Not all that long ago we assumed habitable planets needed a star like our Sun to thrive, but that view has continued to evolve. M-class red dwarfs may account for as many as 80 percent of the stars in our galaxy, making habitable worlds potentially more numerous around them than anywhere. And let's extend our notion of habitability to what Luca Fossati (The Open University, UK) and colleagues call a Continuous Habitable Zone (CHZ). Now things really get interesting, for a red dwarf evolves slowly, so planets could have a CHZ with surface water for billions of years. But what about white dwarfs? Stellar evolution seems to rule out habitable worlds around them because we normally think of stars entering their red giant phase and destroying their inner planets enroute to becoming a white dwarf. But can a new planetary system emerge from the wreckage? We've already found planets orbiting close to the exposed core of a red giant (KOI 55.01 and KOI 55.02), showing that the end of main...

By Larry Klaes One result of the biennial Astrobiology Science Conference (AbSciCon) held the last week of April in 2010 was to gather SETI specialists from around the world to look at everything from search strategies and signal processing to the best ways of creating an interstellar message. Tau Zero's Larry Klaes has been reading the collected papers from the meeting's SETI sessions, which have inspired him to ponder SETI's place in the scheme of things and how our reaction to the search tells us something about who we are and who we are becoming. Readers with a long memory may recall that the first major conference on interstellar communications, held in Soviet Armenia in 1971, produced a volume of proceedings titled Communication with Extraterrestrial Intelligence, a title editor Douglas Vakoch deliberately echoes in the current work, partly as a nod to the field's past and partly as a measure of how far it has come. I love anthologies. There is nothing like having a collection...

Michael Chorost is a science writer whose research interests grow directly out of his personal experience. You may have already read about his struggle with hearing loss -- a problem he has dealt with since childhood -- in his book Rebuilt: How Becoming Part Computer Made Me More Human (Houghton Mifflin, 2005). It's natural to find Chorost writing often on things like cochlear implants and neurotechnology, but intriguing to find that he is also a SETI advocate, and one who believes his hearing issues have a bearing on a field he has studied passionately all his life. In fact, the book he plans next, which follows on 2011's World Wide Mind (Free Press) will be a SETI title. So what's the connection between deafness and hunting for signs of an extraterrestrial civilization? Chorost sees it as a matter of isolation and communication, as he notes in a recent entry on the Psychology Today site. Is the entire human race subject to deafness? It is in the sense that we have no idea whether...

I haven't even finished the first line of this post and I'm already in a digressive mood. The mental sidetrack comes from yesterday's talk about the Square Kilometer Array, whose primary installations are now to be built in both South Africa and Australia. By observing an object through many instruments simultaneously, astronomers can use the technique called interferometry to combine incoming data and emulate a much larger instrument. The SKA's sensitivity promises to be high enough to allow the detection of possible leakage radiation from another civilization, which prompted me to recall a quote I had buried in my archives: "I know perfectly well that at this moment the whole universe is listening to us -- and that every word we say echoes to the remotest star." The words are those of Jean Giraudoux, a French writer and diplomat whose plays, written between the two world wars, gained him an international audience (Christopher Fry was among the admirers who adapted Giraudoux's work...

We often speak of habitable zones around stars, most commonly referring to the zone in which a planet could retain liquid water on its surface. But the last ten years has also seen the growth of a much broader idea, the galactic habitable zone (GHZ). A new paper by Falguni Suthar and Christopher McKay (NASA Ames) digs into galactic habitable zones as they apply to elliptical galaxies, which are generally made up of older stars and marked by little star formation. Ellipticals have little gas and dust as compared to spirals like the Milky Way and are often found to have a large population of globular clusters. Are they also likely to have abundant planets? The answer is yes, based on the authors’ comparison of metallicity -- in nearby stars and stars with known planets -- to star clusters in two elliptical galaxies. While many factors have been considered that could affect a galactic habitable zone, Suthar and McKay focus tightly on metallicity, with planet formation dependent upon the...

I've been trying to figure out why exomoons -- moons around planets that orbit stars other than our own -- have such a fascination for me. On the purely scientific level, the sheer amazement of discovery probably carries the day, meaning that I grew up in a time long before we had confirmation of any exoplanets, and now we're talking about getting data on their moons. But there's also that sense of the exotic, for we can wonder whether gas giants in the habitable zone, which may be more plentiful than we realize, might have life on their own rocky moons. David Kipping (Harvard-Smithsonian Center for Astrophysics) has been a key player in the exomoon hunt for some time now (search under his name in the archives here and you'll retrieve articles going back for years). David is now working with a 'crowd-funding' source called Petridish.org to fund a new mini-supercomputer that will go to work on the Hunt for Exomoons with Kepler (HEK) project. The idea behind HEK is to use Kepler data...

Let's imagine for a moment that John Mathews (Pennsylvania State University) is right in theorizing that space-faring civilizations will use self-reproducing probes to expand into the galaxy. We've been kicking the issues around most of this week, but the SETI question continues to hang in the background. For if there really are extraterrestrial civilizations in the nearby galaxy, how would we track down their signals if they used the kind of communications network Mathews envisions, one in which individual probes talked to each other through tight-beam laser communications designed only for reception by the network itself? One problem is that the evidence we're looking for would most likely come in the form of spread-spectrum signals, a fact Jim Benford pointed out in a comment to my original post on Mathews, and one that also pointed to recent work by David Messerschmitt (UC-Berkeley). The latter makes a compelling case for spread-spectrum methods as the basis for interstellar...

It was back in the 1980s when Robert Freitas came up with a self-reproducing probe concept based on the British Interplanetary Society's Project Daedalus, but extending it in completely new directions. Like Daedalus, Freitas' REPRO probe would be fusion-based and would mine the atmosphere of Jupiter to acquire the necessary helium-3. Unlike Daedalus, REPRO would devote half its payload to what Freitas called its SEED package, which would use resources in a target solar system to produce a new REPRO probe every 500 years. Probes like this could spread through the galaxy over the course of a million years without further human intervention. A Vision of Technological Propagation I leave to wiser heads than mine the question of whether self-reproducing technologies like these will ever be feasible, or when. My thought is that I wouldn't want to rule out the possibility for cultures significantly more advanced than ours, but the question is a lively one, as is the issue of whether...

"With exoplanets we are entering new territory," says René Heller (Leibniz Institute for Astrophysics, Potsdam), talking about recent studies looking at axial tilt as a parameter for habitability on a planet. Heller is getting at the fact that while we've studied the axis of a planet's spin relative to the plane of its orbit rather thoroughly here in our own Solar System, we are a long way from being able to discern the axial tilt of exoplanets, much less make definitive statements about its effect on habitability. Right now we can say something about the size, mass and orbital period of many distant planets (and in a few cases, some of the components of their atmosphere) and that's about where our knowledge stops. Heller imagines the Earth with an axial tilt something akin to that of Uranus, whose equator and ring system run almost perpendicular to the plane of its orbit. Introduce such high obliquity to the Earth and the north pole would point at the Sun for a quarter of the...

Let me draw your attention to two interesting stories this morning, one harking back to the night in August of 1977 when the Big Ear radio telescope at Ohio State University recorded the famous 'Wow!' signal. For those unfamiliar with it, the 'Wow!' signal gets its name from Big Ear volunteer Jerry Ehman's annotation (several days later) on the signal's printout. 'Wow!' seemed appropriate for a signal that was 30 times stronger in volume than the background noise and took up a single 10 kilohertz-wide band on the receiver, an enigmatic 70-second narrow-band burst at almost precisely 1420 megahertz, the emission frequency of hydrogen. A message from an extraterrestrial civilization? 'Wow!' seemed to fit the bill, but it disappeared and despite more than 50 repeated searches by the Big Ear team, it never recurred. In this article for The Planetary Society, Amir Alexander calls the signal "...the single most intriguing result ever produced by the Search for Extraterrestrial...

Yesterday’s post looked at SETI and its assumptions, using the lens of a new paper on how the discipline might be enlarged. The paper’s authors, Robert Bradbury, Milan ?irkovi? and George Dvorsky, are not looking to supplant older SETI methods, but rather to broaden their scope by bringing into play what we are learning about astrobiology and artificial intelligence. It is perilous, obviously, to speculate on how an alien civilization might behave, yet to some extent we’re forced to do it in choosing SETI targets, and that being the case, why not add into the mix methods that go beyond our current radio and optical searches, methods that may have a better chance of success? The Engima of Contact A key to extending SETI’s reach is to question the very idea of contact. One assumption many of SETI’s pioneers had in common was that there was an inherent need to communicate with other species, and that this need would take the form of intentional radio beacons or optical messages. What...

Have you ever given any thought to intergalactic SETI? On the face of it, the idea seems absurd -- we have been doing SETI in one form or another since the days of Project Ozma and without result. If we can’t pick up radio signals from nearby stars that tell us of extraterrestrial civilizations, how could we expect to do so at distances like M31’s 2.573 million light years, not to mention even the closest galaxies beyond? Herein lies a tale, for what intergalactic SETI exposes us to is the baldness of our assumptions about the overall SETI attempt, that it is most likely to succeed using radio wavelengths, and that it may open up two-way communications with extraterrestrials. It’s the nature of these assumptions that we need to explore today. The Visibility of a Galactic Culture Let’s suppose, for example, that Nikolai Kardashev’s thoughts about types of civilizations are compelling enough to put to the test. A Kardashev Type III civilization is one that is able to exploit the energy...

Beamed propulsion continues to be a particular fascination of mine, which is why I want to start a discussion tomorrow of Jim Benford's latest paper on beamed sails and how they might be optimized for both performance and cost. Reading through Benford's work, however, I also came across Chris Wilson's recent articles in Slate, which discuss Jim and Gregory Benford's work on interstellar beacons and the SETI ramifications. I want to be sure to point to Wilson's How to Build a Beacon because I don't see 'Benford beacons,' as they're increasingly called, discussed much in the media, and Wilson does a fine job at setting the concept in context. Messages into Deep Time The two part Slate series (the first article is The Great Silence) considers humanity's legacy and relates it to the issues raised by SETI. The Arecibo message sent in the direction of the globular cluster M13 in November of 1974 is Wilson's point of departure. Carl Sagan and Frank Drake set up the famous message in the...

The on-again, off-again SETI search at the Allen Telescope Array is back in business as Jill Tarter and team focus in on some of the more interesting worlds uncovered by the Kepler space telescope and follow-up observations. You'll recall that last April the ATA was in hibernation, having lost its funding from the University of California at Berkeley, which had operated the Hat Creek Observatory in northern California where the ATA is located. It took a public campaign to raise the funds needed for reactivation and new operations, as well as help from the US Air Force in the form of its own assessment of the ATA's applicability in its space situational awareness studies, which include developing a catalog of orbiting space objects. The SETI Institute, along with third-party partners and volunteers, has set up SETIstars.org as a fund-raising operation specifically targeting the ATA -- it's important to realize that getting the array back in operation is a first step in the larger...

Could life exist on a world with a methane rather than a water cycle? The nitrogen-rich atmosphere of Titan, laden with hydrocarbon smog, is a constant reminder of the question. Cassini has shown us the results of ultraviolet radiation from the Sun interacting with atmospheric methane, and we've had radar glimpses of lakes as well as the haunting imagery from the descending Huygens probe. Our notion of a habitable zone depends upon water, but adding methane into the mix would extend the region where life could exist much further out from a star. Chris McKay and Ashley Gilliam (NASA Ames) have been actively speculating on the possibilities around red dwarfs and have published a recent paper on the subject. It's intriguing, of course, that with methane we get the 'triple point' that allows a material to exist in liquid, solid or gaseous form at a particular temperature and pressure. That makes Titan 'Earthlike' in the sense that our initial view showed a landscape with the clear signs...

If you're looking for a new tactic for SETI, the search for extraterrestrial intelligence, Avi Loeb (Harvard-Smithsonian Center for Astrophysics) and Princeton's Edwin Turner may be able to supply it. The duo are studying how we might find other civilizations by spotting the lights of their cities. It's an exotic concept and Loeb understates when he says looking for alien cities would be a long shot, but Centauri Dreams is all in favor of adding to our SETI toolkit, which thus far has been filled with the implements of radio, optical and, to a small extent, infrared methods. Image: If an alien civilization builds brightly-lit cities like those shown in this artist's conception, future generations of telescopes might allow us to detect them. This would offer a new method of searching for extraterrestrial intelligence elsewhere in our Galaxy. Credit: David A. Aguilar (CfA). Spotting city lights would be the ultimate case of detecting a civilization not through an intentional beacon but...

by Dave Moore Dave Moore, a frequent Centauri Dreams contributor, tells me he was born and raised in New Zealand, spent time in Australia, and now makes his home in California. "As a child I was fascinated by the exploration of space and science fiction. Arthur C. Clarke, who embodied both, was one of my childhood heroes. But growing up in New Zealand in the 60s, anything to do with such things was strictly a dream. The only thing it did lead to was to getting a degree in Biology and Chemistry." But deep space was still on Dave's mind and continues to be, as the article below, drawing on his recent paper in the Journal of the British Interplanetary Society, attests. "While I had aspirations at one stage of being a science fiction writer," Dave adds, "I never expected that I would emulate the other side of Arthur C. Clarke and get something published in JBIS." But he did, and now explains the thinking behind the paper. The words from "Science Fiction/Double Feature" in the Rocky...

It makes perfect sense to me that we usually think of extraterrestrial intelligence in terms of technology. After all, when we listen to the stars for the whisper of a distant signal, we're saying that SETI is all about finding something that was produced with tools, like a beacon. Or if we extend the thought to science fiction, we might dream of studying alien civilizations through their ruins on long-dead worlds, learning about them by studying what they once built. After all, this is how we do archaeology, digging up spear-points or the bricks of ziggurats, the things that a culture leaves behind that it built with its tools. But will we always confine the idea of intelligence to the presence of an artifact? Science writer and Astronomy Now editor Keith Cooper examines the question in Dolphins, Aliens, and the Search for Intelligent Life, an incisive new essay for Astrobiology Today, one that offers us a new technology that may prove that intelligence doesn't necessarily need...

Most people think that SETI is worth doing, whether or not they actually believe there are other technological civilizations in the galaxy. Ben Zuckerman, a professor of astronomy at UCLA, is certainly in the skeptics' camp, thinking there are no technological ETs in the Milky Way, but he's quoted in this story from QUEST (KQED San Francisco) as calling for more SETI. "Given that the costs are not very high," says Zuckerman, "why not continue the search?" Zuckerman, who once worked with Carl Sagan in graduate school, no longer thinks we live in a crowded galaxy, but a potential discovery of this magnitude justifies the relatively modest expenditure. It's not surprising to find Jill Tarter echoing Zuckerman. The recent funding problems of the Allen Telescope Array have not daunted the woman who more than anyone else has come to represent the search for other intelligent life. And although she believes we may one day come to the 'extraordinary conclusion' that we really are alone, the...