accretion disk

American  

noun

Astronomy.

1. the rapidly spinning disk of gas that forms around the more compact component of a close binary star system as mass is transferred to the compact companion from the primary star.

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accretion disk Scientific  

1. A spinning disk of gas and dust surrounding a celestial object with an intense gravitational field, such as a star or a black hole. In binary star systems, the gravitational attraction of the denser star can pull matter from the other star into an accretion disk in its own orbit. The material in the accretion disk eventually spirals into the attracting star and adds to its mass. The gas in accretion disks that surround black holes becomes condensed and heated as it is sucked into the hole, emitting x-rays and other radiation that provide evidence for the presence of the black hole.

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Etymology

Origin of accretion disk

First recorded in 1975–80

Example Sentences

Active galactic nuclei occur when material spirals into a galaxy's central black hole, forming an extremely hot accretion disk.

From Science Daily

In this model, the central engine is an active galactic nucleus containing a supermassive black hole with an accretion disk, but instead of dust, the entire system is enshrouded in a thick layer of hydrogen gas that reddens the emitted light.

From Science Daily

The team suggests the answer lies in the temperature of the accretion disk around the central object.

From Science Daily

GX13+1 shines brightly in X-rays that come from an accretion disk of superheated material spiraling inward and striking the star's surface.

From Science Daily

Most of the emitted light, for example visible light and X-ray, get blocked by thick layers of cosmic dust and can’t pass through the accretion disk around them.

From Space Scoop