Explanation: Over the course of billions of years, whole clusters of galaxies merge. Above is an X-ray image of Abell 2142, the result of the collision of two huge clusters of galaxies, and one of the most massive objects known in the universe. This false-color image shows a concentration of gas 50 million degrees hot near the center of the resulting cluster. Oddly, it is the relative coldness of the gas that makes this situation particularly interesting. The center of Abell 2142 is surrounded by gas fully twice as hot, a temperature thought to have been created by energy released during the colossal collision. Still, since we can only see a snapshot in time, much remains unknown about how clusters of galaxies form and coalesce.

<<  Mart  >> Pn Vt Sr Cht Pt Sb Vs     1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 25 26 27 28 29 30 31     1995   1996   1997 1998   1999   2000 2001   2002   2003 2004   2005   2006 2007   2008   2009 2010   2011   2012 2013   2014   2015 2016   2017   2018 2019   2020   2021 2022   2023   2024

Yanvar' Fevral' Mart Aprel' Mai Iyun' Iyul' Avgust Sentyabr' Oktyabr' Noyabr' Dekabr'

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: cluster of galaxies - Skoplenie galaktik - rentgenovskoe izluchenie Publikacii so slovami: cluster of galaxies - Skoplenie galaktik - rentgenovskoe izluchenie
Sm. takzhe: Skoplenie galaktik v Volosah Veroniki UHZ1: dalekaya galaktika i chernaya dyra Skoplenie galaktik v Pechi Skoplenie galaktik Eibell 370 i za nim Tumannost' Orla i goryachie rentgenovskie zvezdy Pervoe glubokoe pole teleskopa "Dzheims Vebb" Skoplenie galaktik Pandora Vse publikacii na tu zhe temu >>