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.[5]
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 magnitudeof−2.7 ± 0.7.[2] Observations indicate its mass is about 0.4 million solar masses, which means that Willman's 1 mass to light ratio is around 800.[3] 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.[3]
The stellar population of Willman 1 consists mainly of old stars formed more than 10 billion years ago.[1] The metallicity of these stars is also very low at [Fe/H] ≈ −2.1, which means that they contain 110 times less heavy elements than the Sun.[3]
NED (9 January 2007), "Results for SDSS J1049+5103", NASA/IPAC Extragalactic Database, Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration
Martin, N. F.; De Jong, J. T. A.; Rix, H. W. (2008). "A Comprehensive Maximum Likelihood Analysis of the Structural Properties of Faint Milky Way Satellites". The Astrophysical Journal. 684 (2): 1075–1092. arXiv:0805.2945. Bibcode:2008ApJ...684.1075M. doi:10.1086/590336. S2CID17838966.
Willman, Beth; Blanton, Michael R.; West, Andrew A.; Dalcanton, Julianne J.; Hogg, David W.; Schneider, Donald P.; Wherry, Nicholas; Yanny, Brian; Brinkmann, Jon (2005), "A New Milky Way Companion: Unusual Globular Cluster or Extreme Dwarf Satellite?", The Astronomical Journal, 129 (6): 2692–2700, arXiv:astro-ph/0410416, Bibcode:2005AJ....129.2692W, doi:10.1086/430214, S2CID826898
10h49m22.3s, +51° 03′ 03.6″
