each hot zone, distributing heat between the zones.

Note, however, that only one “hot” end can face the star at any given moment. The center of each hot zone would face the star continuously for blistering days on end, and then suffer a long night. (I haven’t worked out what the day-night cycle would look like on various points of the planet. Perhaps the temperate zones would be in continuous but relatively soft illumination. For this I need the help of someone who specializes in orbital dynamics.)

In any case, GJ832c would be a nasty planet. It’d have high gravity, temperature extremes, constant wind, and possibly a thick atmosphere and ultraviolet flares from its star. I don’t think you would get large-brained mammals here simply because of the gravity: blood circulation and locomotion would be expensive. Predator actions like leaping and throwing things would be difficult. So would prey defenses like running and climbing.

What would flourish here? Bugs. Bugs are modular, tough, and cheap. They are small enough to be relatively unaffected by gravity, and their chitinous exoskeletons would be relatively impervious to UV flares.

So let’s say that social insect colonies evolve in the temperate zone. But the temperate zone is exceedingly narrow, perhaps just a few hundred miles across. Sooner or later population pressures are going to drive new colonies into the hot and cold zones. There, new colonies could find resources that aren’t in the temperate zone, say particular kinds of hothouse flowers, lichens, and fungi. And they would face new scarcities too, say of water.

On GJ832c, colonies that learned to trade resources across zones would have an enormous survival advantage. Water for nectar, nectar for fungus, and so on. Insects on Earth have signaling mechanisms that could be adapted to manage such trades. For example, they engage in territorial displays in which soldiers posture at the borders between colonies, inflating their limbs to seem more threatening, while “head-counting” ants on each side carry information about the enemy back to the nest. (They probably don’t actually count the soldiers using numerals; more likely they sense the rate of encounters with them.) [8] Such signaling mechanisms could be adapted to convey information for economic exchanges. Colonial brains would store such information, remembering who traded what and for how much. Over many generations, such signaling systems could evolve into language.

You may wonder about tools, since tools have fundamentally shaped the development of language in humans. For brevity’s sake I won’t go into it here, but I’ve worked out how insect colonies could ignite fire, forge metals, and use tools; again, I’ve extrapolated from things social insects do on Earth. With language and tools a species is just a few hops, skips, and jumps away from having a full-fledged civilization.

This doesn’t mean they would think like humans, of course. They would have networks that can support long-term memory, but those networks would have a very different organization and would support very different kinds of physical needs. In the manuscript I discuss the role of simulation and embodied cognition on the development of language.

So, Conclusion B: With the right environmental pressures, social insects could develop long-term memory, language, tool use, and a civilization.

Again, I am not arguing that this is likely, only that it is possible. What do you think? Am I correct in thinking it is possible, or is there something fundamental that I am neglecting?

I’m asking you to put pressure on these ideas. To look for their weak spots. But I would also appreciate it if, for each weak spot, you could suggest a solution, if you can think of one.

Many thanks in advance for your comments and ideas.

——-

Footnotes

1. Seeley, Thomas (2010). Honeybee Democracy, Princeton.

2. Muehlhauser, Luke (2013). Facing The Intelligence Explosion. Machine Intelligence Research Institute. Kindle location 655.

3. Pinker, Steven (2007.) The Language Instinct: How the Mind Creates Language. Harper Perennial, p. 75.

4. Masuko, Keiichi (1986). “Larval hemolymph feeding: a nondestructive parental cannibalism in the primitive ant Amblyopone silvestrii Wheeler (Hymenoptera: Formicidae).” Behav Ecol Sociobiol 19: 249-255. See also http://blog.wildaboutants.com/2010/06/21/question-1-ant-digestion/.

5. Carroll, Sean (2006). Endless Forms Most Beautiful: The New Science of Evo Devo. Norton, p. 176.

6. Planetary Habitability Laboratory data for GJ832c, http://www.hpcf.upr.edu/~abel/phl/hec_plots/hec_orbit/hec_orbit_GJ_832_c.png

7. Brown et al. (2014). “Photosynthetic Potential of Planets in 3:2 Spin Orbit Resonances.” International Journal of Astrobiology 13:4 (279-289). Page 284. I’ve used the figure computed for an eccentricity of 0.2, which I figure is close enough.

8. Hölldobler, B., and Wilson E. O. (2008). The Superorganism: The Beauty, Elegance, and Strangeness of Insect Societies. New York: W. W. Norton, p. 306.

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‘Time Delays’ and Exploding Stars

With our focus on nearby stars for both exoplanet detection and SETI work, I don’t often find the time to talk about cosmology and ‘deep sky’ observations, although galaxy structure and formation are an interest of mine. But today I have a story too good to pass up, involving using gravitational lensing and time delays in how light reaches us to investigate events at the edge of the visible universe. In such work, the curvature of spacetime itself is part of our toolkit.

Consider four images found around a foreground galaxy that were created by a background supernova. Here celestial alignments lead us to successful prediction, and for the first time, a supernova appears where astronomers have said it would. Or I should say, ‘re-appears.’

The elliptical galaxy in question is located within the galaxy cluster MACS J1149+2223, which since 2012 has been known to lie between us and a background galaxy whose light is being magnified by the lens of the cluster. In November of 2014, astronomers found four separate images of a supernova from this background galaxy, appearing in the form of a so-called Einstein Cross. Have a look at the image below, where the cross-shaped pattern is clear.

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Image: The galaxy cluster MACS J1149+2223. Four images of the same supernova are apparent in the inset image. Credit: NASA, ESA, S. Rodney (John Hopkins University, USA) and the FrontierSN team; T. Treu (University of California Los Angeles, USA), P. Kelly (University of California Berkeley, USA) and the GLASS team; J. Lotz (STScI) and the Frontier Fields team; M. Postman (STScI) and the CLASH team; and Z. Levay (STScI).

Now we have word that on December 11 of this year, a team of astronomers successfully predicted a fifth appearance of the supernova. Of course, the supernova event can occur but once, but we are seeing multiple images whose light has in each case taken a different path to reach us, affected by visible and dark matter in the intervening cluster. This means the images from the background galaxy are somewhat out of synch. A team of astronomers involved in the Grism Lens Amplified Survey from Space (GLASS) and a team from another project called Frontier Fields has been able to model these lensing events with great accuracy.

Tommaso Treu (UCLA) is lead author of one of two papers on this work, which looks at the details of the modeling:

“We used seven different models of the cluster to calculate when and where the supernova was going to appear in the future. It was a huge effort from the community to gather the necessary input data using Hubble, VLT-MUSE, and Keck and to construct the lens models. And remarkably all seven models predicted approximately the same time frame for when the new image of the exploding star would appear.”

The supernova is nicknamed Refsdal, a reference to the Norwegian astronomer Sjur Refsdal, who discussed using time-delayed images from a lensed supernova back in the 1960s. Refsdal believed that such images could be a useful tool for studying the universe’s expansion.

Supernova Refsdal turned up exactly when the astronomers had predicted. Hubble has been at work on MACS J1149 since the end of October, making a series of periodic observations by way of testing the models. The model predicting the supernova’s reappearance was also based on data drawn from the Multi Unit Spectroscopic Explorer (MUSE), attached to ESO’s Very Large Telescope (VLT) at Paranal. This November 25 ESO announcement highlights the prediction, which described the supernova’s brightness as well as its timing and location.

The paper on the supernova’s reappearance points out that despite Refsdal’s early paper, a gravitationally lensed supernova with multiple resolved images was not found in the subsequent five decades (although several individual images have been found with magnification caused by lensing). But astronomers have been able to work on time delays within lensed systems by studying multiply imaged quasars, an effort that has been going on since the 1970s. The ‘reappearance’ paper draws two conclusions about the result of the supernova study:

First, SN Refsdal indeed reappeared approximately as predicted, implying that the unknown systematic uncertainties are not substantially larger than the random uncertainties, at least for some models. This is a remarkable and powerful validation of the model predictions specifically and of general relativity indirectly.

And now that we have a successful prediction, we can start to apply its lessons to the modeling process going forward:

The second conclusion is that already this first detection provides some discriminatory power: not all models fare equally well. Grillo-g, Oguri-g, Oguri-a, and Sharon-a [referring to earlier studies] appear to be the ones that match the observations most closely. In general most models seem to predict a slightly higher magnification ratio than observed, or shorter delays. A detailed statistical analysis of the agreement between the model predictions and the observations will have to wait for the actual measurement of the magnification and time delays, which will require analysis of the full light curve past its peak during 2016.

ann15088a

Image: This NASA/ESA Hubble Space Telescope image shows the positions of the past, present and predicted future appearances of the Refsdal supernova behind the galaxy cluster MACS J1149+2223. The uppermost circle shows the position of the supernova as it could have been seen in 1995 (but was not actually observed). The lowermost circle shows the galaxy which lensed the Refsdal Supernova to produce four images — a discovery made in late 2014. The middle circle shows the predicted position of the reappearing supernova in late 2015 or early 2016. Credit: NASA, ESA, S. Rodney (John Hopkins University, USA) and the FrontierSN team; T. Treu (University of California Los Angeles, USA), P. Kelly (University of California Berkeley, USA) and the GLASS team; J. Lotz (STScI) and the Frontier Fields team; M. Postman (STScI) and the CLASH team; and Z. Levay (STScI).

Never before has the appearance of a supernova at a particular time and location in the sky been successfully predicted. We’re now in position to test models involving magnification and time delays for other lensed supernovae. The time delays we see in multiple images of the same event become tools for probing not just the properties of the lensing galaxy and background object, but the properties of cosmic expansion. The fifth image of supernova Refsdal is influenced not only by an individual galaxy but by the gravitational potential of the entire MACS J1149.5+2223 cluster, a reminder of the complexity of the underlying analysis.

The ‘prediction’ paper is Treu et al., “‘Refsdal’ Meets Popper: Comparing Predictions of the Re-appearance of the Multiply Imaged Supernova Behind MACS J1149.5+2223,” in press at The Astrophysical Journal (preprint). The ‘reappearance’ paper is Kelly et al., “Deja Vu All Over Again: The Reappearance of Supernova Refsdal,” submitted to The Astrophysical Journal (preprint).

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Charter

In Centauri Dreams, Paul Gilster looks at peer-reviewed research on deep space exploration, with an eye toward interstellar possibilities. For many years this site coordinated its efforts with the Tau Zero Foundation. It now serves as an independent forum for deep space news and ideas. In the logo above, the leftmost star is Alpha Centauri, a triple system closer than any other star, and a primary target for early interstellar probes. To its right is Beta Centauri (not a part of the Alpha Centauri system), with Beta, Gamma, Delta and Epsilon Crucis, stars in the Southern Cross, visible at the far right (image courtesy of Marco Lorenzi).

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