By now, our outer Solar System probes have brought us so many surprises that finding yet another one should be passé. But it never is, and imagine the wonders we'll find, for example, when New Horizons arrives at Pluto/Charon and moves on to the Kuiper Belt beyond. Now Cassini has once again made news with the discovery of what may be described as an 'ice volcano.' The beauty of the concept is that it may explain the presence of atmospheric methane on Titan. "Before Cassini-Huygens, the most widely accepted explanation for the presence of methane in Titan's atmosphere was the presence of a methane-rich hydrocarbon ocean," said Dr. Christophe Sotin, distinguished visiting scientist at NASA's Jet Propulsion Laboratory, Pasadena, Calif. That otherworldly ocean was the most exotic of constructs, creating images of the Huygens lander bobbing about amidst frigid swells as its batteries failed. What the probe parachuted into was quite different. In a way, it's a shame to lose the...
Supernova Remnants and Star Formation
Apropos to our earlier discussion about shielding an interstellar probe comes this new image from the Hubble Space Telescope (click to enlarge). This chaotic and expanding mass of gas and dust, known as LMC N 63A, is the result of the explosion of a massive star. It's found in the N 63 region of the Large Magellanic Cloud, an irregular galaxy 160,000 light years from the Milky Way that is visible in the southern hemisphere. Numerous studies have been made of star formation and supernova remnants in this region. Imagine the shielding requirements that would be needed to penetrate such a active patch of sky! Fortunately, the interstellar medium is rarely so dense, but images like these remind us that space is anything but empty. Instead, it houses to a greater or lesser extent gas and dust particles that have to be reckoned with. We've also looked recently at the growing evidence that Voyager 1 is at the edge of the heliosphere, that 'bubble' of relatively clear space blown by the...
Astrodynamics at Princeton
Ed Belbruno did a terrific job putting together the New Trends in Astrodynamics and Applications II conference, from which I returned yesterday. I chose to drive to Princeton because of my growing aversion to airline travel. It was a long but generally uneventful drive except for the usual delays around Washington DC -- over an hour to clear the Beltway because of construction on one of the access ramps. But driving through western New Jersey is, as anyone who has done it knows, a pleasant experience, beautiful farmlands giving way to small villages here and there, with Princeton itself an oasis of lovely architecture, fine restaurants and, of course, a great university. About the only thing that didn't cooperate was the weather -- we had a chill rain for the first two days -- but Peyton Hall is about half a mile from the Nassau Inn, Princeton's fine colonial-era hostelry, and it was an energizing walk even with umbrella. The conference sessions were intense; we generally ran from...
Getting Ready for Deep Impact
Deep Impact's arrival at Comet Tempel 1 should be spectacular. Due to reach the comet on July 4 of this year, the two-part probe will launch a 360 kg impactor designed to produce a crater on the comet's nucleus and a plume of gas and dust. Getting inside a comet is a key mission goal: the ejected material should tell us much about the early days of the Solar System. Right now astronomers are engaged in making baseline observations through Earth-based telescopes to characterize Tempel 1 as completely as possible. By examining its albedo (reflectivity), rotation period and size, the mission team will be able to differentiate between impact effects and the natural activity of the comet during the Deep Impact encounter. The photograph on the right (click to enlarge) shows an image of Tempel 1 together with a number of visual artifacts. What has happened here is that images were taken through various filters, one after the other. The motion of the comet against background objects accounts...
New Trends in Astrodynamics
Centauri Dreams will be in Princeton over the weekend for the New Trends in Astrodynamics conference (Web site here). Topics are to range from upcoming missions to low-energy trajectories (a specialty of conference organizer Edward Belbruno) and near-Earth object impact projections. Among the papers targeting advanced propulsion technologies: Gregory Matloff, "Phobos/Diemos Sample Return via Solar Sail" Marc Millis, "Assessing Potential Propulsion Breakthroughs" Edgar Choueiri, "Advanced Propulsion Concepts for High-Energy Space Exploration Missions" I will be presenting "The Interstellar Conundrum: A Survey of Concepts and Proposed Solutions." And it will be wonderful to have the chance to talk to two Italian theorists, Giancarlo Genta (Politecnico di Torino) and Claudio Maccone (Alenia Spazio), whose work I have long admired. It should be a rich and full weekend, busy enough to require a brief suspension of postings here. Centauri Dreams will resume its normal publication schedule...
Inside the Carina Nebula
Panoramas this stunning deserve a lingering look (and be sure to click the image for a higher resolution view). You're looking at more of the fruits of the Spitzer Space Telescope's remarkable labors, this time a false-color image showing a part of the star-forming region known as the Carina Nebula. Using infrared, Spitzer was able to penetrate the so-called 'South Pillar' region of the nebula to reveal yellow and white stars in their infancy, wrapped up inside pillars of thick pink dust. The hottest gases here are green; the foreground stars are blue, which shows up better in the enlargement. And note the bright area at the top of the frame, which is what this story is all about. The glow is caused by the massive star Eta Carinae, which is too bright to be observed by infrared telescopes. Stellar winds and ultraviolet radiation from this star are what have torn the gas cloud, leaving the tendrils and pillars visible here. It is this 'shredding' process that triggers the birth of the...