Imagine two neutron stars colliding, or even worse, a neutron star and a black hole. The release of energy would be catastrophic, and has apparently now led to the first detection in visible light from a short gamma-ray burst. Thus we're beginning to get a handle on the most powerful explosions in the known universe, whose identity has bedeviled astronomers for thirty years. There are actually two different kinds of gamma-ray bursts. The longer ones have been linked to the explosion of a massive star as it collapses into a black hole. It's the short-duration bursts that have proven the greater challenge. The new work, performed at La Silla (Chile) and at the European Southern Observatory's Very Large Telescope, used data from NASA's HETE-2 satellite to guide the observations, and the fading source was found. "That was the clue we were waiting for," said Garrett Jernigan, a research physicist at the Berkeley Space Sciences Laboratory. "Bursts seem to come mainly in two varieties - the...
1991 VG: Natural or Artificial?
The search for extraterrestrial intelligence (SETI) has seen a great deal of publicity, from television programs interviewing involved scientists to blockbuster movies like Contact. But the idea that there might be signs of extraterrestrial life closer to home has received relatively short shrift. Nonetheless, SETA (the search for extraterrestrial artifacts) has spawned interesting work, from Gregory Matloff's examinations of anomalous Kuiper Belt objects to Robert Freitas' surveys of 'halo orbits' around the Lagrangian points. So far both kinds of search -- SETI and SETA -- have come up short, but a few curious things have been observed on each side. One interesting SETA investigation involved an object called 1991 VG, which made a close approach to Earth in 1991 (thanks to Adam Crowl for bringing this one to my attention). Discovered by Jim Scotti using the University of Arizona's Spacewatch telescope (normally used to detect small asteroids near the Earth), 1991 VG seemed to be...
A Correction on Adaptive Optics
The sharp-eyed Jon Lomberg writes with a correction to today's story on Xena and its moon Gabrielle. Specifically, my statement that adaptive optics 'bounces' the light of a laser off the atmosphere to create an artificial star used in refining the telescope's images. Lomberg rightly points out that what the laser actually does is to excite sodium atoms at a specific height. The glow from this excitation is then tracked and used to adjust for atmospheric distortion. The results, as we have seen, are nothing short of spectacular. What's ahead for adaptive optics? "A future improvement of the technique," writes Lomberg, "would use different lasers to excite other elements at other altitudes, thus giving a more detailed profile of distortion in the atmosphere resulting in more precise adjustments."
A Moon for Xena
Everyone is calling 2003 UB313, the Solar System's 10th planet, Xena. The name comes from a TV warrior princess of whom the curmudgeonly Centauri Dreams, never one for television, was utterly unaware. Now Xena has been found to have a moon, inevitably named Gabrielle after an equally incrutable character on the series (apparently the sidekick of Xena herself). One-tenth the size of Xena, Gabrielle is slated for further observations with the Hubble Space Telescope that will allow more accurate determination of its mass. The advent of Gabrielle is good news for those wishing to learn more about Xena. From a California Institute of Technology press release quoting Michael Brown, the 10th planet's discoverer: "A combination of the distance of the moon from the planet and the speed it goes around the planet tells you very precisely what the mass of the planet is," explains Brown. "If the planet is very massive, the moon will go around very fast; if it is less massive, the moon will travel...