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{{Galaxy | |||
⚫ | |||
| name = Messier 99 | |||
| image = ] | |||
<small>Spiral Galaxy Messier 99 | |||
| epoch = ] | |||
| type = SA(s)c: I | |||
| ra = 12<sup>h</sup> 18<sup>m</sup> 49.6<sup>s</sup> | |||
| dec = +14° 25' 01" | |||
| dist_ly = ] ] | |||
| z = +0.008036 | |||
| appmag_v = +9.7 | |||
| size_v = 5.4' × 4.7' | |||
| constellation name = ] | |||
| radius_ly = ? | |||
| absmag_v = 13 | |||
| names = NGC 4254,<br>'''''Coma Pinwheel Galaxy''''' | |||
}} | |||
⚫ | '''Messier 99''' (also kown as '''''NGC 4254''''' or '''''M99''''' for short, nicknamed '''''Coma Pinwheel Galaxy''''') is a ] approximatly ] ]s away in the ] ]. It was discovered by ] in ]. | ||
⚫ | 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 ]. The gravity from the ] ] 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. | ||
⚫ | 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 ]. The gravity from the ] ] 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== | ||
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== Other resourses == | |||
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==External links== | === External links === | ||
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{{galaxy-stub}} | |||
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Revision as of 00:21, 7 April 2006
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 VIRGOHI 21. 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.
Other resourses
See also
External links
- SEDS: Spiral Galaxy M99
- UniverseToday: Dark Matter Galaxy?
- PPARC: New evidence for a Dark Matter Galaxy
This galaxy-related article is a stub. You can help Misplaced Pages by expanding it. |