vIcarus: Interstellar Mission in Cyberspace

One of the most useful technologies the Project Daedalus team lacked when designing its interstellar probe back in the 1970s was the personal computer. Today's effort to re-visit Project Daedalus can draw on the strength of intercontinental networking for fast communications and widespread computer availability to design a probe differently. It's exciting to hear that the Project Icarus team plans vIcarus, a 'virtual' interstellar mission drawing on the completed Icarus design and 'flown' through ongoing computer simulation. Spun out in real time, vIcarus will give designers and the public a chance to follow the mission step by step. Andreas Tziolas (Variance Dynamical Corporation) discussed the idea on the Project Icarus blog recently, noting that over the next few years, the Icarus team will be creating computational models for propulsion, fault repair, communications, flight through the interstellar medium and all the factors impinging upon the behavior and stability of the...

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To Join the ‘Galactic Club’

Is there a 'Galactic Club' of civilizations to which our species might one day deserve admission? If so, the club's members are being mighty quiet about their existence. But David Schwartzman (Howard University) thinks it might be out there. In that case, he finds three possible explanations for the 'Great Silence,' our failure to detect any signs of extraterrestrial intelligence in the last fifty years. He rejects the first, the notion that we are alone in the galaxy -- life is, in his view, all but inevitable in the universe, and he's keen on the idea of high levels of intelligence developing on many worlds, as he tells us in this article in Astrobiology Magazine: I have argued that encephalization - larger brain mass in comparison to body mass -- and the potential for technical civilizations are not very rare results of self-organizing biospheres on Earth-like planets around Sun-like stars. Biotically-mediated climatic cooling creates the opportunity for big-brained multicellular...

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The Milky Way from Outside

We sometimes forget the conditions under which great images get made. A few years back, in one of the earliest posts on his systemic site, Greg Laughlin (UC-Santa Cruz) showed the image you see below, a famous shot made by the Hubble telescope of the 'Sombrero Galaxy,' M104. It's obvious why this image is a classic. As Greg notes, "The glow of its halo makes the idea of 100 billion stars seem comprehensible." But look at the follow-up picture, which Greg made to demonstrate his point. While the Hubble image is a long CCD time-exposure to light gathered by a 240 cm mirror, your own eyes would deliver something considerably different. From 300,000 light years, M104 is noticeable only as a dim and lurking shape. You can see the same effect for yourself if you find the Andromeda Galaxy, subtening an angle larger than the full Moon in our skies but as evanescent as smoke when viewed by the naked eye. The dim, fuzzy object is out there if you know where to look, but it's not exactly...

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WISE: First Survey Ends in July

What a glorious image WISE has given us. The Wide-field Infrared Survey Explorer has finished three-quarters of its infrared map of the entire sky, with the final images scheduled for July, after which time the spacecraft will spend three months on a second survey before its solid-hydrogen coolant (needed to keep its infrared detectors chilled) runs out. The public WISE catalog will be released a little over a year from now, but we can already marvel at spectacles like the Heart and Soul nebulae, seen below. Be sure to click on the image, presented at the American Astronomical Society meeting in Miami, to enlarge it and spend some time among the newly forming stars. Image: Located about 6,000 light-years from Earth, the Heart and Soul nebulae form a vast star-forming complex that makes up part of the Perseus spiral arm of our Milky Way galaxy. The nebula to the right is the Heart, designated IC 1805 and named after its resemblance to a human heart. To the left is the Soul nebula,...

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Disturbing the Habitable Zone

It's AAS week in Miami, and the American Astronomical Society usually gives us plenty to talk about. Inclined orbits, for one thing. In our Solar System, the process of planetary formation seems relatively intuitive. The eight major planets orbit largely in the same plane, reinforcing the idea that the cloud of gas that collapsed to form the Sun contained leftover material that formed into a planet-yielding disk. We can point to outer system objects like Pluto (and certainly Sedna) as exceptions, but they're much further out and subject to gravitational influences that this model can account for. But as Barbara McArthur (University of Texas at Austin) and team told an AAS session yesterday, the star Upsilon Andromedae A has yielded a different result. We already knew that three Jupiter-class planets orbited the star, some 44 light years away and a bit younger and more massive than our Sun. But McArthur's team now has determined the mass of two of the three known planets, and has...

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A New Horizons Wake Up Call

Recently we've been talking about long-distance repair, and how any probe launched beyond the Solar System is going to have to fix its own problems rather than relying solely on transmissions from Earth. New Horizons, halfway to Pluto/Charon in terms of distance, isn't yet in that category. It's going to eventually make its way into the Kuiper Belt, but for now, it's close enough for controllers to wake it up periodically for checks. In fact, the next wakeup call, which comes tomorrow, begins a nine-week period of rigorous tests. Long-term missions like New Horizon demand annual checkouts, and this one (as opposed to last year's) is to be comprehensive, ranging from conducting heliospheric cruise science to uploading a series of code enhancements and bug fixes to the spacecraft's fault protection software. The spacecraft's backup systems will be checked and its seven scientific instruments re-calibrated. Principal investigator Alan Stern describes the process in his latest report. I...

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IKAROS Aloft: Shaking Out Sail Technologies

Congratulations to JAXA, the Japan Aerospace Exploration Agency, for the successful launch of the IKAROS space sail, launched from the Tanegashima Space Center along with the Venus Climate Orbiter yesterday evening US time. The launch was a beautiful sight via JAXA's Internet feed and we now have the opportunity to shake down solar sail technologies in space, from deployment to navigation and maneuvering. The mission sequence ahead is shown in the diagram below, but as we wait for further news, a special nod of appreciation for IKAROS project leader Osamu Mori and the fine team that has made this solar sail a reality. Image: After separation from H-IIA, IKAROS will spin at up to 20 rpm, deploying the sail membrane and generating solar power by means of thin film solar cells (minimum success level) within several weeks. Acceleration and navigation using the solar sail will then be demonstrated (full success level) within half a year. Credit: JAXA. The AKATSUKI climate orbiter is a...

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Burying the Digital Genome

I once had an uncle who, in his eccentric way, taught me the glories of reading widely and across many disciplines. Every year he would visit us from Florida and each time he came, he was off on another tangent, usually a scientific pursuit of some kind, and now and then a venture into linguistics. One of his more memorable visits found him arriving with a set of slides he had made from books on Egyptian hieroglyphics, and we went through them one at a time as he explained what he had learned about Egyptian culture by mastering these symbols. Hieroglyphics Meet the Machine I think about that every time I ponder the fate of digital data, and this Reuters story, which mentions hieroglyphics, triggered the memory. For as Andreas Rauber (University of Technology of Vienna) points out, hieroglyphics -- or, for that matter, stone inscriptions or medieval manuscripts -- have a shelf life of millennia, and have proven it. In my own wandering way, I was for a time focused on medieval...

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A Cassini Double Flyby

Raw images from Cassini's Enceladus encounter yesterday are becoming available, the most fascinating of which show the view of the plumes as the spacecraft approached the moon from the night side. And check the image below, which is an extraordinary combination of Cassini targets the like of which I never thought I would see. At the bottom of the image, darkened almost to invisibility, is Enceladus' south pole as the spacecraft speeds over its surface (click on the image to enlarge). Swinging into view beyond it are Saturn's rings and Titan, its atmosphere clearly visible. Cassini will make a Titan flyby late this evening, in the early hours of May 20 UTC, this time passing to within 1400 kilometers of the surface in a study that will fill out Titan's thermal map. Enceladus and Titan are so aligned that Cassini will be able to make this second flyby with no additional maneuvering required. By studying the gravitational pull on the spacecraft, researchers hope to learn more about...

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Three Views of Icarus

Two versions of Icarus are on my mind today. Well, actually three. The first is the Japanese solar sail/solar cell hybrid called IKAROS, scheduled for launch today but scrubbed because of the weather at Tanegashima. The new launch date is Thursday May 20 at 2158 UTC (1758 EDT). IKAROS will piggyback aboard the JAXA H-2A booster with the Venus Climate Orbiter (AKATSUKI), and will be a ground-breaking shakedown of solar sail technologies in interplanetary space. Needless to say, we'll follow this one with interest as solar sails move to the next level of testing. Meanwhile, Kelvin Long reports that Project Icarus, the joint-undertaking between the British Interplanetary Society and the Tau Zero Foundation, made the pages of the London Metro newspaper recently. Be sure to click 'This Week's Graphic' at the bottom of the article to view the whole story. Icarus, often discussed in these pages, is the successor to the BIS Project Daedalus starship study, and seeks to examine fusion...

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Call for Papers: Searching for Life Signatures

Like astrobiology, SETI is a multi-disciplinary effort, one that pulls together our knowledge and speculation about everything from life's origins to the development of planetary systems and the evolution of civilizations. It's remarkable to remember that it was only fifty years ago that Frank Drake launched the enterprise by scanning a 400 kHz window for interstellar radio transmissions. Epsilon Eridani and Tau Ceti, his target stars, gave us no evidence of extraterrestrial life, but we're continuing to refine the tools for detection. The Allen Telescope Array is just one example of the radio telescope equipment being brought to bear. The Low Frequency Array (LOFAR) and the Square Kilometer Array (SKA) will offer new SETI options in a wide range of wavelengths. SKA will cover 70 MHz to 10 GHz, later extending up to 30 GHz, while LOFAR will survey the skies from 10 to 240 MHz. LOFAR is currently being built and will be the most sensitive radio observatory in the world until SKA comes...

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Life’s Adaptations Among the Stars

Gliese 581 d seems to be emerging as the exoplanet to talk about in terms of possible life, at least for now. You'll recall that the initial furor was all about Gl 581 c, but that world now looks to be more Venus-like than anything else, while Gl 581 d may just skirt the outer region of the habitable zone in this interesting system. Thus Dirk Schulze-Makuch's contention at the recent astrobiology conference in Houston that this 'super Earth,' if it holds life, may have creatures on it that have adapted to the gravity of a planet at least seven times as massive as the Earth. That would probably produce a population that tends to crawl rather than fly, said the Washington State researcher, and we can let our imaginations go to work on the possibilities. As to Gl 581 d itself, its orbit around this red dwarf may place it in the same relative position that Mars is to our Sun, but throw in volcanoes, a magnetic shield and a thick atmosphere with water oceans below and you could have the...

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Restoring Earth: The Space Imperative

I've heard of Dyson spheres and Dyson swarms, but what exactly are Dyson 'dots'? As coined by Greg Matloff, C Bangs and Les Johnson in their book Paradise Regained, the term refers to a type of solar sail. These sails are not meant for moving things around the Solar System, but for reducing the amount of solar radiation hitting the Earth. The authors imagine large numbers of the Dyson dots placed near the L1 point, using the momentum from solar photons to maintain their position. Imagine thousands -- maybe millions -- of these sails equipped with sensors to receive the instructions of their builders, communicate with each other, and make changes in the configuration of the swarm. Could you use a sail array like this to cool off the planet? From the book: ...using reasonable middle values for the parasol parameters -- 80 percent reflectivity or albedo, mass 53 grams per square meter, positioned 2,100,000 kilometers from Earth -- we would need almost 700,000 km2 of sunshade area to...

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Clues to Missing Matter

We'd better get familiar with WHIM, the Warm-Hot Intergalactic Medium. According to some cosmologists, this sparse gas exists in the spaces between the galaxies, accounting for up to fifty percent of the normal matter found in today's universe. That would explain a conundrum. By 'normal matter,' I mean baryons, the protons and electrons of the matter we deal with every day. It turns out that we can study distant gas clouds and galaxies well enough to form an estimate of the normal matter found in the early universe, and the problem is that the nearby universe, much older, shows only about half the amount of normal matter that we would expect to find. Now researchers have used the Chandra X-ray Observatory and ESA's XMM-Newton to detect a huge reservoir of interstellar gas apparently embedded in a large-scale structure known as the Sculptor Wall, some 400 million light years from Earth, providing strong support for the WHIM theory. We're probably looking at material left over from the...

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Warm ‘Saturns’ and Their Moons

Recent work from the Lick-Carnegie team has found that the M-dwarf HIP 57050 is orbited by a Saturn-mass world with an orbital period of 41.4 days. What catches the eye about this exoplanet is its temperature, some 230 kelvin or -43 degrees Celsius, warm enough to place it in the habitable zone of the star. Based on our knowledge of the gas giants in our own Solar System, it's a natural supposition that this is a world with moons, and if so, their location in the habitable zone draws inevitable comparisons with fictional worlds like Pandora. M-dwarf Habitable Zones So what do we know about M-dwarfs that can help us with this system? For one thing, they're exciting objects for radial velocity studies because of their low mass, making the signature of an orbiting planet more readily apparent than with larger stars. We also know that their low temperatures move their habitable zones in much closer to the star than in our system, ranging from 0.1 to 0.2 AU, corresponding to an orbital...

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Voyager 2: The Art of Deep Space Repair

The fastest moving spacecraft in our Solar System is currently Voyager 1, which is moving at 61,419 kilometers per hour, a figure that works out to 17.06 kilometers per second. It's always interesting to weigh such speeds against the hypothetical upper limits we would get from certain kinds of propulsion. Geoffrey Landis told me years ago, when we were talking in his office at Glenn Research Center in Cleveland, that a reasonable Sun-diver maneuver (a close pass by the Sun to get the ultimate gravitational boost) might result in a properly designed solar sail getting up to 500 kilometers per second. Quite a jump from Voyager 1. On the other hand, contrast it to a journey to the nearest stars. Moving at 500 kilometers per second (assuming they could withstand the acceleration of the maneuver), the occupants of our solar sail starship would travel some 2580 years before reaching Centauri A and B. I've seen some extrapolations that get travel time to the Centauri stars down to about...

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Project Icarus Update

Is Jupiter the best place to collect massive amounts of helium-3? The Project Daedalus designers thought so. Back in the 1970s, members of the British Interplanetary Society set out to design a starship that would use pulsed fusion propulsion, with deuterium and helium-3 as fuel. Daedalus had mind-bending requirements, for the plan was to drive it to 12 percent of lightspeed on a flyby mission to Barnard's Star that would take fifty years to arrive. 250 pellets of deuterium and helium-3 would be detonated every second in its combustion chamber over a thrust period of four years. That calls for a lot of fuel, and therein lies the problem. Fueling Up the Probe We can find deuterium (an isotope of hydrogen) right here on Earth, but helium-3 is a rarity. The Daedalus team figured it needed some 30,000 tons of helium-3, so it envisioned mining Jupiter's atmosphere, where the stuff is plentiful. Imagine floating factories in the atmosphere of the giant planet using waste heat to generate...

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Finding Titan on Earth

Finding life on a world in the outer Solar System -- think Enceladus or Titan for starters -- would be an extraordinary step forward. Martian microbes, if they exist, might be evidence of contamination, or we might be evidence of ancient contamination from Mars, given the ready exchange of materials between our planets in the last several billion years. But the outer system offers the possibility of discovering life that originated entirely separately from anything we know. The problem is that we're a long way from having built the spacecraft that can make these detections. That's why places like Pitch Lake, on the island of Trinidad, are so useful. Other than the temperature, conditions here are about as close to what we might find on Titan as anything we know. The 114-acre lake is a cauldron of hot asphalt permeated with hydrocarbon gases and carbon dioxide. As you can see in the image below, it's hardly a hospitable-looking place. But this asphalt hell-hole defies expectation. As...

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Artificial Intelligence Among the Stars

Talk of a 'singularity' in which artificial intelligence reaches such levels that it moves beyond human capability and comprehension plays inevitably into the realm of interstellar studies. Some have speculated, as Paul Davies does in The Eerie Silence, that any civilization we make contact with will likely be made up of intelligent machines, the natural development of computer technology's evolution. But even without a singularity, it's clear that artificial intelligence will have to play an increasing role in space exploration. If we develop the propulsion technologies to get an interstellar probe off to Alpha Centauri, we'll need an intelligence onboard that can continue to function for the duration of the journey, which could last centuries, or at the very least decades. Not only that, the onboard AI will have to make necessary repairs, perform essential tasks like navigation, conduct observations and scientific studies and plan and execute arrival into the destination system....

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SETI: Handling a Detection

The Stephen Hawking controversy continues to bubble, with discussion on the Larry King show and the appearance of David Brin's essay The Other Kind of Aliens. It's all to the good to get such discussions widely circulated, even if it can be dismaying to find that so many respondents believe the answers about how alien cultures will behave are obvious and can be readily deduced from our own cultural experiences. But maybe that's because this is a new controversy, one that the search for exoplanets is only now bringing to a wider public in any serious way. There is plenty to ponder, and while we debate the nature of alien culture, let's look at something more immediate. The Protocols of SETI Success SETI continues to look for signals of extraterrestrial civilizations. What happens if a signal is actually detected? For the answer, we can look to the SETI Post-Detection Taskgroup, created by the SETI Permanent Study Group of the IAA (International Academy of Astronautics). The...

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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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