Comet Tempel 1, the target of NASA's Deep Impact probe back in July, has offered scientists a stunning view of cometary topography. The first published results from the mission team will appear in the September 9 issue of Science and have been released at the Division of Planetary Sciences meeting at Cambridge. Among other things, Tempel 1 is the first comet to demonstrate impact craters, an indication of collisions with various space debris over the aeons. The craters range from 40 to 400 meters across, but are they common to all comets? Those we've had good views of, including Borelly and Wild 2, show significant differences in topography and shape. Of Tempel 1, we can only say that its lifetime has been complex. "This comet is a geologic wonder," said Peter Schultz, a professor of geological sciences at Brown University and a co-investigator on the mission team. "There are smooth surfaces, filled-in craters, ridges, cliffs. Tempel 1 also features an area marked by innumerable...
Enceladus and the Hunt for Life
Saturn's moon Enceladus is back in the news at the Division of Planetary Sciences meeting at Cambridge University this week. Not that it has ever quite left the spotlight since 1981; that's when Voyager 2 photographs told scientists that parts of the moon had been geologically active as recently as 100 million years ago. The moon's smooth terrain was hard to explain -- how does an object 314 miles across get hot enough to melt? Then Cassini came and Enceladus' wonders increased. We now know that the moon has an atmosphere of water vapor, nitrogen, carbon dioxide and other organic (i.e., carbon-based) molecules concentrated at its south pole. Moreover, that polar region is hotter than expected, -183 degrees Celsius vs. -203 Celsius as predicted by the models, and is marked by 80-mile long parallel cracks that vent vapor and ice particles. Some of this material may have crystallized on the surface as recently as the past decade. At the Cambridge meeting, Robert H. Brown (University of...
Hubble Makes ‘Movie’ of Neptune’s Atmosphere
The Hubble Space telescope used 14 different color filters to dig out the details of different layers in Neptune's atmosphere, showing the haze and clouds in considerable detail, and producing a time-lapse movie that has now been released on the Internet. In the image below (click to enlarge), a natural color view of Neptune appears on the left; the familiar blue-green of the atmosphere is the result of absorption by methane of the red wavelengths striking the planet. At upper right is an enhanced color view. But now check the view at bottom right, taken using methane filters that bring out details above the bulk of the atmospheric methane. At these wavelengths, the planet appears much darker and the long exposure times this permits help to reveal some of Neptune's smaller moons. You can see these in the natural color image, which is a composite of images in green, red and blue light. Clockwise from the top, Proteus is the brightest moon; the others are Larissa, Despina and Galatea....
Fast Neutron Star Leaving the Galaxy
What would give a neutron star the kind of push that would send it out of the galaxy at over 1000 kilometers per second? Nobody knows, but data from the Very Long Baseline Array, a system of radio telescopes spanning 5,000 miles with locations from Hawaii to the US Virgin Islands, have revealed just such an object, and have allowed astronomers to measure its motion with unprecendented accuracy. "This is the first direct measurement of a neutron star's speed that exceeds 1,000 kilometers per second," said Walter Brisken, a National Radio Astronomy Observatory astronomer. "Most earlier estimates of neutron-star speeds depended on educated guesses about their distances. With this one, we have a precise, direct measurement of the distance, so we can measure the speed directly," Brisken said. The star's speed translates to 670 miles per second, numbingly fast, but even at these speeds, an object like this would still take 1200 years to cross the 4.3 light years that separates us from the...
An Infrared Hunt for Artificial Kuiper Belt Objects
If extraterrestrials were to set up a colony in our Solar System, where would they choose to settle? Gregory Matloff and Anthony R. Martin make the case for the Kuiper Belt in a recent paper for the Journal of the British Interplanetary Society. Kuiper Belt Objects (KBOs) are, after all, easy to exploit as a resource base without the burden of a planet's gravity well. They are rich in volatile materials (more so than main belt asteroids), close enough to the Sun to harvest solar power, and far enough out that visits by those of us living in the inner Solar System would be few and far between. Moreover, the orbits of KBOs are relatively unaffected by planetary perturbations. Matloff was intrigued enough by these factors to make a proposed infrared search of the Kuiper Belt the subject of a 2004 paper ("A Proposed Infrared Search for Artificial Kuiper Belt Objects," JBIS 57, pp. 283-287). His new paper follows this up with an examination of the characteristics that artificial KBOs...