Aosta Update for Wednesday

Today we get into the heart of this interstellar conference, with multiple sessions on propulsion via solar and electric sail, as well as looks at specific mission concepts and robotic applications in deep space. I spent a good part of our bus ride back from Bard castle yesterday talking to Pekka Janhunen, creator of the electric sail concept, about its possible interstellar applications. Pekka does not believe this system, based on electric tethers riding the solar wind, could muster the velocity to go interstellar, but he does see it as a viable candidate for braking into a destination system, and just as important, exploring it. I'm anxious to get the latest on his work and also to look at fusion alternatives, which Claudio Maccone will present now that we've learned that Claudio Bruno can't make it here. As I get ready for the day to start, I'll drop in here some notes from the first day. These are no more than a skeletal outline -- I'll use the conference proceedings when I get...

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Busy Times in Northern Italy

I had intended to use today's post to talk about yesterday's sessions here in Aosta, but it's going on midnight here, and tomorrow will clearly not afford any opportunities to write. Tuesday turns out to be our sightseeing day. We leave the hotel at 9:00 and head for Verrès, where we visit the Mechatronics Laboratory of the Politecnico di Torino. Then we head up into the mountains, visiting the Bard fortress, with individual visits to the Museum of the Alps. After lunch at what is said to be an excellent restaurant called La Polveriera, we go to an exhibition called 'Verso l'alto, l'ascesa come esperienza del sacro' -- Towards the heights: The ascent as experience of the sacred. Then to dinner at the Hotel Notre Maison, where we are promised traditional Aosta Valley food. Image: The Aosta town hall, where our opening sessions were held. Later, we moved to the Hotel Europe. As for tomorrow, we don't get back to the hotel until midnight. No more today or I'll be late for the bus, but...

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First Day in Aosta

What I'll surely remember the most about arriving in Italy is the sight of snow on the Alps as the plane descended out of a cloudy morning sky into Milan. But right after that comes the two hang gliders that soared past an alpine peak as the van that was taking me to Aosta moved north toward the town, the landscape becoming a series of valleys cutting through the steep clefts. The second of the two hang gliders looked for all the world as if it were going to land right on the highway, a daunting thought given how the traffic was moving, but as we rounded a turn I saw that it had caught an updraft and was angling out and away. What a view the pilot must have had. Image: The view from my room at the Hotel Europe in Aosta. It was hot and humid when I took this, but cooled off dramatically during the night. If the air conditioner worked, all would be perfect. Below is a photo from the street in front of the hotel. As you can tell, this is the place to be for a guy who loves mountains the...

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Notes & Queries 7/3/09

Night Flight to Italy I'm off tomorrow night to Italy, specifically to the Sixth IAA Symposium on Realistic Near-Term Advanced Scientific Space Missions. I'll be delivering a talk at the conference and a public lecture in the town of Aosta and, assuming a robust Internet connection, I'll also be sending along news of the conference as it unfolds. I'm looking forward particularly to catching up with Giancarlo Genta, Greg Matloff and wife C Bangs, and Claudio Maccone, and it will be great to touch base again with Les Johnson, whom I haven't seen since we talked at Marshall Space Flight Center in 2003. Superluminal Radio Waves and their Uses An article in the Santa Fe New Mexican discusses the work of John Singleton, a physicist at Los Alamos National Laboratory, who has created a 'polarization synchrotron,' which according to the report pushes radio waves faster than the speed of light. In a paper on this work, Singleton explains that: ...though no superluminal source of...

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Two Stars, Two Systems?

Imagine what space exploration would look like if the Sun were a member of a binary system. Suppose we had another star a few hundred AU away, one that had built its own planetary system. The second star, a thousand times brighter than any other star in our night sky, would be an object of obvious interest, its planets visible to our astronomers and reachable targets for early space technology. The question of life on a planet in that star's habitable zone would be relatively easy to resolve, and the imperative to study that world first-hand would surely drive space science. Now we learn that a binary system some 1300 light years from Earth may be evolving in a similar direction. Located in the Orion Nebula, a region rich in star-birth, the stars are about a third the mass of the Sun, considerably cooler and redder in color. One is known to be an M2 dwarf, while the other's spectral type hasn't been precisely identified because of obscuration by the disk. The stars are 400 AU apart,...

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Of Technological Lifetimes and Survival

Is the movement toward ever more sophisticated technology irreversible? If you've studied history, the answer is obviously no. Various speculations arise from this -- Carl Sagan once opined that without the intervening collapse known as the Dark Ages, we might have seen a Greek civilization exploring near-Earth space a thousand years ago. It's also likely that no law prevents another collapse into technological and scientific somnolence, perhaps sparked by war, or disease, or economic catastrophe. This is why I always hedge my bets when asked about timetables for space exploration. How long until we get humans to the outer system? How long until we launch a fast starship? Everyone is in a hurry, but so much depends on whether we keep growing our technology. Nanotechnology, for example, could change everything, but it's one thing to be using molecular assemblers by the end of the century, and quite another to see the fruition of this work stalled for a millennium by external events....

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‘Blobs’ Flag Early Galaxy Formation

Look back far enough in time (and hence far enough in distance) and you see things that don't correspond to nearby cosmic objects. The so-called 'Lyman-alpha blobs' that astronomers have found associated with young, distant galaxies are a case in point. Huge collections of hydrogen gas (some of them the largest single objects yet found in the universe), they're bright at optical wavelengths, raising the question of what powers the glow and how they factored into the galaxy formation process. New research may be offering an answer. The key is something called 'feedback,' a stage in galaxy formation that shows the interplay between galaxies and the intergalactic medium. Here, the cooling of gas within the dark matter halos enshrouding a young galaxy is countered by heating from active galactic nuclei (think supermassive black holes), which helps to enrich intergalactic space and also slow down star formation. Image: An artist's representation showing what one of the galaxies inside a...

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Finding Life in the Ice

As we contemplate using long-range tools like spectroscopy to examine distant exoplanets for life, we're also developing the hands-on equipment we'll need for seeking it out in our own Solar System. Project SLIce (Signatures of Life in Ice) is a case in point, an attempt to study how organic material behaves in ice on other worlds by using Earth settings as an analogy. On that score, the archipelago of Svalbard has proven to be a helpful testbed. Located in the Arctic Ocean between Norway and the North Pole, Svalbard is icy and spectacular. The image below conjures up memories of a nautical journey I took around Iceland in the 1970s, with white-capped seas pushing up against snow-clad peaks. The SLIce team sees Svalbard as a laboratory for looking for extant or extinct life, and a place to develop the protocols for working with rovers in operating environments like Mars. Image: I love Iceland, but pushing as far north as Svalbard would really bring out the adventurer in me. Here we...

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A Cometary Closeup for NExT

By Larry Klaes Apropos of yesterday's story on the possible cometary origin of the Tunguska Event in 1908, Tau Zero journalist Larry Klaes looks at the NExT (New Exploration of Tempel) mission, which gives us a second crack at observing comet Tempel 1. Ancient artifacts of the early Solar System, comets can tell us much about its earliest days, but as Larry points out, getting data out of the Deep Impact mission proved to be unexpectedly complicated. NExT is a useful re-purposing of an earlier mission that may unlock further cometary secrets when it returns to Tempel 1 in 2011. If a comet did cause Tunguska, here's hoping such events continue to be rare, but in the meantime, garnering all the information we can about how comets are made is as important for planetary security as it is for the study of Solar System origins. An Impact to Remember Late on the Fourth of July in 2005, while fireworks brightened the sky across the United States, another group of American citizens were...

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Comet Implicated in Tunguska Blast

Back in my flying days, I found myself becoming absorbed with meteorology, enough to wind up teaching the subject in various flight school settings. I was no expert, but looking for clues on flying conditions in the next few hours by studying cloud formation and movement was fascinating. In all that time, the one cloud phenomenon I always wanted to see but never did was the noctilucent cloud, an unusual, lovely formation made up of ice particles that occurs at extremely high altitudes. 'Noctilucent' means 'night-shining,' and that's just what these clouds do when they're illuminated by sunlight from below the horizon. Space Shuttle launches have been found to generate them as the vehicle pumps about 300 metric tons of water vapor into the thermosphere, the layer of atmosphere beginning at about ninety kilometers above the surface, just above the mesosphere. Photographs of such clouds show a unique beauty, though it's one that might also seem eerie, at least in certain settings. For...

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Enceladus: Riddle of the Plumes

Is there really an underground ocean on Enceladus? The Cassini spacecraft's striking images have created a cottage industry in speculation, with spectacular glimpses of erupting plumes composed of ice and water vapor. This week, however, we get two contrasting views on what all this means. In one, a paper in Nature by a European team led by Frank Postberg (Universität Heidelberg), studies of sodium salts in dust ejected by the Enceladus plumes reveal telltale signs of a salty ocean deep below the surface. Postberg was working with data from the Cosmic Dust Analyzer (CDA) instrument aboard Cassini, and the results imply a level of sodium chloride that may be as high as that found in Earth's oceans. The data come from ice grains in Saturn's E-ring, which is thought to consist largely of material from Enceladus. Thus we seem to be gathering direct evidence for the presence of the hypothesized ocean, which should be salty from long contact with the rocky core. But not so fast. The same...

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SETI: A Detectable Neutrino Signal?

Somehow I never thought of the IceCube neutrino telescope as a SETI instrument. Deployed in a series of 1,450 to 2,450 meters-deep holes in Antarctica and taking up over a cubic kilometer of ice, IceCube is fine-tuned to detect neutrinos. That makes it a useful tool for studying violent events like galactic collisions and the formation of quasars, providing insights into the early universe. But SETI? Perhaps, says Zurab Silagadze (Novosibirsk State University), who notes that most SETI work in the past has focused on centimeter wavelength electromagnetic signals. Says Silagadze: Here we question this old wisdom and argue that the muon collider, certainly in reach of modern day technology... provides a far more unique marker of civilizations like our own [type I in Kardashev's classification... Muon colliders are accompanied by a very intense and collimated high-energy neutrino beam which can be readily detected even at astronomical distances. Image: The IceCube array in the deep ice,...

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TESS Mission Fails to Make the Cut

NASA has made its choices, and TESS is not one of them. The Transiting Exoplanet Survey Satellite would have used six telescopes to observe the brightest stars in the sky, a remarkable 2.5 million of them, hoping to find more than 1,000 transiting planets ranging in size from Jupiter-mass down to rocky worlds like our own. An entrant in the agency's Small Explorer program, TESS could have accelerated the time-frame for discovering another habitable world, assuming all went well. Not that we don't have Kepler at work on 100,000 distant stars, looking for transits that can give us some solid statistical knowledge of how often terrestrial (and other) planets occur. And, of course, the CoRoT mission is actively in the hunt. But TESS would have complemented both, looking at a wide variety of stars, many of which would have been M-dwarfs. Not long ago I referred to a Greg Laughlin post that noted a 98 percent probability that TESS would locate a potentially habitable transiting planet...

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Brute-Force Engineering and Climate

The eruption of Mt. Tambora in Indonesia in 1815 pumped so much sulfur dioxide into the stratosphere that New England farmers found their fields frosted over in July. Climate change, it seems, can be quick and overwhelming, at least on short scales. The eruption of the Mt. Pinatubo in the Philippines in 1991 cooled global temperatures for several years by about half a degree Celsius. Sulfur dioxide works. So how about this: We send a fleet of airships high into the stratosphere, attached to hoses on the ground that pump 10 kilos of sulfur dioxide every second. The airships then spew this mix into the upper atmosphere, a aerosolized pollutant that, turning the skies Blade Runner red, shields the planet from the Sun's heat. Call it geo-engineering, an extreme form of human climate manipulation that is the subject of a recent story in The Atlantic. Into the Anthropocene Writer Graeme Wood notes that our activities have been transforming the planet for centuries now, leading some to dub...

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Huge Outburst from a Magnetar

We get yet another example of space-based observatories complementing each other with the recent outburst of X-rays and gamma rays detected last August. The Swift satellite first noted the event on August 22, while the European Space Agency's XMM-Newton satellite began making detailed spectral studies of the radiation twelve hours later, followed by the Integral observatory. The outburst went on for more than four months, accompanied by hundreds of smaller bursts. The source for these events was a magnetar, a type of neutron star that is the most highly magnetized object known, with a magnetic field some 10,000 million times stronger than Earth's. The new magnetar, christened SGR 0501+4516, is of the type known as Soft Gamma-Ray Repeaters (SGR), and is the first such found in the last decade. Magnetars are known for spectacular periods of irregular burst activity, changing their luminosity up to ten orders of magnitude on timescales of just a few milliseconds. We occasionally discuss...

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Two Angles on Meteorites

Meteorites are in the news in two starkly different ways this week, but I'll lead with a story that has implications for how planetary systems like ours are born. Philipp Heck (University of Chicago) and colleagues have been analyzing interstellar grains from the Murchison meteorite, a large object that fell near the town of Murchison, Victoria in Australia in 1969. The Murchison grains are thought to have been blown into space by dying stars long before the formation of Earth. We'd like to know more about such grains because they became incorporated into the earliest solids forming in the Solar System, and hence offer a window into that era. Moreover, their composition helps us understand a bit more about their history. "The concentration of neon," says Heck, "produced during cosmic-ray irradiation, allows us to determine the time a grain has spent in interstellar space." Image: A fragment of the Murchison meteorite. Copyright New England Meteoritical Services, 2001. The...

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Notes & Queries 6/16/09

Life Beneath the Ice Three kilometers down in the Greenland ice sheet is what I call an extreme environment. Even so, Penn State researchers have been able to bring a bacterium called Herminiimonas glaciei back to life after a dormancy of 120,000 years in these conditions. The work involved incubating the samples at 2 degrees Celsius for seven months, then at 5 degrees Celsius for a further four and a half, a patient process rewarded by the appearance of the purple-brown bacteria. Ten to fifty times smaller than E. coli, Herminiimonas glaciei evidently used its size to survive in liquid veins amongst the ice crystals. Jennifer Loveland-Curtze describes the find: "These extremely cold environments are the best analogues of possible extraterrestrial habitats. The exceptionally low temperatures can preserve cells and nucleic acids for even millions of years. H. glaciei is one of just a handful of officially described ultra-small species and the only one so far from the Greenland ice...

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A Longer Life for Earth’s Biosphere?

If we can find a way to double the lifespan of Earth's biosphere, we'll have changed the odds for finding extraterrestrial civilizations. After all, the amount of time an advanced culture can exist is one of the variables in the famous Drake equation, which estimates how many intelligent civilizations there are in the Milky Way. Lengthen potential habitability and you give any civilization that much more chance to spread into the cosmos. Thus recent work out of Caltech intrigues us in several directions. Joseph Kirschvink and colleagues look at effects that could add a billion years on to our planet's projected habitability. Consider: Earth took some four billion years to develop intelligent life, leaving us about a billion before our planet becomes uninhabitable. That result would be caused by a brighter and hotter Sun, the loss of carbon dioxide in the atmosphere through the weathering of rocks, and the eventual evaporation of water from the oceans, leaving nothing alive. Reducing...

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Modeling an Interstellar Future

The bet between Tibor Pacher and myself continues to draw emails, proving that my friend Tibor was right when he saw an interstellar wager as a teaching opportunity. I still maintain that an interstellar mission will not be launched anywhere near as early as 2025, but Tibor does have his advocates, as you can see on the Long Bets site. Moreover, it's been useful to plug in distances and velocities for a 2000-year mission to a place like Proxima Centauri when I speak to audiences about how large the distance between the stars really is. 2000 years is a long time, but we're still talking 650 kilometers per second, and just 20 years to the Oort Cloud! And as a guy who used to build model airplanes back in my youth, first in plastic and then from balsa wood (wonderful memories of working with kits of World War I and II aircraft from Guillow), I can relate to Tibor's latest venture. MiniSpaceWorld is an attempt to create, at a European site still to be determined, a wide-ranging exhibit...

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Earthlight’s Bio-signature Measured

Among the most interesting of the future missions now being weighed by NASA, TESS (the Transiting Exoplanet Survey Satellite) would help scientists using the James Webb Space Telescope know where to look for Earth-like planets around nearby stars. While the invaluable Kepler mission scans 100,000 distant stars, hoping to gain statistics on Earth-sized exoplanets, TESS would have a different aim, looking for transiting terrestrial worlds around only the brightest stars. A 2012 launch is possible if the mission is approved. Here's Greg Laughlin (UC-Santa Cruz) on TESS' possibilities: TESS... provides the cheapest, shortest, and most direct path to the actual characterization of a potentially habitable planet. Included in the 2.5 million brightest stars are a substantial number of M dwarfs. Detailed Monte-Carlo simulations indicate that there's a 98% probability that TESS will locate a potentially habitable transiting terrestrial planet orbiting a red dwarf lying closer than 50 parsecs....

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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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