Misplaced Pages

Messier 99: Difference between revisions

Article snapshot taken from Wikipedia with creative commons attribution-sharealike license. Give it a read and then ask your questions in the chat. We can research this topic together.
Browse history interactively← Previous editNext edit →Content deleted Content addedVisualWikitext
Revision as of 07:42, 9 June 2006 editYurikBot (talk | contribs)278,165 editsm robot Adding: ru:M99← Previous edit Revision as of 14:32, 10 June 2006 edit undoBluebot (talk | contribs)349,597 edits Unicodifying using AWBNext edit →
Line 5: Line 5:
| type = SA(s)c: I | type = SA(s)c: I
| ra = 12<sup>h</sup> 18<sup>m</sup> 49.6<sup>s</sup> | ra = 12<sup>h</sup> 18<sup>m</sup> 49.6<sup>s</sup>
| dec = +14&deg; 25' 01" | dec = +14° 25' 01"
| dist_ly = ] ] | dist_ly = ] ]
| z = +0.008036 | z = +0.008036
Line 31: Line 31:
* *
<br> <br>

{{galaxy-stub}}


] ]
Line 44: Line 42:
] ]
] ]


{{galaxy-stub}}

Revision as of 14:32, 10 June 2006

Galaxies
Morphology
Structure
Active nuclei
Energetic galaxies
Low activity
Interaction
Lists
See also

Messier 99 (also kown as NGC 4254 or M99 for short, nicknamed Coma Pinwheel Galaxy) is a spiral galaxy approximatly 60 million light-years away in the constellation Coma Berenices. It was discovered by Pierre Méchain in 1781.

The galaxy has a normal looking arm and an extended arm that is less tightly wound. A bridge of neutral hydrogen gas links NGC 4254 with VIRGOHI21. The gravity from the dark galaxy VIRGOHI21 appears to have distorted M99 and drawn out the gas bridge, as the two galaxy-sized objects have a close encounter, before they go their separate ways. It is expected that the drawn out arm will relax to match the normal arm once the encounter is over.

See also

External links



Stub icon

This galaxy-related article is a stub. You can help Misplaced Pages by expanding it.

Categories: