Explanation: How did spiral galaxy ESO510-13 get bent out-of-shape? The disks of many spirals are thin and flat, but not solid. Spiral disks are loose conglomerations of billions of stars and diffuse gas all gravitationally orbiting a galaxy center. A flat disk is thought to be created by sticky collisions of large gas clouds early in the galaxy's formation. Warped disks are not uncommon, though, and even our own Milky Way Galaxy is thought to have a small warp. The causes of spiral warps are still being investigated, but some warps are thought to result from interactions or even collisions between galaxies. ESO510-13, pictured above, is about 150 million light years away and about 100,000 light years across.

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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.

Publikacii s klyuchevymi slovami: disk - warp - spiral galaxy - ESO - spiral'naya galaktika - disk, galakticheskii - vzaimodeistvuyushie galaktiki Publikacii so slovami: disk - warp - spiral galaxy - ESO - spiral'naya galaktika - disk, galakticheskii - vzaimodeistvuyushie galaktiki
Sm. takzhe: NGC 1546 ot teleskopa im.Habbla Mess'e 66 krupnym planom NGC 4565: galaktika, vidimaya s rebra NGC 2403 v Zhirafe Rasputyvayushayasya galaktika NGC 3169 M100: galaktika s regulyarnym spiral'nym uzorom Licom k NGC 1232 Vse publikacii na tu zhe temu >>