Holmberg IX | |
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![]() Hubble Space Telescope image of the dwarf irregular galaxy Holmberg IX | |
Observation data (J2000 epoch) | |
Constellation | Ursa Major |
Right ascension | 09h 57m 32.1s [1] |
Declination | +69° 02′ 46″ [1] |
Distance | 12 Mly (3.6 Mpc) [2] |
Apparent magnitude (V) | 16.5 [1] |
Characteristics | |
Type | dI [1] |
Apparent size (V) | 1.41 ± 0.07 [1] |
Notable features | Satellite galaxy of Messier 81 |
Other designations | |
UGC 5336, [B93] 17, DDO 66, 2E 0953.7+6918, 2E 2199, 1ES 0953+69.3, HIJASS J0957+69A, Holmberg IX, [IW2001] H42, [IW2001] P63, K68 62, LEDA 28757, Mailyan 48, MCG+12-10-012, [MI94] Im 62, SPB 118, PGC 28757 |
Holmberg IX is a dwarf irregular galaxy and a satellite galaxy of M81, located in the constellation of Ursa Major. It is a Magellanic type galaxy, similar to the Small Magellanic Cloud, neighbour galaxy to the Milky Way Galaxy. [3] The galaxy is named after Erik Holmberg who first described it, though it was originally discovered by Sidney van den Bergh in 1959. [4] [3] Based on the observed age distribution of stars it contains, 20% of its stellar mass formed within the last 200 Myr, making it the youngest nearby galaxy. [5] It is also home to one of two yellow supergiant eclipsing binary systems. [6] [7]