HLX-1

118,000 kmevent horizon diameter

Updated

118,000km
Visual creditscaleofspace.org / CC BY-NC 4.0

Details

HLX-1 is one of the strongest known candidates for an intermediate-mass black hole and lies off the plane of ESO 243-49. Hubble observations suggest it may be the stripped core of a cannibalized dwarf galaxy, leaving a midsize black hole with a small cluster of young stars around it.

HLX-1 is an off-nuclear, hyperluminous X-ray source in ESO 243-49. Its luminosity, changing X-ray spectrum and repeated outbursts are consistent with an intermediate-mass black hole, although the mass depends on how its accretion flow is modeled.

A surrounding stellar population has prompted the hypothesis that HLX-1 is the stripped nucleus of a dwarf galaxy. That origin is plausible but not established.

Key facts

Category
Black holes
Object class
Intermediate-mass black hole candidate
Host
ESO 243-49
Scale fact
118,000 kmevent horizon diameter
Mass
~20,000 solar masses (model estimate)
Embed

Size neighbors

Objects near HLX-1 on the scale

On the logarithmic size axis, HLX-1 falls between Saturn and Jupiter. 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 HLX-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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