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Willman 1 is an ultra low-luminosity dwarf galaxy or a star cluster. Willman 1 was discovered in 2004.〔Space.com, ("Puzzling Milky Way Companion Found" ), Robert Roy Britt, 25 October 2004 (accessed 12 June 2013)〕 It is named after Beth Willman of Haverford College, the lead author of a study based on the Sloan Digital Sky Survey data. The object is a satellite of the Milky Way, at ~120,000 light-years away.〔 Willman 1 has an elliptical shape with the half-light radius of about 25 pc. Its heliocentric velocity is approximately −13 km/s.〔 As of 2007, it was declared the least massive galaxy known, opening up a new category of ultra-low-mass galaxies, lower than the then-theoretical minimum of 10 million solar masses thought to be needed to form a galaxy.〔New Scientist, ("Smallest galaxy hints at hidden population" ), David Shiga, 4 June 2007 (accessed 12 June 2013)〕 As of 2011, it is the second dimmest likely galaxy known, after Segue 1, and is less than one ten millionth the Milky Way's luminosity. It has an absolute magnitude of .〔 Observations indicate its mass is about 0.4 million solar masses, which means that Willman's 1 mass to light ratio is around 800.〔 A high mass to light ratio implies that Willman 1 is dominated by dark matter. It is difficult, however, to estimate the mass of such faint objects because any mass estimate is based on an implicit assumption that an object is gravitationally bound, which may not be true if the object is in a process of disruption.〔 The stellar population of Willman 1 consists mainly of old stars formed more than 10 billion years ago.〔 The metallicity of these stars is also very low at , which means that they contain 110 times less heavy elements than the Sun.〔 == Notes == : a. 15.2 ± 0.4 apparent magnitude − 5 * (log10(38 ± 7〔 kpc distance) − 1) = −2.7〔 absolute magnitude 抄文引用元・出典: フリー百科事典『 ウィキペディア（Wikipedia）』 ■ウィキペディアで「Willman 1」の詳細全文を読む スポンサード リンク
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