It may be that the center of the galaxy is the least likely place to find an extraterrestrial civilization. New findings reported in Astrophysical Journal Letters indicate the galactic core undergoes periodic eras of star formation that are caused by inflowing gas from a band of material about 500 light years away from the center. The result: massive -- and (on an astronomical scale) frequent -- explosions that would spew deadly radiation at any planets to be found there. The team, led by astronomer Antony Stark of the Harvard-Smithsonian Center for Astrophysics, discovered that tidal forces and interactions with nearby stellar material cause the ring of gas to build until it reaches a critical point, at which time it collapses into the galactic center and fuels a burst of star formation. Stark believes the next starburst in the Milky Way will occur within 10 million years; life on any planets nearby would be snuffed out quickly. The Earth, at 25,000 light years from the core, is...
The View from Antarctica
A team of Australian researchers has built an unmanned observatory high on an Antarctic plateau that may provide images nearly the equal of Hubble's. That's the word from Nature, where University of New South Wales associate professor Michael Ashley, co-author of the paper, described the capabilities of the new viewing site. The paper's lead author is Dr. Jon S. Lawrence, a postdoctoral fellow at the University of New South Wales. The location is known as Dome C, 3250 meters above sea level on the Antarctic Plateau, at latitude 75 degrees south. Among its favorable characteristics are low infrared sky emission, dry and extremely cold air, few clouds and low dust and aerosol content. The upshot: much less 'star jitter.' All of these factors make the site, which is 400 meters higher than the South Pole, far better for viewing than the location of instruments currently in place in Chile, Hawaii and the Canary Islands. Having established the superiority of Dome C, the team now argues for...
Something Exquisite for the Weekend
NGC 6543 is called the Cat's Eye Nebula; it was one of the first planetary nebulae to be discovered. This gorgeous view from Hubble shows that it is also one of the most complex nebulae ever studied. You're looking at a Sun-like star at the very end of its life, losing its outer gaseous layers to create concentric clouds in ways that are still mysterious. Each bright ring is actually the edge of a spherical bubble of gas. Hubble used its Advanced Camera for Surveys (ACS) to make this image.
Brighter Than 200 Million Suns
It looks bright enough to be a foreground star, but this supernova, called SN 2004dj, is 11 million light years away in a galaxy known as NGC 2403. Not particularly germane to interstellar propulsion or finding candidates for robotic probes, but simply too remarkable a sight to ignore. You can read more about this Hubble photograph here. From the press release issued by the Space Telescope Science Institute: The heart of NGC 2403 is the glowing region at lower left. Sprinkled across the region are pink areas of star birth. The myriad of faint stars visible in the Hubble image belong to NGC 2403, but the handful of very bright stars in the image belong to our own Milky Way Galaxy and are only a few hundred to a few thousand light-years away. This image was taken on Aug. 17, two weeks after an amateur astronomer discovered the supernova. What we're seeing here is the creation of heavy chemical elements like calcium, iron and gold, all of which, on Earth and elsewhere, came from...
European Space Agency to Create Catalog of Stars
Although ESA has cancelled its Eddington mission, which was to have used a precision photometer to record the transit of planets across the disks of distant stars, the agency is pressing ahead with a mission that will compile a catalog of up to a billion stars. As described in the ESA press release, the Gaia mission would be launched in 2010, and would spend almost a decade plotting these stars into a three-dimensional grid that would show not just their current position, but direction of motion, color and composition. It always startles me how little we know about even nearby stars. It was only last year that the red dwarf SO25300.5+165258 was discovered, but at 7.8 light years away, it is the third closest star to the Sun. Projects like Gaia will be invaluable at filling in our information about other close stars that have so far evaded detection, many of them simply because of their size and dimness -- some 70 percent of all stars in the galaxy are type M red dwarfs like Proxima...
Hubble and the Solar Wind
The Hubble Space Telescope has given us no end of gorgeous astronomical photographs. This one is of an enormous cavity of gas carved out by the stellar wind from the nebula N44f; the image comes from the ESA/Hubble Information Centre. You're looking at what happens when a cloud of gas is inflated by fast-moving particles from a hot young star. This stellar wind is moving at about 7 million kilometers per hour, far faster than the Sun's (a sedate 1.5 million kilometers per hour). Keep this image in mind when thinking about new propulsion concepts like Robert Winglee's M2P2, which uses the solar wind to push a magnetic sail. You can read about Winglee's work at this Web site at the University of Washington. And note that when we talk about the solar wind pushing a magnetic sail, we are discussing something different than a solar sail, which gets its push solely from the momentum imparted by photons. They are two entirely different concepts.