Messier 96
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| Observation data: J2000 epoch | |
|---|---|
| Constellation: | Leo |
| Right ascension: | 10h 46m 45.7s[1] |
| Declination: | +11° 49′ 12″[1] |
| Redshift: | 897 ± 4 km/s[1] |
| Distance: | 34 ± 3 Mly (10.4 ± 1.1 kpc)[2] |
| Type: | SAB(rs)ab[1] |
| Apparent dimensions (V): | 7′.6 × 5′.2[1] |
| Apparent magnitude (V): | +10.1[1] |
| Notable features: | |
| Other designations | |
| NGC 3368,[1] UGC 5882,[1] PGC 32192[1] | |
| See also: Galaxy, List of galaxies | |
Messier 96 (also known as NGC 3368) is an intermediate spiral galaxy about 34 million light-years away in the constellation Leo. It was discovered by Pierre Méchain in 1781.
[edit] Environment
M96 is the brightest galaxy within the M96 Group, a group of galaxies in the constellation Leo also includes the Messier objects M95 and M105 as well as at least nine other galaxies.[3][4][5][6]
[edit] External links
[edit] References
- ^ a b c d e f g h i NASA/IPAC Extragalactic Database. Results for NGC 3368. Retrieved on October 24, 2006.
- ^ J. L. Tonry, A. Dressler, J. P. Blakeslee, E. A. Ajhar, A. B. Fletcher, G. A. Luppino, M. R. Metzger, C. B. Moore (2001). "The SBF Survey of Galaxy Distances. IV. SBF Magnitudes, Colors, and Distances". Astrophysical Journal 546 (2): 681-693.
- ^ R. B. Tully (1988). Nearby Galaxies Catalog. Cambridge: Cambridge University Press. ISBN 0-521-35299-1.
- ^ P. Fouque, E. Gourgoulhon, P. Chamaraux, G. Paturel (1992). "Groups of galaxies within 80 Mpc. II - The catalogue of groups and group members". Astronomy and Astrophysics Supplement 93: 211-233.
- ^ A. Garcia (1993). "General study of group membership. II - Determination of nearby groups". Astronomy and Astrophysics Supplement 100: 47-90.
- ^ G. Giuricin, C. Marinoni, L. Ceriani, A. Pisani (2000). "Nearby Optical Galaxies: Selection of the Sample and Identification of Groups". Astrophysical Journal 543: 178-194.
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