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The Doomed Dust Disk of NGC 7052
<< Yesterday 22.06.1998 Tomorrow >>
The Doomed Dust Disk of NGC 7052
Credit & Copyright: R. P. van der Marel (STScI) et al., WFPC2, HST, NASA
Explanation: What created the dust disk in the center of NGC 7052, and what keeps it spinning? Although the disk might appear as a relatively tame "hubcap in space", the unusual center of elliptical galaxy NGC 7052 is probably the remnant of a titanic collision between galaxies. What's more, the disk's spin indicates the tremendous gravity of a massive central black hole. Analysis of this recently released photo by the Hubble Space Telescope indicates that the disk is thousands of light-years across, rotates faster than 100 kilometers per second, at a distance of 150 light-years from the center, and contains more mass than a million Suns. The theorized central black hole is thought to be yet 100 times more massive, and may swallow the entire disk in the next few million years.

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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.

Russkii tekst
Based on Astronomy Picture Of the Day
Publikacii s klyuchevymi slovami: black hole - dust disk - Elliptical Galaxy - chernye dyry - Yadra galaktik - pylevoi disk - ellipticheskaya galaktika
Publikacii so slovami: black hole - dust disk - Elliptical Galaxy - chernye dyry - Yadra galaktik - pylevoi disk - ellipticheskaya galaktika
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