Imagine a form of life so unusual that we cannot figure out how it dies. That's exactly what researchers are finding beneath the floor of the sea off Peru. The microbes being studied there -- single-celled organisms called Archaea -- live in time frames that can perhaps best be described as geological. Consider: A bacterium like Escherichia Coli divides and reproduces every twenty minutes or so. But the microbes in the so-called Peruvian Margin take hundreds or thousands of years to divide. "In essence, these microbes are almost, practically dead by our normal standards," says Christopher H. House (Penn State). "They metabolize a little, but not much." House goes on to discuss what a slow metabolism may imply about environments outside our own planet. Imagine hydrothermal vents on Europa, where the energy ration may be slim. For that matter, with Phoenix still working its magic at the Martian pole, imagine subsurface aquifers on that planet whose energy resources may be just enough...
Simulating the First Stars
Without the explosions of supernovae, the heavy elements so essential to life itself would be unavailable, and stars would lack the raw materials to form planets. Thus Carl Sagan's famous "We are star-stuff" quotation, an idea validated by our extrasolar studies, which allow us to correlate the presence of planets with the existence of heavy elements in their stars. Much remains to be done here, but stars with higher metallicity and more heavy elements do appear more likely to have planets. Volker Bromm (now at the University of Texas) puts it this way: "We're now just beginning to investigate the metallicity threshold for planet formation, so it's hard to say when exactly the window for life opened. But clearly, we're fortunate that the metallicity of the matter that birthed our solar system was high enough for the Earth to form. We owe our existence in a very direct way to all the stars whose life and death preceded the formation of our Sun. And this process began right after the...
New Precursors of Life Identified in Meteorite
We know that organic compounds have been found in meteorite fragments. But are they truly extraterrestrial, or the result of contamination here on Earth? The subject, always controversial, has been given new impetus by a paper that points to the former, with interesting ramifications. Did life begin on Earth or was the Earth seeded by life from the cosmos? Or perhaps a third alternative exists, with pre-existing life influenced by infall from outer space. If we can build a viable case for the latter two possibilities, we can build one just as viable for planets around a wide variety of stars, giving the idea that granted enough time, life of some kind may become ubiquitous a most interesting boost. The scientists involved have been working with fragments of the Murchison meteorite, which fell in 1969 about 100 km north of Melbourne, Australia. Quite a bit of material -- over 100 kg -- could be recovered, enough for batteries of subsequent tests and the discovery of various amino...
Low Frequency Musings on Extraterrestrial Life
When it comes to SETI investigations, the Low Frequency Array (LOFAR) being built in Europe offers intriguing possibilities. With a plan to encompass roughly 25,000 small antennae, arranged in clusters spread out over an area 350 kilometers in diameter, LOFAR may prove sensitive enough to detect the radiation leakage of transmitters in the radio and television bands from extraterrestrial civilizations. The array will operate between 10 and 240 MHz. When completed, it will offer not only myriad astronomical possibilities but SETI opportunities with a difference. Michael Garrett (Leiden University) is general director of ASTRON, the Netherlands Institute for Radio Astronomy, now involved in building the new array. Garrett makes note of what's possible if LOFAR's formidable resources are turned to SETI: "LOFAR can extend the search for extra-terrestrial intelligence to an entirely unexplored part of the low-frequency radio spectrum, an area that is heavily used for civil and military...
Hunting ETI on the Ecliptic
Imagine a team of astronomers from a distant extraterrestrial civilization. Anxious to find blue and green living planets like their own, they study various methods of planetary detection and put them to work on small, relatively nearby stars. Detecting planetary transits, they refine their techniques until they trace the signature of a planet much like home. Now assume that, despite the presence of their own version of skeptics like myself (some of us think that sending deliberate signals to the stars is premature without further, wider discussion), they decide to encode information about themselves into a message to be sent by a repeating beacon. Naturally, they turn to those stars around which they've found planets that look to be not only the right size, but in the right position, within the habitable zone where water could exist on the surface. Fanciful? You bet, especially in the idea that a nearby extraterrestrial civilization would be more or less at the same state of...
Astrobiology: Finding a Place Like Ours
It's not my usual practice to begin a post with a quotation, but Lee Billings, writing in a recent essay for SEED Magazine, so precisely captures an essential truth about our future in space that I want to give it pride of place. Looking at the ways we search for life on planets around other stars, Billings says this: Throughout history, our knowledge has grown through human ambition and curiosity, only to regress beneath human apathy and caprice. The greatest obstacle to efforts to find another Earth, to discover life elsewhere in the universe, isn't some flaw in our methodology or our technology, but in our will. Most of us alive today are unlikely to see these efforts bear their fullest fruit. Even optimistic young astronomers are uncertain that they will see the light from other living worlds in their careers, or even their lifetimes. But they work as though they will. Whether they see it personally doesn't matter; what matters is that these other planets be seen someday. In...
A Galactic Neutrino Network?
SETI quite naturally started with the assumption that we should look in the realm of photons for signals from other stars. After all, radio or optical wavelengths were things we understood, and the interest in radio and attendant theorizing about 'waterhole' frequencies and interstellar beacons continues to be worth examining. But a truly advanced civilization might be using methods we haven't yet managed to exploit. Of these, a singularly interesting choice is communication by neutrino. John Learned (University of Hawaii) and colleagues take on this issue in a new paper just posted to the arXiv site, looking at the advantages of the notoriously elusive neutrino. A major plus is that the signal to noise problem is tricky for radio and optical methods, especially in the galactic plane, whereas neutrinos, depending on their energy levels, can offer an essentially noise-free band. We also run into severe problems with photons as we look at line of sight communications anywhere near the...
Rethinking Galactic Empire
How much would an extraterrestrial civilization resemble our own? The question resonates because on the one hand, the signature of our activities is what we tend to translate into the SETI search. We look, for example, for the signs of civilizations that are like us but more advanced technologically, which means we apply human thinking and motivations to cultures that are by definition not human. This is natural enough, because we're the only technological civilization we know about, but it leads to results that may mislead us and obscure the actual situation. Fermi's Great Silence bothers us because we assume that what Milan ?irkovi? calls advanced technological civilizations (ATCs) will necessarily move out into the galaxy to colonize it. Yet we see no signs of this, no presence of an expansive power, no characteristic emissions telling us of any intelligence operating around nearby stars. This observation becomes a paradox only if we think in specifically human terms, relating...
The Odds on Interstellar Panspermia
Our recent look at panspermia concepts was largely devoted to the transmission of life via microbes or spores here in our own Solar System. The even richer question of how life might pass from star to star is far more problematic, but as a follow-up to that earlier story, I want to look at work that graduate student Jess Johnson did with Jonathan Langton and advisor Greg Laughlin at the University of California, Santa Cruz. Their work suggests that while life might readily survive an interstellar journey, it is unlikely to wander close enough to seed another system. Ponder the era here on Earth known as the Late Heavy Bombardment (LHB). After the period of planetary accretion ended some 4.4 billion years ago, life apparently began. But 3.8 to 4 billion years ago, the LHB saw the planet again pummeled, causing debris to be ejected into space. Looking specifically at the mass that is ejected at 16.7 kilometers per second in the direction of the Earth's motion (this is Solar System...
Scattering Life Through the Cosmos
Olaf Stapledon's Last and First Men (1930), amongst other wonders, pictures our descendants millions of years hence moving from world to world as they attempt to save the species. The Moon approaches the Earth, an imminent peril the 'Fifth Men' escape by terraforming Venus, unfortunately destroying indigenous life forms there. Later, the Fifth Men move on to Neptune, and when their existence there is endangered, they make an attempt to save themselves as a species by seeding their cells among the stars. Interestingly enough, Francis Crick (famed as a co-discoverer of the structure of DNA) suggested in 1973 that life could have been intentionally sent from elsewhere in the universe with the express purpose of finding a new home, an idea that made the later work of Fred Hoyle and Chandra Wickramasinghe seem positively tame. We're talking panspermia, the idea that life can survive long journeys through space to seed other planets (a notion Hoyle addressed in 1982's Evolution from...
The ‘Great Filter’ Tackles Fermi
Suppose for a moment that life really is rare in the universe. That when we are able to investigate the nearby stars in detail, we not only discover no civilizations but few living things of any kind. If all the elements for producing life are there, is there some kind of filter that prevents it from proceeding into advanced and intelligent stages that use artifacts, write poetry and build von Neumann probes to explore the stars? Nick Bostrom discusses the question in an article in Technology Review, with implications for our understanding of the past and future of civilization. Choke Points in the Past Maybe intelligent beings bring about their own downfall, a premise that takes in more than the collapse of a single society. Alaric's Goths took Rome in 410, hastening the decline of a once great empire, but the devastated period that followed saw Europe gradually re-build into the Renaissance. And as Bostrom notes, while a thousand years may seem like a long time to an individual,...
Degrees of Visibility
Alexander Zaitsev's latest contribution to the debate over sending messages to the stars is a short paper that looks at how visible our planet might be thanks to transmissions from planetary radars like Arecibo, Goldstone or the Evpatoria site from which directed transmissions have already been sent. METI (Messaging to Extra-Terrestrial Intelligence) is broadly dedicated to transmitting messages to stars likely to have habitable planets, but so far the number of transmissions is relatively sparse. The debate over METI discusses the wisdom of continuing them without broader discussion. But tucked within that debate is the specific question of our civilization's visibility. For in addition to the messages that have already been sent, beginning with the Arecibo message in 1974 and continuing in the far more targeted transmissions from Evpatoria between 1999 and 2003, we are using our planetary radars to perform crucial astronomical studies. The work these dishes do in refining our...
Calls Into the Cosmos
Larry Klaes tackles the METI question -- do we intentionally broadcast to the stars? -- in Athena Andreadis' Astrogator's Logs today, looking at the pros and cons of an issue that continues to bedevil the scientific community. Of METI advocate Alexander Zaitsev (Russian Academy of Science), for example, Klaes writes this: In a paper Zaitsev published in 2006, the scientist notes that "SETI is meaningless if no one feels the need to transmit." Zaitsev also feels that if there are advanced cultures bent on harming humanity, they will find us eventually, so it is in our best interests to seek them out first. Zaitsev sees the great distances between stars and the physical limits imposed by attempting to attain light speed serve as a natural protective barrier for our species and any other potentially vulnerable beings in the galaxy. David Brin among others takes the other side of the debate in an article tuned for newcomers to these issues. And that's an important audience. Most...
Life as Rarity in the Cosmos
Although I suspect that intelligent life is rare in the cosmos, I'm playing little more than a hunch. So it's interesting to see that Andrew Watson (University of East Anglia) has analyzed the chances for intelligence elsewhere in the universe by looking at the challenges life faced as it evolved. Watson believes that it took specific major steps for an intelligent civilization to develop on Earth, one of which, interestingly enough, is language. Identifying which steps are critical is tricky, but in the aggregate they reduce the chance of intelligence elsewhere. A linguist at heart, I wasn't surprised with the notion that the introduction of language marks a crucial transition as intelligence develops. But what are the other steps, and how do they feed into the possibility of life elsewhere? These interesting questions relate to how long the biosphere will be tenable for life as we know it. If, as was thought until relatively recently, Earth might support life for another five...
Dyson Spheres: Hoping to Be Surprised
"Were the chemicals here on Earth at the time when life began unique to us? We used to think so. But the most recent evidence is different. Within the last few years there have been found in the interstellar spaces the spectral traces of molecules which we never thought could be formed out in those frigid regions: hydrogen cyanide, cyano acetylene, formaldehyde. These are molecules which we had not supposed to exist elsewhere than on Earth. It may turn out that life had more varied beginnings and has more varied forms. And it does not at all follow that the evolutionary path which life (if we discover it) took elsewhere must resemble ours. It does not even follow that we shall recognise it as life -- or that it will recognise us." -- Jacob Bronowski, from The Ascent of Man How accurate do you think we are in projecting what extraterrestrial civilizations might do? The question is prompted by recent speculation on Dyson spheres and the supposition that advanced cultures will...
Life’s Precursors: The Interstellar Connection
Was the early Earth seeded with amino acids from deep space? The variety of molecules found between the stars makes the supposition provocative, but finding interstellar amino acids has been a challenge. Various amino acids have indeed been found in meteorites, but it has been argued that these could have been produced right here in the Solar System within asteroids. Yet laboratory experiments have shown that amino acids can form among the molecules found in interstellar clouds, including such important ones as glycine, alanine and serine. What's next is to identify amino acids in the interstellar medium, and we're coming close. Ponder this: Since 1965, more than 140 molecules have been identified in space, both in interstellar clouds and circumstellar disks, many of them organic or carbon-based. Now researchers from the Max Planck Institute for Radio Astronomy in Bonn have detected amino acetonitrile (NH2CH2CN), a potential precursor of the simplest amino acid, glycine. The odds are...
If the Phone Doesn’t Ring, It’s Me
The line in the title above is from a Jimmy Buffett song. A friend who knows all Buffett songs line by line uses it on his answering machine, invariably provoking a chuckle when I ponder the implications. If the phone doesn't ring, just what kind of message is being sent? Or is any message being sent at all? Thus does the singer capture the bewildered funk of romantic attachments, which can make hash out of all our logic. Like the dog that doesn't bark (think Sherlock Holmes), the phone that doesn't ring carries its own meaning, one we must now try to parse. For the SETI phone isn't ringing. If extraterrestrial civilizations are out there, is their silence a way of sending us a message? Alan Tough created a Web site with the express purpose of offering a communications venue to any nearby alien probes, spacecraft designed to study us and report home. The Invitation to ETI contains a number of essays explaining the project and more or less asking for participation by ET (Paul Davies'...
Re-seeding Life from Space
I've always found the idea of panspermia oddly comforting. Growing out of the work of Swedish chemist and Nobel Prize winner Svante Arrhenius, panspermia assumes that life can move between worlds by natural means, and implies that planets with the right conditions will wind up with living things on them. That idea of all but universal life, and the weird notion that we might all be in some way 'related,' was exhilarating to thinkers like Fred Hoyle and Chandra Wickramasinghe, who went on to suggest that the influx of life from space triggers continuing changes on Earth today, which might involve epidemics and new diseases. Now comes a variant called lithopanspermia, which questions whether rocks blasted off a planetary surface by impacts might not be the transfer vehicles for microorganisms that travel between planets and perhaps further. After all, we have found Martian meteorites in Antarctica, forty or so to date, so the real question becomes the survival possibilities. Can a...
The Reconfiguration of the Stars
Even the most adamant enthusiasts for METI -- Messaging to Extraterrestrial Civilizations -- haven't come up with anything as audacious as what virtual reality guru Jaron Lanier is now talking about. Writing for Discover Magazine, Lanier has the notion of rearranging basic material objects to make them not just noticeable by aliens but blindingly obvious. Nothing new there, as the concept of such messaging goes back to the 19th Century. Mathematician Karl Gauss considered geometric plantings of trees and wheat to create shapes that might be visible from space, while Joseph von Littrow (perhaps basing the idea on Gauss' work) talked about digging huge ditches and setting kerosene within them on fire at night, for the edification of beings on other worlds. But Lanier isn't talking about anything quite so mundane. This is a guy who thinks big -- he wants to arrange stars. If you can find a way to create stable patterns of stars that are obviously artificial, then you have a celestial...
Life Under Infrared Skies
So far we know of only one place in the cosmos that has life, our own Earth. That makes the study of interesting organisms, and in particular the so-called 'extremophiles' that stretch our understanding of livable habitats, a key part of astrobiology. Finding an organism living around a deep-water vent on the ocean floor doesn't prove life exists in such environments on other worlds, but by understanding the limits of the possible, we're learning more about where and how to look. And sometimes we find unusual life forms in seemingly benign places like Australia's Great Barrier Reef, which brings us to Acaryochloris marina. That tongue twister identifies a bacterium that is unusual because it uses a rare type of chlorophyll -- chlorophyll d -- to take advantage of near infrared long wavelength light. Acaryochloris marina is actually a cyanobacterium, meaning a bacterium that use photosynthesis to derive its energy. Its huge genome (8.3 million base pairs) has now been sequenced for...