Messier 110
M 110 credit: Atlas Image 2MASS/UMass/IPAC-Caltech/NASA/NSF. |
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Observation data Epoch J2000 |
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Constellation | Andromeda[2] |
Right ascension | 00h 40m 22.1s[3] |
Declination | +41° 41′ 07″[3] |
Apparent dimension (V) | 21.9 × 11.0 moa[3] |
Apparent magnitude (V) | 8.92[3] |
Characteristics | |
Type | E5 pec[3] |
Astrometry | |
Heliocentric radial velocity | -241 ± 3[3]km/s |
Redshift | -0.000804 ± 0.000010[3] |
Galactocentric velocity | -62 ± 8[3] km/s |
Distance | 2,690 ± 90 kly (824.76 ± 27.59 kpc) |
Other designations | |
Database references | |
SIMBAD | Search M110 data
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See also: Galaxy, List of galaxies |
Messier 110 (also known as 'The Edward Young Star' and NGC 205) is a dwarf elliptical galaxy that is a satellite of the Andromeda Galaxy.[4] M110 contains some dust and hints of recent star formation, which is unusual for dwarf elliptical galaxies in general.[4]
Contents
History
Although Charles Messier never included the galaxy in his famous list, it was depicted by him, together with M32, on a drawing of the Andromeda galaxy; a label on the drawing indicates that Messier first observed NGC 205 on August 10, 1773.[5] The galaxy was independently discovered by Caroline Herschel on August 27, 1783; her brother William Herschel described her discovery in 1785.[5] The suggestion to assign the galaxy a Messier number was made by Kenneth Glyn Jones in 1967.[6]
A few novae have been detected in this galaxy. Notably one discovered in 1999 by Johnson and Modjaz,[7] and another detected in 2002, by Nakano and Sumoto. The latter one, designated EQ J004015.8+414420, had also been captured in images taken by the SDSS (Sloan Digital Sky Survey) in October, 2002. [8]
Unlike M32, NGC205 does not show evidence for a supermassive black hole at its center.[9]
See also
References
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External links
Wikimedia Commons has media related to Messier 110. |
- Messier 110 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
- SEDS: Elliptical Galaxy M110
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