File:Messier105_-_HST_-_Potw1901a.jpg · Wikimedia Commons · See Wikimedia Commons
Messier 105 is a giant elliptical galaxy located about 32 million light-years away in the constellation Leo. It's one of the brightest elliptical galaxies visible from Earth and serves as an important reference point for astronomers studying galaxy formation and evolution.
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Wikidata facts
- Distance from Earth
- 8.1
- Image
- Messier105 - HST - Potw1901a.jpg
Show 10 more facts
- redshift
- 0.002983
- Commons category
- Messier 105
- catalog code
- LEDA 32256
- time of discovery or invention
- 1781-03-24
- Commons gallery
- Messier 105
- apparent magnitude
- 8.897
- galaxy morphological type
- E1
- right ascension
- 161.9566667
- declination
- 12.5816306
- radial velocity
- 875
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Article
Messier 105 or M105, also known as NGC 3379, is an elliptical galaxy 36.6 million light-years away in the equatorial constellation of Leo. It is the biggest elliptical galaxy in the Messier catalogue that is not in the Virgo cluster. It was discovered by Pierre Méchain in 1781, just a few days after he discovered the nearby galaxies Messier 95 and Messier 96. This galaxy is one of a few not object-verified by Messier so omitted in the editions of his Catalogue of his era. It was appended when Helen S. Hogg found a letter by Méchain locating and describing this object which matched those aspects under its first-published name, NGC 3379.
Messier 105 has a morphological classification of E1, indicating a standard elliptical galaxy with a flattening of 10%. The major axis is aligned along a position angle of 71°. Isophotes of the galaxy are near perfect ellipses, twisting no more than 5° out of alignment, with changes in ellipticity of no more than 0.06. There is no fine structure apparent in the isophotes, such as ripples. Observation of giant stars in the halo indicate there are two general populations: a dominant metal-rich subpopulation and a weaker metal-poor group.