Dr. Charles Ippolito January 4, 2010
Massive Black Hole Implicated in Stellar Destruction
link: http://www.sciencedaily.com/releases/2010/01/100104120148.htm
Scientists from NASA's Chandra X-ray Observatory believe that a star has recently been destroyed by a big black hole. The scientists suggest that this black hole is much more massive than the Sun. Supposedly a thousand times as massive. These Chandra observations showed a source of X-rays in a cluster of stars and mysterious elements which were in the emissions of X-rays. It is believed that these X-rays are part of the "ultralimonous X-ray source" or ULX category. This would mean that the ULX is more luminant than any stellar X-ray source but its less luminous than the bright X-ray sources that have to do with massive black holes. However the nature of the ultralimonous X-ray sources is still a mystery. The ULX source that was believed to be seen was in a cluster of old stars. Jimmy Irwin of the University of Alabama led the study. Him and his colleagues were able to pick up an optical spectra of the cluster using Magellan 1 and 2 telescopes in Las Campanas, Chile. The data showed emission from gas that had oxygen and nitrogen but not hydrogen. They believe that the gas is orbiting a black hole that has at least 1000 solar masses. Irwin concluded that the destroyed star was a white dwarf.
This article is important for kids who are studying astronomy and chemistry, It teaches about line spectras and how they can be used to identify gases when they are obtained. This current events article is important to me because I had no idea that X-rays, which contain large amounts of energy, could be found in clusters of stars.
I didnt enjoy this article too much. Although it did teach me more about astronomy. When I first came across it it seemed interesting, but I didn't find it very attention grabbing while I was reading it. It isn't the type of article that I would enjoy reading.
NASA/Marshall Space Flight Center. "Massive Black Hole Implicated in Stellar Destruction." ScienceDaily 4 January 2010. 4 January 2010