Black Hole Candidate Cygnus X 1
Explanation:
Is that a black hole?
Quite possibly.
The
Cygnus X-1
binary star system contains one of the best candidates for a
black hole.
The system was discovered because it is one of the brightest
X-ray
sources on the sky, shining so bright it was detected by the
earliest rockets
carrying cameras capable of seeing the previously unknown
X-ray sky.
The star's very name indicates that it is the single brightest X-ray source in the
constellation
of the Swan
Cygnus.
Data indicate that a
compact object
there contains about nine times the mass of the Sun and changes its
brightness continually on several time scales, at least down to milliseconds.
Such behavior is expected for a
black hole,
and difficult to explain with other models.
Pictured above is an artistic impression of the
Cygnus X-1 system.
On the left is the bright blue
supergiant star
designated HDE 226868, which is estimated as having about 30 times the mass of our
Sun.
Cygnus X-1 is depicted on the right, connected to its
supergiant companion by a stream of gas, and surrounded by an impressive
accretion disk.
The bright star in the
Cygnus X-1 system is visible with a small telescope.
Strangely, the
Cygnus X-1 black hole candidate
appears to have formed without a bright
supernova explosion.
Authors & editors:
Robert Nemiroff
(MTU) &
Jerry Bonnell
(USRA)
NASA Web Site Statements, Warnings,
and Disclaimers
NASA Official: Jay Norris.
Specific
rights apply.
A service of:
LHEA at
NASA /
GSFC
& Michigan Tech. U.
