Jump to content

Ring galaxy: Difference between revisions

From IdeaWazaWiki
wikademia>Kalki
higher quality image
wikademia>Wikademia
m Text replace - '[[School:' to '[['
 
(26 intermediate revisions by 22 users not shown)
Line 1: Line 1:
[[Image:Hoag's object.jpg|right|thumb|Hoag's Object, a ring galaxy.]]
[[Image:Hoag's object.jpg|right|thumb|Hoag's Object, a ring galaxy.]]
A '''ring galaxy''' is a [[galaxy]] with a ring-like appearance. The ring consists of massive, relatively young blue [[star]]s, which are extremely bright. The central region contains relatively little luminous [[matter]]. [[Astronomy|Astronomers]] believe that ring galaxies are formed when a smaller galaxy passes through the center of a larger galaxy. Because most of a galaxy consists of empty space, this "collision" rarely results in any actual collisions between stars. However the [[gravity|gravitational]] disruptions caused by such an event could cause a [[wave]] of star formation to move through the larger galaxy.
A '''ring galaxy''' is a [[galaxy]] with a ring-like appearance. The ring consists of massive, relatively young blue stars, which are extremely bright. The central region contains relatively little luminous matter. Some [[Astronomy|astronomers]] believe that ring galaxies are formed when a smaller galaxy passes through the center of a larger galaxy. Because most of a galaxy consists of empty space, this "collision" rarely results in any actual collisions between stars. However the gravitational disruptions caused by such an event could cause a wave of star formation to move through the larger galaxy. Others think that rings are formed around some galaxies when external accretion takes place. The star formation would then take place in the accreted material because of the shocks and compressions of the accreted material. There might be a link between ring galaxies and polar ring galaxies.


[[Hoag's Object]], discovered by [[Art Hoag]] in [[1950]] is an example of such a galaxy.
[[Hoag's Object]], discovered by Art Hoag in 1950 is an example of such a galaxy.


== See also ==
==External links==
*[http://antwrp.gsfc.nasa.gov/apod/ap020909.html Hoag's Object] at Astronomy Picture of the Day


* [[Active galaxy]]
* [[Barred spiral galaxy]]
* [[Dwarf galaxy]]
* [[Dwarf elliptical galaxy]]
* [[Dwarf spheroidal galaxy]]
* [[Elliptical galaxy]]
* [[Galaxy classification]]
* [[Galaxy formation and evolution]]
* [[Groups and clusters of galaxies]]
* [[Irregular galaxy]]
* [[Lenticular galaxy]]
* [[List of galaxies]]
* [[List of nearest galaxies]]
* [[Spiral galaxy]]
* [[Starburst galaxy]]
* [[Seyfert galaxy]]
* [[Timeline of galaxies, clusters of galaxies, and large scale structure]]
== External link ==
*[http://antwrp.gsfc.nasa.gov/apod/ap020909.html Hoag's Object] at [[Astronomy Picture of the Day]].
{{galaxy-stub}}
[[Category:Ring galaxies|*]]
[[Category:Galaxy types]]
[[Category:Galaxy types]]
[[de:Ringgalaxie]]
[[sk:Prstencová galaxia]]
[[sr:Прстенаста галаксија]]

Latest revision as of 03:39, 8 June 2009

Hoag's Object, a ring galaxy.

A ring galaxy is a galaxy with a ring-like appearance. The ring consists of massive, relatively young blue stars, which are extremely bright. The central region contains relatively little luminous matter. Some astronomers believe that ring galaxies are formed when a smaller galaxy passes through the center of a larger galaxy. Because most of a galaxy consists of empty space, this "collision" rarely results in any actual collisions between stars. However the gravitational disruptions caused by such an event could cause a wave of star formation to move through the larger galaxy. Others think that rings are formed around some galaxies when external accretion takes place. The star formation would then take place in the accreted material because of the shocks and compressions of the accreted material. There might be a link between ring galaxies and polar ring galaxies.

Hoag's Object, discovered by Art Hoag in 1950 is an example of such a galaxy.