Explanation: These two mighty galaxies are pulling each other apart. Known as The Mice because they have such long tails, each large spiral galaxy has actually passed through the other. Their long tails are drawn out by strong gravitational tides rather than collisions of their individual stars. Because the distances are so large, the cosmic interaction takes place in slow motion -- over hundreds of millions of years. They will probably collide again and again over the next billion years until they coalesce to form a single galaxy. NGC 4676 lies about 300 million light-years away toward the constellation of Bernice's Hair (Coma Berenices) and are likely members of the Coma Cluster of Galaxies. Not often imaged in small telescopes, this wide field of view catches the faint tidal tails several hundred thousand light-years long.

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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: colliding galaxies - stalkivayushiesya galaktiki - NGC 4676 Publikacii so slovami: colliding galaxies - stalkivayushiesya galaktiki - NGC 4676
Sm. takzhe: NGC 7714: vspyshka zvezdoobrazovaniya posle stolknoveniya galaktik AM1054: formirovanie zvezd pri stolknovenii galaktik Arp 142: galaktika Kolibri Stalkivayushiesya spiral'nye galaktiki Arp 274 Voiny galaktik: M81 i M82 NGC 1316: posle stolknoveniya galaktik NGC 4676: kogda myshki stalkivayutsya Vse publikacii na tu zhe temu >>