02-24-2005, 03:41 PM
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#52 (permalink)
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Apocalypse Nerd
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And GH our bastard love child has been spotted by Nasa Scientists:
http://www.hypography.com/article.cfm?id=32546
Quote:
Hubble Astronomers Feast on Interstellar Hamburger
Aug 2 2002 @ 09:15 by NASA/JPL
Hold the pickles; hold the lettuce. Space is serving up giant hamburgers.
NASA's Hubble Space Telescope has snapped a photograph of a strange object that bears an uncanny resemblance to a hamburger. The object, nicknamed Gomez's Hamburger, is a Sun-like star nearing the end of its life. It already has expelled large amounts of gas and dust and is on its way to becoming acolorful, glowing planetary nebula.
The ingredients for the giant celestial hamburger are dust and light. The hamburger buns are light reflecting off dust, and the patty is the dark band of dust in the middle. The Hubble Heritage image was taken Feb. 22, 2002, with the Wide Field and Planetary Camera 2, designed and built by NASA's Jet Propulsion Laboratory, Pasadena, Calif.
The image shows the structure of Gomez's Hamburger with high resolution, particularly the striking dark band of dust that cuts across the middle. The dark band is actually the shadow of a thick disk around the central star, which is seen edge-on from Earth. The star itself, with a surface temperature of approximately 10,000 degrees Celsius (18,000 degrees Fahrenheit), is hidden within this disk. However, light from the star does emerge in the directions perpendicular to the disk and illuminates dust above and below it.
The reason why the star is surrounded by a thick, dusty disk remains somewhat uncertain. It is possible that the central object is actually a pair of stars. If so, then the star that ejected the nebula may be rapidly rotating, expelling material mostly from its equatorial regions.
Stars with masses similar to our Sun's end their lives as planetary nebulae. The star evolves to become a bloated red giant, with a girth about 100 times greater than its original diameter. Then it ejects its outer layers into space, exposing the star's hot core. Ultraviolet radiation from the central core streams out into the surrounding ejected gas, causing it to glow. The glowing gas is called a planetary nebula. The Hubble Space Telescope has provided numerous spectacular images of planetary nebulae over the past several years.
Less well-known are "proto-planetary nebulae," objects like Gomez's Hamburger that are in a state of evolution immediately before the true planetary-nebula stage. Just after the red giant expels its outer layers, the remnant star in the center is still relatively cool. Consequently, it emits ordinary visible light, but not yet any ultraviolet radiation. Therefore the surrounding gas does not glow.
However, the ejected material also contains vast numbers of microscopic dust particles, which can reflect the starlight and make the material visible. This same effect of "light scattering" produces halos around streetlights on a foggy night.
The lifetime of a proto-planetary nebula is very brief. In less than a thousand years, astronomers expect that the central star will become hot enough to make the dust particles evaporate, thus exposing the star to view. At that time the surrounding gas will glow. Gomez's Hamburger will have become a beautiful, glowing planetary nebula.
Gomez's Hamburger was discovered on sky photographs obtained by Arturo Gomez, an astronomer at the Cerro Tololo Inter-American Observatory in Chile. The photos suggested that there was a dark band across the object, but its exact structure was difficult to determine because of the atmospheric turbulence that
hampers all images taken from the ground.
The Space Telescope Science Institute is operated by the Association of Universities for Research in Astronomy, Inc., for NASA, under contract with the Goddard Space Flight Center, Greenbelt, Md. The Hubble Space Telescope is a project of international cooperation between NASA and the European Space Agency. The California Institute of Technology, Pasadena manages JPL for NASA.
Image Credit: NASA and the Hubble Heritage Team (STScI/AURA)
Acknowledgment: A. Gomez (Cerro Tololo Inter-American Observatory)
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