Ed Minchau offers up the latest Carnival of Space at his Robot Guy site. Centauri Dreams readers will want to look at Amanda Bauer's presentation of an image taken by the Pluto-bound New Horizons spacecraft. It's actually a composite showing Jupiter and a startlingly nearby Io. We've all seen Jupiter images, of course (thank you Voyager, Galileo, et al.), but take a look at this one to note the plume of the erupting Tvashtar volcano, a stunning reminder of how active this tortured little world continues to be. Space Files has a nice overview of solar sail technologies beginning with Lou Friedman's plans to develop Cosmos-2, a replacement for the lamented sail that perished in its launch attempt back in 2005. We still need to shake out this intriguing concept in space, and with NASA funding for sails in limbo, the private sector is the place to turn. Space Files gets into Japan's recent experiments (useful as we learn how to deploy various sail configurations) and ESA's GeoSail study....
Of Impatience and Stellar Distance
One thing I'm always asked when I talk about interstellar topics is how long it would take a spacecraft like Voyager to get to the nearest star. After explaining how far away Proxima Centauri and the slightly farther Centauri A and B really are, I tell the audience that Voyager, if headed in that direction, would be facing a travel time of over 70,000 years. That usually shifts the conversation considerably, because many people assume that if we can get to the outer planets, the nearest stars can't be that far behind. If only it were so. The Centauri stars are, of course, only the closest known (and who knows, perhaps there's a brown dwarf a bit closer). Assume a space technology able to travel at close to the speed of light and you're still dealing with travel times that amount to years, although time for the crew would be shorted according to those interesting Einsteinian effects that cause the crew of a vehicle traveling at 86 percent of lightspeed to experience half the elapsed...
Probing Exoplanet Atmospheres in Texas
With Hubble's Space Telescope Imaging Spectrograph now out of commission, the study of exoplanetary atmospheres becomes a bit more problematic. But Seth Redfield (University of Texas at Austin) has now used a ground-based instrument to detect the atmosphere of a planet orbiting the star HD189733, some 63 light years away in the constellation Vulpecula. Discovered in 2004, this transiting world is about twenty percent more massive than Jupiter, orbiting its parent ten times closer than Mercury orbits our Sun. Working from the ground is tricky but the odds go up when you observe more than a single transit. Redfield worked with eleven transits observed over the course of a year, using the Hobby-Eberly Telescope (HET) at McDonald Observatory in Austin. Studying the chemical composition of a distant atmosphere involves taking a spectrum during a transit and another when no transit is occurring. Working with the difference and comparing results over multiple transits helps you put together...
Site Security Bug Fixed
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Allen Telescope Array: Listening for ETI
By Larry Klaes Larry Klaes' look at the Allen Telescope Array reminds us of the power of philanthropy at getting serious projects funded. It's a topic we'll be re-visiting as the Tau Zero Foundation comes online early in the coming year. I'm reminded also of the One Laptop Per Child project, which is seeing private donations for these educational tools supplanting government shortfalls in some developing countries. Properly targeted, the philanthropic dollar is a powerful thing, and think of the results if the ATA finds a genuine signal! Cornell astronomer and science popularizer Carl Sagan left quite a legacy in a number of science fields, including and especially those which were considered to be somewhat fringe at one time. One prime example of his support of a science field that was not universally accepted in earlier eras was SETI, the Search for Extraterrestrial Intelligence. At a time when many astronomers did not seriously consider the possibility of other beings existing...
Voyager’s Latest, and Hopes for Europa
When the last Voyager pictures from Neptune (and perhaps even more eagerly awaited, the images of Triton) came in back in 1989, I distinctly recall the sense of letdown that set in the following week. All those spectacular Voyager findings were, I then assumed, a thing of the past. But as we've seen, the Voyagers are robust little spacecraft, pushing on toward the heliospause and the edge of interstellar space. Still functional, one or both may be sending us signals when they make this final transition within the next ten to twenty years. Which is not to say we don't need follow-up missions to explore this territory (Innovative Interstellar Explorer, using radioisotope methods to power an ion engine, immediately comes to mind), but what a grand story the Voyagers continue to write. And consider this finding: Because the two spacecraft took entirely different routes, Voyager 2 is crossing the termination shock region some 20 billion kilometers away from Voyager 1's present location....
Out Among the Dark Stars
You would think that a star anywhere from 400 to 200,000 times wider than the Sun would be fairly easy to detect. But not if it's a 'dark star,' the name for a new, theoretical entity about to make its appearance in Physical Review Letters. Astrophysicist Paolo Gondolo (University of Utah) makes the case that dark matter would have affected the temperature and density of the gases that formed the first stars. Dark stars would mostly contain normal matter -- hydrogen and helium -- but they would have been much larger than the Sun, glowing largely in the infrared. So how would the early universe have produced a dark star? Gondolo looks at neutralinos, one type of the weakly interactive massive particles (WIMPS) that may explain dark matter. Calculating how dark matter would have affected the earliest stars, the team's findings suggest that dark matter neutralinos would have annihilated each other, producing quarks and anti-quarks. A proto-stellar cloud trying to shrink into a star...
Of Young Stars and Ancient Planets
Since we've just been looking at young stars -- protostars, at that -- the news from Ann Arbor seems timely. Astronomers at the University of Michigan are announcing systems around UX Tau A and Lk Ca 15, young stars each, located about 450 light years away in the Taurus star formation region. What they're actually observing at infrared wavelengths are gaps in the protoplanetary disks around these stars, the assumed result of planets sweeping the area clear of debris. Unlike the infant star-in-the-making we looked at yesterday, UX Tau A and Lk Ca 15 are old enough -- about a million years each -- for planetary formation. Both are still pre-main sequence, deriving their energy from gravitational contraction instead of hydrogen-to-helium burning. To reach any conclusion about what's happening around them, the Michigan team has to rule out photoevaporation, which is what happens when the dust and gas of a protoplanetary cloud heats up, evaporates and begins to dissipate. Catherine...