List of Milky Way's satellite galaxies
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The Milky Way Galaxy has several smaller galaxies gravitationally bound to it, as part of the Milky Way subgroup. This subgroup is part of the local galaxy cluster, the Local Group.
Announced in 2006, measurements with the Hubble Space Telescope suggest the Large and Small Magellanic Clouds may be moving too fast to be orbiting the Milky Way.[1]
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List [edit]
The Milky Way's satellite galaxies include the following:
| Name | Diameter (kpc) | Distance (kpc) |
Type | Discovered | |
|---|---|---|---|---|---|
| I | Canis Major Dwarf | 1.5 | 8 | Irr | 2003 |
| II | Virgo Stream Dwarf | 2.5 | 15 | Irr | ? |
| III | Sagittarius Dwarf | 2 | 20 | E | 1994 |
| IV | LMC | 4 | 48.5 | SBm | prehistoric |
| V | SMC | 2 | 61 | Irr | prehistoric |
| VI | Ursa Major II Dwarf | 0.2 | 30 | dG D | 2006 |
| VII | Ursa Minor Dwarf | 0.4 | 60 | dE4 | 1954 |
| VIII | Draco Dwarf | 0.7 | 80 | dE0 | 1954 |
| IX | Sculptor Dwarf Galaxy | 0.8 | 90 | dE3 | 1937 |
| X | Sextans Dwarf | 0.5 | 90 | dE3 | 1990 |
| XI | Carina Dwarf | 0.5 | 100 | dE3 | 1977 |
| XII | Ursa Major I Dwarf | - | 100 | dG D | 2005 |
| XIII | Fornax Dwarf | 0.6 | 140 | dE2 | 1938 |
| XIV | Leo II | 0.7 | 210 | dE0 | 1950 |
| XV | Leo I | 0.5 | 250 | dE3 | 1950 |
| ? | Leo IV | 0.3 | 160 | dSph | 2006 |
| ? | Leo V | 0.08 | 180 | dSph | 2007 |
| ? | Leo T | 0.34 | 420 | dSph/dIrr | 2006 |
| ? | Boötes I | 0.3 | 60 | dSph | 2006 |
| ? | Boötes II | 0.1 | 42 | dSph | 2007 |
| ? | Boötes III | 1 | 46 | ? | 2009 |
| ? | Coma Berenices | 0.14 | 42 | dSph | 2006 |
| ? | Segue 2 | 0.07 | 35 | dSph | 2007 |
| ? | Canes Venatici I | 2 | 220 | dSph | 2006 |
| ? | Canes Venatici II | 0.3 | 155 | dSph | 2006 |
| ? | Hercules | 0.7 | 135 | dSph | 2006 |
| ? | Pisces II | 0.12 | 180 | ? | 2010 |
Clickable map [edit]
Milky Way's satellite galaxies (clickable map)
References [edit]
See also [edit]
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