Messier 63
Appearance
Sunflower Galaxy | |
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Observation data (J2000 epoch) | |
Constellation | Canes Venatici |
Right ascension | 13h 15m 49.3s[1] |
Declination | +42° 01′ 45″[1] |
Redshift | 504 km/s[1] |
Distance | 37 Mly[2] |
Apparent magnitude (V) | 9.3[1] |
Characteristics | |
Type | SA(rs)bc[1] |
Apparent size (V) | 12′.6 × 7′.2[1] |
Other designations | |
M63, NGC 5055, UGC 8334, PGC 46153[1] |
The Sunflower Galaxy (also known as Messier 63, M63, or NGC 5055) is a spiral galaxy in the constellation Canes Venatici consisting of a central disc surrounded by many short spiral arm segments. The Sunflower Galaxy is part of the M51 Group, a group of galaxies that also includes the Whirlpool Galaxy (M51).
History
The Sunflower Galaxy was discovered by Pierre Méchain on June 14, 1779.[3] The galaxy was then listed by Charles Messier as object 63 in the Messier Catalogue.
In the mid-19th century, Lord Rosse identified spiral structure within the galaxy, making this one of the first galaxies in which such structure was identified.[3]
In 1971, a supernova with a magnitude of 11.8 appeared in one of the arms of M63.
Gallery
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Messier 63, 24 inch telescope on Mt. Lemmon, AZ.
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Messier 63 seen in infrared by the Spitzer Space Telescope.
References
- ^ a b c d e f g "NASA/IPAC Extragalactic Database". Results for NGC 5055. Retrieved 2006-10-10.
- ^ Frommert, Hartmut & Kronberg, Christine (2002). "Messier Object 63". Retrieved Dec. 6, 2006
- ^ a b K. G. Jones (1991). Messier's Nebulae and Star Clusters (2nd edition ed.). Cambridge: Cambridge University Press. ISBN 0-521-37079-5.
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External links
Wikimedia Commons has media related to Sunflower Galaxy.
- The Sunflower Galaxy on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
- Sunflower Galaxy @ SEDS Messier pages