Dolores Beasley/Don Savage
Headquarters, Washington, DC January 11, 2001
(Phone: 202/358-1547)

Megan Watzke
Chandra X-ray Observatory, Cambridge, MA
(Phone: 617/496-7998)

Ray Villard
Space Telescope Science Institute, Baltimore, MD
(Phone: 410/338-4514)

RELEASE: 01-04

NOT SEEING IS BELIEVING WHEN IT COMES TO EVENT HORIZON EVIDENCE

NASA's two Great Observatories, the Hubble Space Telescope and the Chandra X-ray Observatory, have independently provided what could be the best direct evidence yet for the existence of an event horizon, the defining feature of a black hole and one of the most bizarre astrophysical concepts in nature.

An event horizon is the theorized "one-way ticket" boundary around a black hole from which nothing, not even light, can escape. No object except for a black hole can have an event horizon, so evidence for its existence offers resounding proof of black holes in space.

By using data from Chandra and previous X-ray satellites, a team of researchers studied a dozen "X-ray novae," systems that contain a Sun-like star that orbits either a black hole or
neutron star. By comparing the energy output from X-ray novae in their inactive, or dormant, phase, the Chandra team determined the black hole candidates emitted only one percent as much energy as neutron stars.

"It's a bit odd to say we've discovered something by seeing almost nothing, but, in essence, this is what we have done" said Michael Garcia of the Harvard-Smithsonian Center for Astrophysics, Cambridge, MA. "By detecting very little energy
from these black hole candidates, we have new proof that event horizons exist."

If a collapsed star is a neutron star with a solid surface, energy must be released when infalling material strikes that surface. In contrast, if the accreting object is a black hole, only a small amount of energy can escape before it crosses the event horizon and vanishes forever.

"Seeing just this tiny amount of energy escape from the black hole sources is like sitting upstream watching water seemingly
disappear over the edge," said Ramesh Narayan also of the Chandra team. "The most straightforward explanation for our
observations is that these objects have event horizons and, therefore, are black holes."

Scientists using the Hubble Space Telescope took an entirely different approach. Joseph F. Dolan, of NASA's Goddard Space Flight Center, 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.

Hubble, measuring fluctuations in ultraviolet light from gas trapped in orbit and around the black hole found two examples of a so-called "dying pulse train," the rapidly decaying,
precisely sequential lashes of light from a hot blob of gas spiraling into the black hole. Without an event horizon, the blob of gas would have brightened as it crashed onto the
surface of the accreting body. One event had six decaying pulses; the other had seven pulses. The results are consistent with what astronomers would expect to see if matter were really
falling into a black hole, Dolan said.

Chandra researchers used the Advanced CCD Imaging Sectrometer for exposure times that vary roughly from 10,000 to 40,000 seconds per object. Hubble's high-speed photometer sampled light at the rate of 100,000 measurements per second, during three separate Hubble orbits, executed in June, July and August of 1992.

The Space Telescope Science Institute is operated by the Association of Universities for Research in Astronomy, Inc., for NASA under contract with Goddard Space Flight Center. The Hubble Space Telescope is a cooperative project between NASA
and the European Space Agency.

NASA's Marshall Space Flight Center, Huntsville, AL manages the Chandra program. The Smithsonian's Chandra X-ray Center controls science and flight operations from Cambridge, MA. The Chandra work was also supported by funds from the National Science Foundation.

Images associated with the release are available at:

http://oposite.stsci.edu/pubinfo/pr/2001/03

http://chandra.harvard.edu
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