Cygnus X-1

120 kmevent horizon diameter

Updated

120km
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Details

Cygnus X-1 was the first cosmic object widely accepted as a black hole. It blazes in X-rays because the black hole is stripping hot gas from a massive blue supergiant companion and funneling it into a compact accretion flow.

Cygnus X-1 contains a black hole with a measured mass of about 21 solar masses, orbiting a massive blue supergiant. Gas drawn from the star heats in an accretion flow and emits X-rays; the black hole itself remains unseen.

The system became the first widely accepted stellar-mass black hole because its compact object was too massive to be a neutron star. Radio astrometry and optical measurements have since refined both its distance and mass.

Key facts

Category
Black holes
Object class
Stellar black hole
Mass
~21 solar masses
Scale fact
120 kmevent horizon diameter
Estimated age
~5 million years
Host
Cygnus X-1 binary system
Embed

Size neighbors

Objects near Cygnus X-1 on the scale

On the logarithmic size axis, Cygnus X-1 falls between Pandora and 21 Lutetia. The band uses nearby Black holes records.

Shared physical scale
181billion km
Cygnus X-1120 km
NGC 4395 Black Hole59,000 km
HLX-1118,000 km
Sagittarius A*24.5 million km
M87*38 billion km
Holm 15A*236 billion km

Sources

References for Cygnus X-1

Measurements and descriptive context are compiled by the Scale of Space team from the references below. If you find an error, please let us know.

Continue with nearby objects or open the full scale.

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