Willman 1
Template:Use dmy dates Template:Short description Template:Infobox Galaxy
Willman 1 is an ultra low-luminosity dwarf galaxy or a star cluster.<ref name="Willmanetal2011">Template:Cite journal</ref> Willman 1 was discovered in 2004 and is located near Ursa Major in the night sky.<ref>{{#invoke:citation/CS1|citation |CitationClass=web }}</ref><ref>Template:Cite journal</ref> It is named after Beth Willman of Haverford College, the lead author of a study based on the Sloan Digital Sky Survey data.<ref>Template:Cite book</ref> The object is a satellite of the Milky Way, at ~120,000 light-years away.<ref>Template:Cite journal</ref> Willman 1 has an elliptical shape with the half-light radius of about 25 pc.<ref name="Martin2008">Template:Cite journal</ref> Its heliocentric velocity is approximately −13 km/s.<ref name="Willmanetal2011"/>
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.<ref>{{#invoke:citation/CS1|citation |CitationClass=web }}</ref>
As of 2016, it is the third dimmest likely galaxy known, after Segue 1 and Virgo I, and is over ten million times less luminous than the Milky Way. It has an absolute magnitude of Template:Nowrap.<ref name="Martin2008"/> Observations indicate its mass is about 0.4 million solar masses, which means that Willman's 1 mass to light ratio is around 800.<ref name="Willmanetal2011"/> A high mass to light ratio implies that Willman 1 is dominated by dark matter.<ref>Template:Cite journal</ref><ref>Template:Cite journal</ref> 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.<ref name="Willmanetal2011"/>
The stellar population of Willman 1 consists mainly of old stars formed more than 10 billion years ago.<ref>Template:Citation</ref> The metallicity of these stars is also very low at Template:Nowrap, which means that they contain 110 times less heavy elements than the Sun.<ref name="Willmanetal2011"/>
NotesEdit
- a. Template:Note label15.2 ± 0.4 apparent magnitude − 5 * (log10(38 ± 7<ref name="Martin2008"/> kpc distance) − 1) = −2.7<ref name="Martin2008"/> absolute magnitude
ReferencesEdit
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