by Paul Gilster | Sep 23, 2013 | Culture and Society |
There is much to say about the 100 Year Starship Symposium in Houston, and as I have done with prior conferences, I will be drawing on my notes in the coming weeks. But I want to start the Houston coverage with the good news that emerged from the outer Solar System. Some time back, Jon Lomberg came up with the idea of sending a new kind of message into deep space. No, this wasn’t to be a controversial signal beamed at a nearby star, but a message from humanity that would fly aboard one of our spacecraft. New Horizons is already in the outer system on its way to a Pluto/Charon encounter in 2015 and, we hope, a close pass of a Kuiper Belt object after that. But Jon thought we could still use it, Voyager style, to house the sights and sounds of Earth.
The plan: To re-purpose a chunk of New Horizons’ computer memory, about 120 MB worth, after it has achieved its mission and is continuing out into interstellar space. The 120 MB figure is at this point a rough guess; it represents about 1 percent of the onboard memory. The message from humanity could be assembled by crowd-sourcing the project, getting input from all over the world, and uploading to the spacecraft — Lomberg’s idea is to begin a global contest allowing people to submit their ideas exactly one year before New Horizons flies by Pluto in July of 2015.
Image: Jon Lomberg, who is once again thinking about how to send the sights and sounds of Earth into the cosmos.
I was happy to join the advisory team for the project, for if there’s anyone who can make this happen, it’s Jon. He’s well known as an artist who worked with Carl Sagan on COSMOS and with Frank Drake in designing the cover for the Voyager Interstellar Record. Sending human artifacts on interstellar trajectories is not exactly a common thing to do, but Jon Lomberg is one of the few who has experience at it.
While conversations about the project went into into full gear on the Net earlier this summer, my son Miles went to work on the website that would eventually take the New Horizons Message public. I had assumed when I left for Houston and the 100 Year Starship that I would be focused solely on the various meetings and presentations there, but on Friday night Miles, who had been tuning up the site off and on during the conference, told me that it was ready to go. A quick confirmation with Jon gave the go-ahead to make the project public. Serendipity rules, for who better to make the announcement than the guiding force of SETI, Jill Tarter, who was herself on Jon’s advisory panel, and who even as we were discussing this happened to walk right by?
Image: A lively Friday night in Houston. From left, former Planetary Society executive director Louis Friedman, my son Miles, Jill Tarter and TZF founder Marc Millis.
Thus Friday night, which had already been enlivened by a panel with writers Jack McDevitt, Ken Scholes, Karin Lowachee and Mary Doria Russell, became an impromptu planning moment in the crowded foyer outside the ballroom. Jill quickly agreed, Miles forwarded the relevant URL to her computer, and the next morning, after guiding an excellent panel on recent discoveries (about which more later this week), Jill announced the New Horizons Message Initiative and put the site up on the screen. We then asked the formidable LeVar Burton, also intercepted in the foyer, to blast out a tweet to his 1.7 million followers on Twitter, and the initiative was launched.
Image: A quick chat with LeVar Burton. Talk about a fun guy to be around, LeVar is a strong advocate for pushing to the stars, and he signed off on the New Horizons Message without hesitation.
There is much to do. First of all, we need people to go to the site to sign the petition to demonstrate public support that will persuade NASA. The New Horizons Message is a private initiative, and thousands of signatures on the online petition along with endorsements from leaders in astronomy and space sciences will be crucial in making the case to NASA. Also ahead is a fundraising campaign to provide the necessary budget supporting the project, which will pay for developing the techniques for storing and sending the message, holding meetings and conferences to plan and manage the submission process, and formulating and executing the ensuing contest.
The key here is to make this a message from the entire world, searching globally for pictures and other materials that can be voted upon in various categories of content. A self portrait of Earth in the early 21st Century will thus emerge. Unlike the Voyager Golden Record or the Pioneer plaques, however, this is a record that, once uploaded, can be updated over time, as long as the spacecraft is still in communication with the Earth.
No one realistically sees the New Horizons Message as a way to reach ET. This initiative is really about the Earth, and you might think back to the days of Apollo 8 and the stunning Earthrise photograph that so changed our perspective on our own planet. Astronaut Eugene Cernan is famous for saying “We went to explore the Moon, and in fact discovered the Earth.” That sentence was printed on a large poster in the ballroom at the 100 Year Starship Symposium, and along with it a parallel one: “What will we discover from another star?”
It’s a question with profound implications. I’ve said before in these pages that while the problem of the starship is a problem of science, it is also a problem of philosophy, for we have key choices to make as a species on how we want to live. Turning our aspirations toward space offers us the opportunity to reflect on our place in the cosmos and to see what we are doing in a new light. I strongly support the New Horizons Message Initiative and hope you will as well.
by Paul Gilster | Sep 18, 2013 | Uncategorized |
by Stephen Ashworth
Being a jazz buff (the 1950s and early 1960s are my era of choice) I naturally note that frequent Centauri Dreams commenter and contributor Stephen Ashworth is a tenor sax man who regularly plays in venues near and around Oxford in the UK. Stephen is also, of course, an insightful writer on matters touching our future in space, not only through his work in the Journal of the British Interplanetary Society but also in his Astronautical Evolution site, which bills itself as studying “The social and political basis for the optimistic, progressive, astronautical society of the present and future.” In this essay, Stephen looks at ways of viewing extraterrestrial intelligence that pose different models for the emergence and spread of life in the universe. NOTE: If you’d like to comment, be aware that today is a travel day for me, so comment moderation will be sporadic, but I’ll catch things up tonight.
Speculations about the existence of extraterrestrial civilisations analogous to our own fall naturally into two broad camps, which we may for convenience describe as the Steady State model versus the Big Bang model (not to be confused with the cosmological theories of the same names). There is also a Hybrid model which combines the two in true Hegelian fashion (thesis ? antithesis ? synthesis).
The Steady State model
This is the basis of the famous Drake equation. Drake assumed that for a long time in the past, and for a long time to come, civilisations have been and will continue to be coming into existence, persisting for a while and then vanishing again. The question which interested him was whether the rate of appearance of civilisations capable of interstellar radio communication, and their average longevity, were large enough to make it statistically likely that we would be able to establish contact with a nearby alien society before either they or we became extinct.
Drake regarded civilisations as entirely sedentary or static phenomena. Thus the locations at which they might be found today are always the same as those at which they originally evolved from their biological forebears, and thus closely resemble our planet Earth. They must be found orbiting closely Sun-like stars in circular orbits, thus in the so-called “habitable zone” (planets outside the zone where surface liquid water is possible presumably being habitable only by creatures who were not capable of radio astronomy, or of changing the atmospheric chemistry if there was no atmosphere, and therefore undetectable by astronomical means).
Diagram 1: The Steady State model.
Diagram 1 shows schematically how many civilisations exist at any one time in the Galaxy on the Steady State model. For simplicity it is assumed that each star has either one civilisation, or none. The total number of stars continues to increase slowly as long-lived dwarf stars are added to the population. The number of civilisations rises slightly faster, as longer-lived planets come into play. We are now at point A on the time axis.
The number of stars occupied at any one time is a small fraction of the total (the diagram exaggerates the fraction for clarity). For example, if we share the Galaxy with a million other civilisations at the present time, as optimists may hope, then only 0.00001 of the stars are currently occupied.
All such civilisations arise independently of one another. Collapsed civilisations are not replaced on their planet of origin, but are replaced by other civilisations arising elsewhere. Civilisations are randomly scattered throughout the Galaxy, though Gonzalez, Brownlee and Ward have presented arguments as to why the centre and the outlying galactic regions may be less hospitable than a ring partway out from the centre, where indeed our own Solar System is found.
Civilisations remain completely dependent upon their planet of origin, and the distance between nearest-neighbour planets of that type (perhaps tens of light-years) forbids interstellar settlement.
The Big Bang model
In his book Contact with Alien Civilisations, Michael Michaud reviews the ideas of a number of people who have gone beyond the Drake equation by taking account of the possibility of interstellar colonisation, including Freeman Dyson and Seth Shostak. A similar view has been taken by Ian Crawford, whose article in Scientific American a few years ago discussed the prospect of a dynamic civilisation colonising the entire Galaxy by star-hopping.
Using technologies readily conceivable today (such as nuclear fusion rocket propulsion), a wave of colonies from an expanding civilisation in our Galaxy might take 1,000 years to make each 5 light-year jump (say, travelling for 500 years at 1% of light speed, then taking another 500 years to build up sufficient infrastructure at the target system to make the next jump). Since the Galaxy is about 100,000 light-years across, such a civilisation could spread daughter civilisations to every suitable star and planetary system in the Galaxy within 20 million years.
This, however, is only 0.2% of the age of the Galaxy. The introduction of faster ship speeds makes absolutely no difference: even without warp drive or FTL travel, on a cosmological timescale such a transition from civilisation nowhere to civilisation everywhere is, as Crawford demonstrated, essentially instantaneous.
For a long time, then, the Galaxy is completely devoid of intelligent life. But then one civilisation appears, and spreads throughout the Galaxy in a burst of expansion which we are calling the Big Bang. Thereafter, the locations at which intelligent, technological life is found are almost all colonies, and that life is ubiquitous and permanent.
Diagram 2: the Big Bang model.
Diagram 2 shows schematically how many civilisations exist at any one time in the Galaxy on the Big Bang model. If humanity is alone, then we are at point A. But there is a possibility (though a small one) that another civilisation in our Galaxy is, say, only a million years more advanced than we are, and has not yet colonised our part of the Galaxy, in which case we are at point B.
In contrast with the Steady State model, in which stars are occupied randomly, galactic real estate is occupied by colonies in an expanding bubble of space centered on the first civilisation’s planet of origin. Two or more such expanding bubbles may appear, but only if two or more independent civilisations make the breakthrough to space colonisation within about 20 million years of one another – unlikely to occur within any one galaxy. Once the Big Bang is complete the number of stars occupied at any one time is a large fraction of the total, including virtually all main-sequence stars, thus certainly over 0.9 of the total.
Collapsed civilisations are likely to be recolonised from other colonies. In fact, it is possible for every single civilisation to collapse (just as every individual in a population dies), but so long as each civilisation despatches on average more than one colony during its lifetime, the galactic population of civilisations continues to grow.
The original civilisation quickly leaves its planet of origin and adopts a new, space-colony mode of living which allows its offshoots to prosper at all stable stars with orbiting planetary or asteroidal material. This both reduces the distances of interstellar journeys for such a species, and pre-adapts them to living conditions on multi-generational voyages. But all civilisations which evolve after the Big Bang (unless they appear almost simultaneously with it, around point B on the diagram) grow up in an environment dominated by their local colony of the original civilisation.
Their access to space transport would presumably be analogous to the access which a non-developed tribal people on present-day Earth may or may not have to the developed world’s existing motor, rail, shipping and air networks.
The Hybrid model
It is possible to combine these two contrasting models in a single Hybrid model if some emerging technological civilisations get as far as radio astronomy but do not achieve interplanetary and hence interstellar space colonisation.
Diagram 3: the Hybrid model.
Diagram 3 shows schematically how many civilisations exist at any one time in the Galaxy on the Hybrid model. If our own civilisation collapses before we establish viable extraterrestrial colonies, then we are at point A; if we do succeed in spreading into space, then we are at point B.
In either case, we are unlikely to find interstellar conversation partners. The level of development at which we have radio astronomy but not space colonisation is not in itself a long-term sustainable level, I would argue, but rather an unstable intermediate stage. Having got as far as radio astronomy, a civilisation will either complete the transition to a space-based civilisation within a few centuries, or completely collapse.
This means that the longevity of a society which tried to stabilise itself at that level would be very small, certainly less than 1000 years; the number of such civilisations present at any one time would be correspondingly small; and the distance over which any messages would have to be exchanged correspondingly large, making successful communication correspondingly unlikely.
(If there were as many as 1000 civilisations at any one time, i.e. N = L in Drake’s equation after all the other factors have roughly cancelled each other out, and 1011 stars in the Galaxy, then for an average interstellar spacing of 5 light-years the average spacing between active civilisations would be 2000 light-years, and the waiting time between sending a question and receiving a reply would be greater than the lifetimes of both the transmitting and receiving civilisations.)
The question of longevity
Given modern fears about nuclear war, peak oil, environmental degradation, social degeneration, technological disaster, climate change and terrorism, spiced with a strong dose of post-colonial guilt and self-loathing, for many people it goes against the grain to think of an industrial civilisation like ours as something which might become a permanent feature of the universe.
What is the lesson from the past evolution of life? Firstly, it must be acknowledged that industrial mankind is as different from our pre-industrial forebears as they were from single-celled Precambrian organisms. Unless one is to maintain that science and technology are somehow unnatural, an aberration from the God-given natural order, then the facts must be acknowledged: a new type of life has emerged with capabilities never before seen. They include the abilities to access other heavenly bodies, and to digest the raw materials found there, neither of which was possible before, except in the marginal case of small numbers of bacteria being randomly exchanged between Earth and Mars.
The pattern from evolution is that each level of biology has given rise to a higher level founded on it: thus prokaryotic cells produced eukaryotic cells produced multicellular life produced technological life – in my own terminology: microbiota ? gaiabiota ? technobiota.
As each new level of complexity appears, the previous level also persists in symbiosis with it. Furthermore, whereas even bacterial life could not originally have hoped to outlive the death of the Earth (and of Mars) when the Sun approaches its red giant phase, providing that our civilisation fulfils its potential then those less complex organisms will, along with ourselves, continue to live and prosper long after the death of the Sun.
The pattern therefore suggests not only that our technological civilisation will produce some kind of successor at a higher level of complexity, but also that it will not die out once it has become properly established.
Clearly our society is still going through a period of rapid transition, and cannot possibly be regarded as well established yet. It is still experiencing technological and social revolutions, it has not yet reached its final form, and it is still a monoculture. Only once it has technologically matured and begun to diversify at a variety of different Solar System locations, and even more so at a variety of nearby stars, will it be possible to say that civilisation has finally arrived.
Once it has arrived in full flower, the more dynamic branches of it will certainly spread, because regardless of the precise impulse at work that is what life has always done.
Consider the question: where can one find bacteria on Earth? The answer is: nowhere, for an unknown period of time early in Earth’s history. Then there is a Big Bang, a relatively brief explosion of bacterial life, and thereafter the answer is: everywhere.
Our industrial society has yet to experience the equivalent of that Big Bacterial Bang, or of the Cambrian explosion of 550 million years ago when a plethora of new and diverse multicellular forms emerged and went their own ways. That will require our descendants to expand on an interplanetary and ultimately an interstellar scale. But when they do, or when some other civilisation does if we don’t make it, and if life develops in the future as it has in the past, then civilisation will certainly become a ubiquitous and universal feature of the Galaxy for as far into the future as it is possible for us to glimpse.
Answering Fermi’s question
I discussed this at length on the I4IS blog last December.
In brief: the question is why civilisation did not arrive before now, with a starting point elsewhere than on Earth, given that the stelliferous universe with earthlike planets is about three times older than the Solar System.
The reason why people have such a problem with this, and refer to it as a paradox, is because they are wedded to the traditional view since Darwin that life evolved from chemistry on Earth, whether in a “warm little pond”, a piece of damp clay or a hydrothermal vent. If that was the case, then since it evolved within about 300 million years after the end of the late heavy bombardment, it should have done so on many other planets, and billions of years earlier.
But Robert Zubrin makes the point that there is a huge complexity gap between the simplest bacterium known to science and the most complex molecule that can be synthesised by shaking up raw materials in a test-tube. Some proto-bacterial form of life must have preceded life as we know it. But there is no evidence of proto-bacterial life on Earth.
This to my mind is strong evidence that, contrary to the generally accepted view, life does not evolve from non-life on Earth-like planets. The obvious alternative scenario involves it first emerging in a microgravity environment in something like a comet nucleus, and doing so only extremely rarely. This decouples its initial emergence from its subsequent evolution to multicellular forms, allows a period perhaps 100 times longer for that initial jump in complexity to occur, explains why proto-bacteria have never been found on Earth, and furthermore adds in the requirement for a low-probability space transfer before evolution towards multi-cellular forms can begin, pushing the Big Bang of technobiotic life to the right on the diagram.
But not too far to the right. For all that the accepted age of the universe of 13.7 billion years seems to us to be unimaginably ancient, on its own terms the universe is still young. Judged by the lifetimes of its longest-lived stars, the red dwarfs, the universe will continue to contain stars and planets as we know them for a period on the order of tens of trillions of years to come, though the brighter stars will fade long before then. If the universe was a human being, it would still only be about a month old.
Another factor may play a part. Carl Sagan has described how the modern alien encounter/alien abduction mania perpetuates the phenomenon of encounters with angels and demons and with the Virgin Mary in earlier centuries. Could the flood of speculations about alien civilisations – where are they? are they hostile or friendly? – be the modern equivalent of the search for God? Do people still yearn to submit to an Overlord (the name given to the aliens in Arthur C. Clarke’s Childhood’s End), whether beneficent, or intent on our punishment?
Until we find any evidence of alien intelligence, the most parsimonious explanation is that there isn’t any where we have looked, that there is no invisible dragon in my garage (Sagan’s image). So we must look further, before it will be possible to use observations to rule out either of the models described here.
References
Ian Crawford, “Where Are They?”, Scientific American, July 2000, p.28-33.
Guillermo Gonzalez, Donald Brownlee and Peter D. Ward, “Refuges for Life in a Hostile Universe”, Scientific American, October 2001, p.52-59.
Michael A.G. Michaud, Contact with Alien Civilisations (Copernicus, 2007).
Carl Sagan, The Demon-Haunted World: Science as a Candle in the Dark (Headline, 1997); Contact (Century Hutchinson, 1986).
Robert Zubrin, “Interstellar Panspermia Reconsidered”, JBIS, vol.54, no.7/8 (July/August 2001), p.262-269.
by Paul Gilster | Sep 17, 2013 | Astrobiology and SETI |
It was back in 2010 that Nir Goldman (Lawrence Livermore National Laboratory) first predicted that the impact of a comet on the early Earth could produce potential life-building compounds like amino acids. Goldman was using computer simulations to make the call, studying molecular dynamics under the conditions of such impacts. He found that the shock of impact itself should produce amino acids and other prebiotic compounds, regardless of conditions on the planet. It was intriguing work because it suggested that impacts in the outer system (think Enceladus, for example) could produce enough energy to create the shock synthesis of prebiotics there.
Now Goldman, working with collaborators from Imperial College London and the University of Kent, has gone beyond the simulations to test the process in the laboratory. By firing a projectile into a mixture comparable to the material found on a comet — water, ammonia, methanol and carbon dioxide — the team was able to produce several different kinds of amino acids including D- and L-alanine and the non-protein amino acids α-aminoisobutyric acid and isovaline as well as their precursors. The high-speed gun, located at the University of Kent, propels steel projectiles at 7.15 kilometers per second into the target mixture. Says Goldman:
“These results confirm our earlier predictions of impact synthesis of prebiotic material, where the impact itself can yield life-building compounds. Our work provides a realistic additional synthetic production pathway for the components of proteins in our Solar System, expanding the inventory of locations where life could potentially originate.”
Planetary impacts from comets were surely widespread in the early Solar System, and we now know that they could produce prebiotic molecules and thus play a role in the development of life. What Goldman’s team has demonstrated is that the shock of impact itself is enough to produce the energy needed for the synthesis of complex organic compounds from the comet’s ices. It is possible that this process began life’s course on Earth during the Late Heavy Bombardment, the era between 4.1 and 3.8 billion years ago when collisions were rife in the inner system.
Image: Comets contain compounds such as water, ammonia, methanol and carbon dioxide that could have supplied the raw materials that, upon impact with the early Earth, would have yielded an abundant supply of energy to produce amino acids and jump-start life. Credit: Lawrence Livermore National Laboratory.
The same building blocks can be produced by the impact of a rocky meteorite into an object with an icy surface, making the icy moons of outer gas giants an interesting environment for astrobiology. Mark Price (Imperial College London) notes how much still needs to be understood:
“This process demonstrates a very simple mechanism whereby we can go from a mix of simple molecules, such as water and carbon-dioxide ice, to a more complicated molecule, such as an amino acid. This is the first step towards life. The next step is to work out how to go from an amino acid to even more complex molecules such as proteins.”
For more, see this Imperial College news release and this release from Lawrence Livermore National Laboratory. The paper is Martins et al., “Shock synthesis of amino acids from impacting cometary and icy planet surface analogues,” published online in Nature Geoscience 15 September 2013 (abstract).
by Paul Gilster | Sep 16, 2013 | Missions |
Tracking Voyager 1 outbound for the past decade has been at times anti-climactic. Had the spacecraft reached interstellar space or hadn’t it, and how exactly would we know? The announcement last week that the milestone has been reached will forever mark August 25, 2012 as the date when a human-built object, still returning data, made the crossing. That it took a year of analysis only reminds us how much we have to learn about even this closest region of the space between the stars, where some interactions with the Sun continue.
“We have been cautious because we’re dealing with one of the most important milestones in the history of exploration,” said Voyager project scientist Ed Stone of the California Institute of Technology in Pasadena. “Only now do we have the data — and the analysis — we needed.”
Image: I use this image — or one much like it — all the time in my talks because it puts huge Solar System distances in perspective. The scale bar is measured in astronomical units (AU), with each set distance beyond 1 AU representing 10 times the previous distance. Each AU is equal to the distance from the Sun to the Earth. It took from 1977 to 2013 for Voyager 1 to reach the edge of interstellar space. Credit: NASA/JPL-Caltech
The caution has certainly been justified. Voyager 1’s plasma spectrometer — able to measure the ionized gas, or plasma, that essentially inflates the heliosphere — stopped working all the way back in 1980. The direction of magnetic field lines emanating from the Sun became became the alternative marker, since solar plasma and interstellar plasma were expected to differ in direction. Another marker: The level of charged particles inside the heliosphere should drop and the level of galactic cosmic rays should rise when the heliosphere was truly crossed.
Last summer brought changes beginning in May and accelerating in July with a jump in the number of outside particles and a drop in the charged particles from the Sun. Confusingly, the magnetic field direction had not changed — was the spacecraft still inside the heliosphere? A solar storm early in 2012 may have furnished the answer. Leading the plasma wave science team, Don Gurnett and Bill Kurth (University of Iowa) realized that radio activity observed earlier in the mission had been the result of interstellar plasma encountering bursts of solar material.
The oscillations caused by such events should be observable when Voyager 1 is surrounded by interstellar plasma, and plasma oscillations in the spring of this year had the signature of that plasma, evidently the outflow from the March, 2012 solar flare activity. The scientists made the call based on the observed electron density of the plasma, which is higher in the interstellar medium. Working back through the data, the duo could pin the onset of these interactions to August of 2012, consistent with the earlier changes in charged particles and doubtless related to the burst of solar activity that set the plasma in motion. While amidst interstellar plasma, the spacecraft was still feeling some influence from the Sun. Let me quote Stone again on this:
“Now that we had actual measurements of the plasma environment – by way of an unexpected outburst from the sun – we had to reconsider why there was still solar influence on the magnetic field and plasma in interstellar space. The path to interstellar space has been a lot more complicated than we imagined.”
NASA is now saying that by August 25 the spacecraft had entered the interstellar region for good, an indication that the heliopause had been crossed. The Voyager team is in agreement that the spacecraft is in interstellar space, although Stone refers to it as “a mixed, transitional region,” and we still see some solar influence, possibly including the unchanged direction of the magnetic field, which is puzzling. Voyager 1 seems to be illustrating what we have been learning for the past sixty years, that the Solar System and its surroundings are much more varied and diffuse than we previously thought. We once conceived of our system as a place of nine planets and a belt of rocky debris. Now we know about numerous small worlds in the Kuiper Belt, a second band of rock and icy objects, and have re-tooled the very definition of the word ‘planet.’ We’ve also learned we’re surrounded by trillions of comets.
That latter point deserves some attention, for the numerous headlines talking about Voyager 1’s departure from the Solar System reflect a continuing misunderstanding about what the system actually is. The Oort Cloud is widely accepted as the home of long-period comets, occasionally jolted by gravitational interactions into sending a new comet into a Sun-grazing orbit. To leave the Solar System, we have to speak of going to a place where the Sun’s gravity no longer dominates, and that could take us out 100,000 AU or more. Voyager 1’s passage through the Oort Cloud will be measured in tens of thousands of years. In 40,000 years, Voyager 1 will be closer to the star AC +79 3888 than to our own Sun.
One of those headlines mistakenly saying that Voyager 1 had left the Solar System occurred in the Washington Post, but the article nonetheless contained this gem:
Launched in 1977, the Voyager’s computing power was impressive for its time. The spacecraft was designed to run most of its operations itself, since the billions of miles separating it and Earth make communication laggy. To accomplish that, Voyager has three interconnected computer systems: one to control the craft’s flight and altitude, another to control its instruments, and a third to manage the first two. The computers can process about 8,000 instructions per second — a fraction of the capability of your smartphone, which handles upwards of 14 billion each second. With memory measured in kilobytes, they can hold only hold a few thousand words worth of text.
We haven’t left the Solar System, but at 121 AU we’ve punched through the heliopause and are in a region where our spacecraft is surrounded by material from other stars rather than being dominated by plasma from the Sun. The achievement is colossal: We launched the Voyagers in 1977 on a mission designed to study specific planetary targets, with no expectations that they could be pushed to become our first interstellar probes. Their data are stored on 8-track digital tape recorders and broadcast back to Earth with a 23-watt signal. That Voyager 1 has now managed the journey speaks to the quality of its construction and the dedication of the teams that have monitored it over the decades. What more will it tell us before it falls finally silent?
The paper is Gurnett, Kurth et al., “In Situ Observations of Interstellar Plasma With Voyager 1,” published online in Science 12 September 2013 (abstract).
Addendum: This just in from Jim Benford, who has been calculating when Voyager 2 and New Horizons will cross into interstellar space:
New Horizons is going the same direction as Voyager 2, as projected onto the ecliptic, but Voyager 2 is going south of the plane, New Horizons staying approx in the plane. It’s headed toward Sagittarius.
- If the ISM is the same distance as Voyager 1 found it (122 AU), New Horizons will take 30 years to reach it. [New Horizons is going 3.165 AU/yr, is 27.35 AU out].
- Similarly, if the ISM is the same distance as Voyager 1 found it, Voyager 2 will reach the ISM in 4.9 years.
