Hubble finally may have proof black holes do exist
SPACE TELESCOPE SCIENCE INSTITUTE RELEASE
Posted: January 11, 2001
NASA's Hubble Space Telescope may have, for the first time, provided direct evidence for the existence of black holes by observing the disappearance of matter as it falls beyond the "event horizon."
Joseph F. Dolan, of NASA's Goddard Space Flight Center in Greenbelt, MD, observed pulses of ultraviolet light from clumps of hot gas fade and then disappear as they swirled around a massive, compact object called Cygnus XR-1. This activity is just as would have been expected if the hot gas had fallen into a black hole.
An event horizon is the mysterious region surrounding a black hole that forever traps light and matter straying nearby. By definition, no astronomical object other than a black hole can possess an event horizon.
Black holes have been inferred by observing the furious whirlpool motion of trapped gas and estimating how much mass is crammed into the tiny region of space the black hole occupies.
Also, previous X-ray observations have offered evidence for an event horizon by surveying black hole candidates that seem to be swallowing nearly a hundred times as much energy as they radiate. Those results imply that trillion-degree gas is falling over the brink of an event horizon, like water over the edge of a waterfall.
But no one has ever seen what actually happens to a piece of matter swirling into the event horizon, like water down a drain. The secret was tucked away in nearly decade-old Hubble data that took meticulous analysis.
Dolan cautions that his Hubble black hole observations see only two infall events. This means there is a finite chance the signature could simply be a statistical fluke that mimics the behavior of matter near a black hole. But Dolan emphasizes the results are consistent with what astronomers would expect to see if matter were really falling into a black hole.
The discovery comes from a detailed statistical analysis of a 1992 observation of one of the first black holes ever discovered, Cygnus XR-1, which lies 6,000 light-years from Earth in the summer constellation Cygnus the Swan.
This signature matches theories of what scientists would predict to see when matter is falling so close to the event horizon that its light rapidly dims as it is stretched by gravity to ever-longer wavelengths. Without an event horizon, the blob of gas would have brightened as it crashed onto the surface of the accreting body. Instead, the gas crossed over into a twilight-zone realm when time and space no longer have any practical meaning. Because of the gravitational stretching of light (an effect called redshift), the fragment disappeared from Hubble's view before it ever actually reached the event horizon. The pulsation of the blob - an effect caused by the black hole's intense gravity -- also shortened as it fell closer to the event horizon.
Finding the signature wasn't an easy task. Hubble's high-speed photometer (a very fast light meter) sampled light at the rate of 100,000 measurements per second, during three separate Hubble orbits, each executed in June, July, and August of 1992. The observation yielded 1 billion data-points, which, if printed out on a chart recorder, would stretch 600 miles! Hubble's ultraviolet capability gave it the ability to see the faint flicker of material within 1,000 miles of the event horizon.
Dolan "mined" the enormous database on and off for years. "Looking for the decaying pulse train was like looking for the proverbial needle-in-a haystack," he says. "Put another way, it was like listening for a specific word in a many hours-long transmission of Morse code."
He found two examples of infall events. One event had six decaying pulses; the other had seven pulses. The pulses spanned an interval of merely 0.2 seconds before the blob forever disappeared from view.