The Last Cry Of MatterNovember 27, 2003'Black holes' are truly black. When an object gets within a certain distance from a black hole, it will get swallowed forever with no chance to escape. That includes light, which means that black holes do not shine. How do astronomers detect black holes if they are unable to see them? Well, to be precise, astronomers do not detect black holes. But they do detect the phenomena that can only be explained by the existence nearby of objects that match the description of black holes! The strong gravitational attraction of a black hole affects the motion of nearby objects. When astronomers see a star circling around something, but they cannot see what that something is, they may suspect it is a black hole, or a neutron star - the ultra-dense 'corpse' of a star. Astronomers can even infer the mass of a black hole by measuring the mass of the star and its speed. The same kind of calculation can be done whith supermassive black holes that lurk at the centre of many galaxies, including our own galaxy, the Milky Way. In the Milky Way, observations have revealed the existence of stars and gas moving very fast near the centre, a behaviour that can only be explained if a mass of several million times that of the Sun is at the centre of the galaxy. Such mass has to be concentrated within a radius of only 10 light-days - roughly 40 times times the distance from the Sun to Pluto - and is most likely to be a black hole. In fact, at the very centre of our galaxy, radio and X-ray telescopes have detected a powerful source called 'Sagittarius A', identified as the candidate to be this massive black hole. This idea has recently received strong support, with the measurement for the first time of the orbit of a star that approaches this mysterious object to within 17 light-hours - only three times the distance between the Sun and Pluto - while travelling at speeds of than 5000 kilometres per second! Shining to death Another piece of evidence in favour of the idea of supermassive black holes in the centre of galaxies is the existence of quasars, discovered in 1967. Quasars are very distant and very luminous at the same time - the most luminous objects in the Universe. To explain the incredible amount of energy they must release, astronomers also need black holes: just before disappearing into a black hole, the matter being swallowed heats up and emits great amounts of energy - its 'last cry'. So quasars are believed to be caused by black holes with masses of one million to several billion times the mass of the Sun. The 'last cry' of matter about to be swallowed is best detected with x-ray and gamma-ray telescopes, because the energy released is given off in the form of hard x-rays. In fact, ESA's orbiting observatories XMM-Newton and Integral have already shown their skills in studying black holes in several discoveries. For example, XMM Newton has recently discovered a small black hole whirling in our galaxy, in the Ara constellation of the southern sky. Integral has detected what could be the first significant hard x-ray emission from the black hole in the centre of our galaxy. European Space Agency (ESA) |
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| Related Black Hole Current Events and Black Hole News Articles Swift XMM-Newton Satellites Tune Into a Middleweight Black Hole While astronomers have studied lightweight and heavyweight black holes for decades, the evidence for black holes with intermediate masses has been much harder to come by. New vista of Milky Way center unveiled A dramatic new vista of the center of the Milky Way galaxy from NASA's Chandra X-ray Observatory exposes new levels of the complexity and intrigue in the Galactic center. Invading black holes explain cosmic flashes Black holes are invading stars, providing a radical explanation to bright flashes in the universe that are one of the biggest mysteries in astronomy today. Sophisticated telescope camera debuts with peek at nest of black holes Less than two months after they inaugurated the world's largest telescope, University of Florida astronomers have used one of the world's most advanced telescopic instruments to gather images of the heavens. NGC 4945: The Milky Way's not-so-distant Cousin ESO has released a striking new image of a nearby galaxy that many astronomers think closely resembles our own Milky Way. First Black Holes Born Starving The first black holes in the universe had dramatic effects on their surroundings despite the fact that they were small and grew very slowly, according to recent supercomputer simulations carried out by astrophysicists Marcelo Alvarez and Tom Abel of the Kavli Institute for Particle Astrophysics and Cosmology, jointly located at the Department of Energy's SLAC National Accelerator Laboratory and Stanford University, and John Wise, formerly of KIPAC and now of NASA Goddard Space Flight Center. First black holes kept to a strict diet, study shows A new supercomputer simulation designed to track the fate of the universe's first black holes finds that, counter to expectations, they couldn't efficiently gorge themselves on nearby gas. Goddard-Led GEMS Mission to Explore the Polarized Universe An exciting new astrophysics mission led by NASA's Goddard Space Flight Center in Greenbelt, Md., will provide a revolutionary window into the universe. Named the Gravity and Extreme Magnetism Small Explorer (GEMS), the satellite will be the first to systematically measure the polarization of cosmic X-ray sources. Turbulence responsible for black holes' balancing act We live in a hierarchical Universe where small structures join into larger ones. Earth is a planet in our Solar System, the Solar System resides in the Milky Way Galaxy, and galaxies combine into groups and clusters. NASA's Fermi Finds Gamma-ray Galaxy Surprises Back in June 1991, just before the launch of NASA's Compton Gamma-Ray Observatory, astronomers knew of gamma rays from exactly one galaxy beyond our own. More Black Hole Current Events and Black Hole News Articles |
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