Conference Evaluates Mars Express Results

Here's an image of the possible Martian pack ice, taken by Mars Express' High Resolution Stereo Camera (HRSC), which is imaging the entire planet in full colour, 3-D and with a resolution of about 10 metres. The 3-D capability allows us to see Martian topography in unprecedented detail. Look here for other extraordinarily detailed images. This image, taken by the High Resolution Stereo Camera (HRSC) on board ESA's Mars Express spacecraft, during orbit 32, shows what appears to be a dust-covered frozen sea near the Martian equator. It shows a flat plain, part of the Elysium Planitia. The scene is a few tens of kilometres across, centred on latitude 5º North and longitude 150º East. Credits: ESA/DLR/FU Berlin (G. Neukum) Meanwhile, findings from Mars Express were discussed in a news conference on the 25th. To say the session was packed with news is an understatement: we have not only the possible pack ice but discussions of Martian methane and formaledhyde and their significance for...

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A New Set of Nearby Stars

The American Astronomical Society meeting in San Diego yielded results we'll be discussing all year. One study that comes immediately to mind (with a paper scheduled for the Astronomical Journal in April) is the work of Wei-Chun Jao and the Research Consortium on Nearby Stars (RECONS) team at Georgia State University, who have measured the distance to four stars -- all of them red dwarfs -- within 33 light years of the Sun. All told, the team has found 26 new neighbors within 25 parsecs (82 light-years), along with the first confirmed binaries comprising a red subdwarf and a white dwarf. Subdwarfs are highly unusual stars, with extremely low metallicity; i.e., few elements heavier than hydrogen and helium. From a press release on the star measurements: Another indicator that both systems are old is that each travels through the Galaxy at nearly 150 km/sec (roughly 100 miles/sec). Contrary to people, older stars like the Jupiter-sized red subdwarfs generally move faster than their...

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Cassini and the Naming of Names

Twenty-four craters on Saturn's tiny moon Phoebe have now been deemed prominent enough to receive their own names. Phoebe was honored by the names of the Argonauts, the explorers who sailed with Jason to find the golden fleece; its largest crater has been christened Jason. The tale was known in the days of Homer and may have served as a pattern for the wanderings of Odysseus. It is most famously told in a four-book epic by Apollonius of Rhodes, one time custodian of the fabulous library of Alexandria. "We picked the legend of the Argonauts for Phoebe as it has some resonance with the exploration of the Saturn system by Cassini-Huygens," said Dr. Toby Owen, of the University of Hawaii at Manoa. He is the chairman of the International Astronomical Union Outer Solar System Task Group and an interdisciplinary scientist on the Cassini-Huygens mission. "We can't say that our participating scientists include heroes like Hercules and Atalanta, but they do represent a wide, international...

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Cryogenic Survival of Ancient Bacteria

Storing and preserving living cells at low temperatures is a staple of science fiction. Who knows how many fictional interstellar journeys have taken place with the crew in cryogenic suspension (my favorite, Van Vogt's "Far Centaurus," springs quickly to mind, but there are many possible references). And with the possibility of Martian ice -- even an ancient Martian sea -- under observation by Mars Express, the question of life surviving in extreme conditions is drawing increased attention. Which is why the discovery of of a new bacterium called Carnobacterium pleistocenium is so interesting. NASA astrobiologist Richard Hoover and his team found the anaerobic bacteria, which grow on sugars and proteins in the absence of oxygen, at the U.S. Army's Cold Regions Research and Engineering Laboratory tunnel north of Fairbanks, Alaska. The tunnel was created in the 1960s to allow scientists to study permafrost as part of the preparation for building the Trans-Alaska Oil Pipeline. Hoover's...

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Doubts on Martian Formaldehyde

Oliver Morton's excellent MainlyMartian weblog has a cautionary analysis of Vittorio Formisano's work on Martian formaldehyde, which we looked at on the 18th. From the weblog: I've posted on the formaldehyde story before. And, even more now than then, I think Formisano is making a mistake...[S]o do a number (quite possibly, from what I hear, all) of his colleagues on the PFS, including those who have more experience modelling atmospheric chemistry and interpreting spectrometer data than Formisano has. I don't want to rehash everything in the earlier post on the subject, but the gist is that a) formaldehyde is expected to have a very short lifetime in the atmosphere, and thus it is very hard to explain how there could be so much of it and b) earth-based telescopes have looked for the stuff and found no evidence for it even at levels far lower than those that Formisano appears to see. You can read Morton's comments here. He has also written thoughtfully on the 'Elysium Sea' (the...

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Transit Timing to Detect Terrestrial Planets

"The Use of Transit Timing to Detect Terrestrial-Mass Extrasolar Planets," by Matthew Holman (Harvard-Smithsonian Center for Astrophysics) and Norman Murray at the University of Toronto, appears in the February 25th issue of Science. The paper covers a new planet-finding technique that studies transit time; i.e., the amount of time it takes a planet to orbit its star. Transit timing studies the variation in apparent stellar brightness caused by the passage of a planet in front of its star as seen from Earth. Because the timing of the transit will vary depending on the presence of other planets in the system, astronomers should be able to make estimates about the mass of a second planet. And here's the best part: While the current radial velocity observations that have been used to detect most of the 150 known extrasolar planets cannot be used for terrestrial worlds, this method may just be sensitive enough to detect them. The method has implications for future transit studies,...

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A Galaxy Made of Dark Matter

Ordinary (or baryonic) matter -- the stuff that you and I and Procyon are made of -- is outnumbered five to one by so-called 'dark matter,' mysterious stuff whose presence can only be inferred from the way galaxies rotate. Some galaxies rotate so fast that, if they were made only of ordinary matter, they would fly apart. So some stronger gravitational force must be involved, even though we can't see what's causing it. Now an international team of astronomers has found a valuable clue in the form of a galaxy that is all but invisible. VIRGOHI21 was found in the Virgo cluster of galaxies some 50 million light years from Earth, and is the first galaxy ever detected that is made up almost entirely of dark matter. Observed by radio telescopes at the University of Manchester and Arecibo (and later studied at the Isaac Newton Telescope in the Canary Islands), the galaxy contains a mass of hydrogen atoms a hundred million times larger than the Sun. The mass rotates, just like a galaxy, but...

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Martian ‘Pack Ice’ Energizes Researchers

The recent finding of a possible ancient sea on Mars has been one of the hotter topics at the ESA Mars Science Conference. The research team, led by John Murray of the UK's Open University, presented its findings at the conference on the 21st, with a paper coming up in Nature next month. One team member, Jan-Peter Muller of University College London had this to say about the significance of the find: "The fact that there have been warm and wet places beneath the surface of Mars since before life began on Earth, and that some are probably still there, means that there is a possibility that primitive micro-organisms survive on Mars today. This mission has changed many of my long-held opinions about Mars - we now have to go there and check it out." Amen to that, since even with instruments like Mars Express' High Resolution Stereo Camera, which offered up the 3D images used in this work, we need hard evidence from the surface before we can claim that life is anything more than a...

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Mars Express Findings Under Debate in Netherlands

The Mars Express conference being held at the European Space Research and Technology Centre in the Netherlands runs through the 25th, and as we saw yesterday is already generating its share of high quality data. The program for the meeting can be found here. Of particular interest will be the special session on exobiology and the hunt for life on Mars that will be held on Thursday the 24th. We should get more information about that conjectural Martian ocean (discussed yesterday) at that gathering. Meanwhile, six papers published online by the journal Science have brought forth new findings about the early history of Mars. "If you want to resolve the big question about life on Mars, you want to go to the right places and get samples," said Brown University's John Mustard. "The new research tells us where some of those places may be." Mustard is part of an international team using data from the Mars Express OMEGA spectrometer that is mapping the surface of the planet in both visible...

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An Ancient Martian Sea?

The Mars Express spacecraft has sent back images that some are interpreting as the broken plates of a Martian sea, surviving in the form of pack ice. New Scientist is running the story, saying the sea appears to be about 800 by 900 kilometers in size and is found 5 degrees north of the Martian equator. From the story: Images from the High Resolution Stereo Camera on Mars Express show raft-like ground structures - dubbed "plates" - that look similar to ice formations near Earth's poles, according to an international team of scientists. But the site of the plates, near the equator, means that sunlight should have melted any ice there. So the team suggests that a layer of volcanic ash, perhaps a few centimetres thick, may protect the structures. We should have more on this tomorrow, since the leader of the research team, John Murray at the Open University, UK is supposed to present the findings at 1st Mars Express Science Conference in Noordwijk, the Netherlands,...

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On Deep Space and the Imagination

How do we create our image of other worlds? The obvious answer -- through instrumentation on space probes -- is inadequate, because the raw data sent back by our spacecraft has to be assembled into the final images we see. Consider Hubble, which uses filters recording different wavelengths of light, and then combines them to create the image. Nor do we need confine ourselves to visible light, since we also get images in the infrared, and views filtered in whatever way will maximize science, like some of Cassini's radar images of Titan. Instead of just seeing an image, we assemble it. What you would see if you were actually there, in other words, isn't necessarily what you get. I notice that Elizabeth Kessler, a doctoral student in the University of Chicago's Committee on the History of Culture, has presented her work on Hubble and artistry at the annual meeting of the American Association for the Advancement of Science in Washington. The title of her talk, "Hubble's Vision: Imaging,...

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A Thought for the Weekend

"...in the historical perspective, the seafaring nations of Europe grew mighty from the wealth returned from the discovery and settlement of the new world. Those societies who stayed home languished, those who embraced the unknown prospered. Seen broadly, we're a species which owes its current success to exploration. Exploration generates opportunities which lead to economic strength, and exploration yields situational awareness which creates survival options. It contributes directly to our survival, not by giving us a second home if we screw this one up - I think that's kind of a lame argument - but by giving us interplanetary technical capability which will allow us to police and secure our own backyard, the solar system. It might possibly give us the means to deliver ourselves from destruction in this cosmic shooting gallery. "Right now if we discovered a comet nucleus or an asteroid on impact course with Earth, we could do exactly what the dinosaurs did, and we could stare upward...

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Mars Story Update

The Bad Astronomy site is reporting that Space.com's story about possible life on Mars has blown up. There apparently is no upcoming article in Nature, nor did researchers Carol Stoker and Larry Lemke engage in a private meeting with space officials to discuss the implications of their work along Spain's Rio Tinto. You can read the whole thing here. Later: Space.com's revised story is now available.

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NASA Denies Mars Claim

This news release from NASA headquarters may slow down the current life on Mars story: News reports on February 16, 2005, that NASA scientists from Ames Research Center, Moffett Field, Calif., have found strong evidence that life may exist on Mars are incorrect. NASA does not have any observational data from any current Mars missions that supports this claim. The work by the scientists mentioned in the reports cannot be used to directly infer anything about life on Mars, but may help formulate the strategy for how to search for martian life. Their research concerns extreme environments on Earth as analogs of possible environments on Mars. No research paper has been submitted by them to any scientific journal asserting martian life. Centauri Dreams note: The NASA press release discusses the work of Carol Stoker and Larry Lemke at Ames Research Center, published as an exclusive by Space.com and described in the February 17 entry below. Today's entry describing Vittorio Formisano's work...

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Solar Sail Launch Now Scheduled for April

The Planetary Society offers an update on its Cosmos 1 solar sail with the announcement that the spacecraft launch date has slipped to April. Planetary Society executive director Louis Friedman said all flight components had been tested and a full-mission sequence simulated with the spacecraft's on-board computer. The sails are not yet attached to the spacecraft, but will be folded for attachment within the next two weeks. Cosmos 1 will then undergo vacuum chamber testing to check for leaks in its compressed air and fuel lines before being shipped to the launch area. Launch will be aboard a Volna rocket from a Delta III Russian submarine in the Barents Sea. "There is no way to simulate or adequately test how a sail, which is 30 meters long and 5-millionths of a meter thick, will behave under weightless conditions in a vacuum," writes Friedman. "It could oscillate, bounce around and even rip apart. Or it could spread wide and sail effortlessly on beams of light as we hope it will. Our...

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Is Formaldehyde an Indicator of Martian Life?

New Scientist continues the focus on possible Martian life with a story on Vittorio Formisano, a European Space Agency scientist who believes he has found formaldehyde on the Red Planet. His data come from the Planetary Fourier Spectrometer aboard Mars Express, and indicate a formaldehyde concentration of 130 parts per billion. Formisano, from the Institute of Physics and Interplanetary Science in Rome, will present these results next week at a conference in the Netherlands. Formisano's views are bound to be controversial; the scientist believes the formaldehyde is being produced by the oxidation of methane, and says that 2.5 million tons of methane would need to be generated each year to create this much of it. New Scientist writer Jenny Hogan quotes Formisano in A Whiff of Life on the Red Planet: "I believe that until it is demonstrated that non-biological processes can produce this, possibly the only way to produce so much methane is life," [Formisano] says. "My conclusion is...

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A Challenge to Planetary Formation Theories

February's issue of the journal Icarus will refine an increasingly intriguing theory of planetary formation. Richard Durisen, a professor of astronomy at Indiana University - Bloomington used computer models to demonstrate the motion of gas as it condenses around a parent star. "These are the disks of gas and dust that astronomers see around most young stars, from which planets form," Durisen said. "They're like a giant whirlpool swirling around the star in orbit. Our own solar system formed out of such a disk." What Durisen's theory of gravitational imbalances adds to the picture is a model of how areas of stability within the planetary disks create places for denser gases to accumulate, allowing the formation of planets. That's valuable information, because until now we haven't understood how a gravitationally unstable disk could avoid violent interactions with other disks materials, thus destroying young planets before they could fully form. Image: The rings near the center of...

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Life on Mars? Not So Fast…

In NASA Researchers Claim Evidence of Present Life on Mars, Space.com writer Brian Berger reports that two NASA scientists have evidence that life may exist on Mars. Which is true enough, though not in itself new, since uneven methane signatures in the Martian atmosphere (detected in 2004 by Mars Express) have already revealed the possibility of an underground biosphere. What Carol Stoker and Larry Lemke of NASA's Ames Research Center in Silicon Valley bring to the table are their findings in southwestern Spain, where the the acidic ecology of the Rio Tinto offers an environment somewhat similar to Mars. It's telling that concentrations of the mineral salt jarosite have been identified both on Mars and in hot springs and bodies of water like the Rio Tinto. If life could exist in an underground microbial ecosystem under conditions not terribly dissimilar from Mars, it might also be found on Mars itself. But proceed with caution. Stoker and Lemke won't have their paper out until May;...

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Neutrino Telescope May Revise Story of Early Cosmos

Construction of the world's largest scientific instrument is proceeding in the frigid wastes of Antarctica. The initial deployment of what will become the IceCube neutrino telescope involved drilling a 1.5-mile deep hole into Antarctic ice, then installing 60 optical detectors in it that will detect the elusive particles. But that's just the beginning: IceCube demands 70 such holes and 4200 of the volley-ball sized optical detectors. The final telescope will take up a cubic kilometer of ice and capture particles from the edge of the visible universe. What makes neutrinos so interesting is their ability to travel vast distances without deflection or absorption; they seem to pass ghost-like through ordinary matter, and are unaffected by magnetic fields. "Neutrinos travel like bullets through a rainstorm," Francis Halzen, a University of Wisconsin-Madison professor of physics and the principal investigator for the project explains. "Immense instruments are required to find neutrinos in...

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New Huygens Audio as Cassini Heads for Enceladus

What Cassini heard from Huygens as it descended to Titan's surface is now available as an audio file from the European Space Agency, but it may be easier to download it from Ralph Lorenz' home page. Lorenz is an assistant research scientist at the University of Arizona's Lunar and Planetary Laboratory and a co-investigator on Huygens' Surface Science Package; he created the sound file based on Cassini data. The file compresses four hours of real-time audio into about a minute. What the listener hears is a tone whose frequency depends on the strength of the Huygens signal as received by Cassini. The probe's antenna emitted radio energy unevenly, "...like the petals of a flower rather than the smooth shape of a fruit," as Lorenz puts it. As the probe's orientation changed durings its long descent, its spin rate slowed, causing rapid changes in the tone. "You can hear how the motion becomes slower and steadier later in the descent," Lorenz said. A UA press release on Lorenz' work can be...

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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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