Slide 1Slide 2Slide 3Slide 4Slide 5Slide 6Slide 7Black Hole in the Center of the GalaxyCompelling EvidenceBlack Hole in the Center of the GalaxyCompelling EvidenceNASA's COBE satellite scanned the heavens at infrared wavelengths in 1990 and produced this premier view of the central region of our own Milky Way Galaxy. The Milky Way is a typical spiral galaxy with a central bulge and extended disk of stars. However, gas and dust within the disk obscure visible wavelengths of light effectively preventing clear observations of the center. Since infrared wavelengths, are less affected by the obscuring material, the Diffuse InfraRed Background Experiment (DIRBE) on board COBE was able to detected infrared light from stars surrounding the galactic center and produce this image. Of course, the edge on perspective represents the view from the vicinity of our Sun, a star located in the disk about 30,000 light years out from the center. The DIRBE experiment used equipment cooled by a tub of liquid helium to detect the infrared light which, composed of wavelengths longer than red light, is invisible to the human eye.Black Hole in the Center of the GalaxyCompelling EvidenceSource: National Science Foundation Date: 1998-09-08 'Supermassive' Black Hole Found In The Center Of Our GalaxyThe presence of an enormous black hole at the center of our galaxy has been detected by a researcher funded, in part, by the National Science Foundation (NSF). The evidence is being reported this week at the Central Parsecs Galactic Center Workshop '98 in Tucson, Arizona, by Andrea Ghez, of the University of California-Los Angeles.Black Hole in the Center of the GalaxyCompelling Evidence"What lies in the center of the Milky Way has been one of this century's 'big' science questions," said Terry Oswalt, NSF program manager for Stellar Astronomy and Astrophysics. "Ghez's work has massive implications on our understanding of how galaxies evolve." Black holes are formed from the remnants of collapsed stars. A black hole consists of a large mass compacted so densely that not even light can escape its force of gravity. Since Ghez could not directly see a black hole, she inferred its presence by searching for the gravitational influence it imposes on nearby objects she could see, namely stars.Black Hole in the Center of the GalaxyCompelling EvidenceIn 1995, using the Keck I Telescope atop Mauna Kea in Hawaii, Ghez began tracking the movement of 200 stars near the galactic center. She found at least 20 stars that exhibited the telling signs of influence by extreme gravitational forces.Black Hole in the Center of the GalaxyCompelling EvidenceThese stars are spiraling around the black hole at speeds of up to three million miles per hour-about 10 times the speed at which stars typically move. In order to account for the rapid speeds of these stars, Ghez determined that an object 2.6 million times more massive than our Sun must be concentrated into a single black hole. Just getting a clear view of the center of our galaxy is an impressive feat in itself. To overcome the distortion created by the Earth's atmosphere, Ghez made her observations using a technique called "infrared speckle interferometry." The procedure, which she helped develop, uses computers to analyze thousands of high-speed, high-resolution snapshots. The result: an image that has at least 20 times better resolution than those made by traditional earthbound imaging techniques. "It's like putting on glasses," said Ghez.Black Hole in the Center of the GalaxyCompelling EvidenceUsing this technique in 1995, Ghez witnessed the disappearance of a star that was, at the time, the closest object to the black hole. Whether the star was sucked into the black hole, or simply went behind it, scientists may never
View Full Document
Unlocking...