< Messier Index
Messier 100 | |
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![]() Credit: w:ESO w:VLT view revealing complex spiral arm structure | |
Observation data (w:J2000 epoch) | |
Constellation | w:Coma Berenices[1] |
Right ascension | 12h 22m 54.9s[2] |
Declination | +15° 49′ 21″[2] |
Redshift | 1571 ± 1 km/s[2] |
Distance | 52.5 Mly[3] |
Type | SAB(s)bc[2] |
Apparent dimensions (V) | 7′.4 × 6′.3[2] |
Apparent magnitude (V) | 10.1[2] |
Other designations | |
NGC 4321 |
Messier 100 (also known as NGC 4321) is a w:spiral galaxy about 52.5 million w:light-years away in the w:constellation w:Coma Berenices. It was discovered by w:Pierre Méchain in w:1781. It is one of the brightest galaxies in the w:Virgo cluster. Five w:supernovae have been identified in M100: w:SN 1901B, w:SN 1914A, w:SN 1959E, w:SN 1979C and w:SN 2006X. M100 also has a w:satellite galaxy named w:NGC 4323.
Other images
- Before and after HST repair mission. Credit: NASA
- SN 2006X in Messier 100. Credit: w:ESO
External links
References
- ↑ R. W. Sinnott, editor (1988). The Complete New General Catalogue and Index Catalogue of Nebulae and Star Clusters by J. L. E. Dreyer. Sky Publishing Corporation and Cambridge University Press. ISBN 0-933-34651-4.
- 1 2 3 4 5 6 "NASA/IPAC Extragalactic Database". Results for NGC 4321. http://nedwww.ipac.caltech.edu/. Retrieved 2006-08-31.
- ↑ "Pattern Speeds BIMA-SONG Galaxies with Molecule-Dominated ISMs Using the Tremaine-Weinberg Method". (Ferrarese et al. 1996). http://arxiv.org/abs/astro-ph/0406426. Retrieved 2006-08-31.
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