Press Release

Not seeing is believing when it comes to event horizon evidence

By SpaceRef Editor
January 11, 2001
Filed under ,

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, Mass. “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 Spectrometer 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, Ala., manages the
Chandra program. The Smithsonian’s Chandra X-ray Center controls science
and flight operations from Cambridge, Mass. The Chandra work was also
supported by funds from the National Science Foundation.

Images associated with the release are available at:

http://chandra.harvard.edu

and

http://chandra.nasa.gov

SpaceRef staff editor.