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Credit & Copyright: April Hobart,
CXC
Explanation:
In the center of a swirling whirlpool of hot gas
is likely a beast that has never been seen directly: a
black hole.
Studies of the bright light emitted by the
swirling gas frequently indicate not only that a
black hole is present, but also likely attributes.
The gas surrounding GRO J1655-40, for example, has been found to display an unusual flickering
at a rate of 450 times a second.
Given a
previous mass estimate for the
central object of seven times the mass of our
Sun, the rate of the
fast flickering can be
explained by a black hole
that is rotating very rapidly.
What physical mechanisms actually cause the flickering -- and a slower quasi-periodic
oscillation (QPO) -- in
accretion disks surrounding
black holes and
neutron stars remains a topic of much research.
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NASA Official: Jay Norris. Specific rights apply.
A service of: LHEA at NASA / GSFC
& Michigan Tech. U.
Based on Astronomy Picture
Of the Day
Publications with keywords: black hole - accretion disk
Publications with words: black hole - accretion disk
See also:
- APOD: 2025 September 24 Á GW250114: Rotating Black Holes Collide
- APOD: 2025 May 9 Á IXPE Explores a Black Hole Jet
- APOD: 2025 May 6 Á The Doubly Warped World of Binary Black Holes
- APOD: 2025 May 4 Á Spin up of a Supermassive Black Hole
- APOD: 2024 November 24 Á Journey to the Center of the Galaxy
- APOD: 2024 October 1 Á Porphyrion: The Longest Known Black Hole Jets
- APOD: 2024 June 16 Á Animation: Black Hole Destroys Star