The Milky Way has several smaller galaxies gravitationally bound to it, as part of the Milky Way subgroup, which is part of the local galaxy cluster, the Local Group.[1]

There are 61 small galaxies confirmed to be within 420 kiloparsecs (1.4 million light-years) of the Milky Way,[2] but not all of them are necessarily in orbit, and some may themselves be in orbit of other satellite galaxies. The only ones visible to the naked eye are the Large and Small Magellanic Clouds, which have been observed since prehistory. Measurements with the Hubble Space Telescope in 2006 suggest the Magellanic Clouds may be moving too fast to be orbiting the Milky Way.[3] Of the galaxies confirmed to be in orbit, the largest is the Sagittarius Dwarf Elliptical Galaxy, which has a diameter of 2.6 kiloparsecs (8,500 ly)[4] or roughly a twentieth that of the Milky Way.

Characteristics

Satellite galaxies that orbit from 1,000 ly (310 pc) of the edge of the disc of the Milky Way Galaxy to the edge of the dark matter halo of the Milky Way at 980,000 ly (300 kpc) from the center of the galaxy,[lower-alpha 1] are generally depleted in hydrogen gas compared to those that orbit more distantly. This is because of their interactions with the dense hot gas halo of the Milky Way that strip cold gas from the satellites. Satellites beyond that region still retain copious quantities of gas.[5][6]

List

The Milky Way's satellite galaxies include the following:[7][2]

Name Diameter (kpc) Distance
(kpc)		 Absolute visual magnitude Type Discovered
Large Magellanic Cloud448.5 −18.1SBmprehistoric
Antlia 22.9 130 −8.5Irr?2018
Sagittarius Dwarf2.620 −13.5E1994
Crater II2.2117.5 −8.2dSph2016 [8]
Small Magellanic Cloud261 −16.8Irrprehistoric
Canes Venatici I1.1220 −8.6dSph2006
Canis Major Dwarf1.58 −14.4Irr2003
Boötes III1.046 −5.75dSph?2009
Sculptor Dwarf0.890 −11.1dE31937
Draco Dwarf0.780 −8.8dE01954
Hercules0.7135 −6.6dSph2006
Leo II0.7210 −9.8dE01950
Fornax Dwarf0.6140 −13.4dE21938
Eridanus II[9]0.55366 −7.1dSph2015 [10][11]
Sextans Dwarf Spheroidal0.590 −9.3dE31990
Carina Dwarf Spheroidal0.5100 −9.1dE31977
Leo I0.5250 −12.0dE31950
Ursa Minor Dwarf0.460 −8.8dE41954
Leo T0.34420 −8.0dSph/dIrr2006
Aquarius II0.32108 −4.2dSph2016 [12]
Boötes I0.3060 −6.3dSph2006
Canes Venatici II0.30155 −4.9dSph2006
Leo IV0.30160 −5.8dSph2006
Tucana IV0.2548 −3.5dSph2015 [13]
Columba I0.21182 −4.5dSph2015 [13]
Ursa Major II Dwarf0.2030 −4.25dG D2006
Grus II0.1953 −3.9dSph2015 [13]
Cetus III0.18251 −2.4dSph?2017 [14]
Coma Berenices0.1442 −4.1dSph2006
Hydra II0.14128 −4.8dSph2015 [15]
Reticulum III0.1392 −3.3dSph2015 [13]
Pisces II0.12180 −5.0dSph2010
Pegasus III0.11215 −3.4dSph2015 [16][17]
Hydrus I0.1028 −4.7dSph2018 [18]
Boötes II0.1042 −2.7dSph2007
Tucana III0.0925 −2.4dSph2015 [13]
Virgo I0.0991 −0.3dSph?2016 [14]
Horologium II0.0978 −2.6dSph2015 [19]
Sagittarius II0.0867 −5.2dSph2015 [20]
Leo V0.08180 −5.2dSph2007
Triangulum II0.0730 −1.8dSph2015
Segue 20.0735 −2.5dSph2007
Segue 10.0623 −1.5dSph2007
Draco II0.0420 −2.9dSph2015 [20]
Tucana V0.0355 −1.6dSph2015 [13]
Cetus II0.0330 0.0dSph?2015 [13]
Reticulum II0.06430 −3.6dSph2015 [10][11]
Tucana II0.3370 −3.9dSph2015 [10][11]
Pisces Overdensity1.580 −13dSph?2009
DES 10.0282 −3.05GC2016 [21]
Eridanus III0.02890 −2.4dSph?[lower-alpha 2]2015 [10][11]
Horologium I0.06100 −3.5dSph?[lower-alpha 2]2015 [10][11]
Kim 2/Indus I0.074100 −3.5GC2015 [10][11]
Phoenix II0.0521100 −3.7dSph?[lower-alpha 2]2015 [10][11]
Ursa Major I Dwarf0.64100 −5.5dG D2005
Pictoris I0.058115 −3.7dSph?[lower-alpha 2]2015 [10][11]
Grus I0.12120 −3.4dSph2015 [10]
Pegasus IV0.08290 −4.25dSph2022 [22]
Carina II0.18236 −4.5dSph2018 [23]
Carina III0.0628 −2.4GC?2018 [23]
Boötes IV0.28209 −4.53dSph2019 [24]
Centaurus I0.076116 −5.55dSph2020 [25]
Pictor II0.04646 −3.2dSph2016 [26]
Willman 10.0238 −2.53dSph2018 [27]
Ursa Major III 0.003 10 +2.2 dSph 2023

Map with clickable regions

Milky Way's satellite galaxies (clickable map)

Streams

The Sagittarius Dwarf Spheroidal Galaxy is currently in the process of being consumed by the Milky Way and is expected to pass through it within the next 100 million years. The Sagittarius Stream is a stream of stars in polar orbit around the Milky Way leeched from the Sagittarius Dwarf. The Virgo Stellar Stream is a stream of stars that is believed to have once been an orbiting dwarf galaxy that has been completely distended by the Milky Way's gravity.

See also

Notes

  1. ↑ The distance to edge of the dark matter halo of the galaxy from its center is the virial radius of a galaxy, Rvir
  2. 1 2 3 4 May be a globular cluster instead

    References

    1. ↑ David G. Turner (15 August 2013). "An Eclectic View of our Milky Way Galaxy". Canadian Journal of Physics (published September 2013). 92 (9): 959–963. arXiv:1310.0014. Bibcode:2014CaJPh..92..959T. doi:10.1139/cjp-2013-0429. S2CID 118390693.
    2. 1 2 A. Drlica-Wagner (2020). "The Astrophysical Journal | Milky Way Satellite Census. I. The Observational Selection Function for Milky Way Satellites in DES Y3 and Pan-STARRS DR1". The Astrophysical Journal. 893 (1): 47. doi:10.3847/1538-4357/ab7eb9. hdl:10150/642363. S2CID 208857848.
    3. ↑ "Press release: Magellanic Clouds May Be Just Passing Through". Harvard University. January 9, 2007.
    4. ↑ Karachentsev, I. D.; Karachentseva, V. E.; Hutchmeier, W. K.; Makarov, D. I. (2004). "A Catalog of Neighboring Galaxies". The Astronomical Journal. 127 (4): 2031–2068. Bibcode:2004AJ....127.2031K. doi:10.1086/382905.
    5. ↑ "Milky Way Ransacks Nearby Dwarf Galaxies". SpaceDaily. 17 October 2014.
    6. ↑ "Milky Way ransacks nearby dwarf galaxies". ScienceDaily. 15 October 2014.
    7. ↑ Sjölander, Nils. "Milky Way satellite galaxies". Archived from the original on 2014-02-19.
    8. ↑ Torrealba, G.; Koposov, S.E.; Belokurov, V.; Irwin, M. (13 April 2016). "The feeble giant. Discovery of a large and diffuse Milky Way dwarf galaxy in the constellation of Crater". Monthly Notices of the Royal Astronomical Society. 459 (3): 2370–2378. arXiv:1601.07178. Bibcode:2016MNRAS.459.2370T. doi:10.1093/mnras/stw733.
    9. ↑ Crnojević, D.; Sand, D.J.; Zaritsky, D.; Spekkens, K.; Willman, B.; Hargis, J.R. (2016). "Deep imaging of Eridanus II and its lone star cluster". The Astrophysical Journal. 824 (1): L-14. arXiv:1604.08590. Bibcode:2016ApJ...824L..14C. doi:10.3847/2041-8205/824/1/L14. S2CID 2202492.
    10. 1 2 3 4 5 6 7 8 9 Koposov, Sergey E.; Belokurov, Vasily; Torrealba, Gabriel; Evans, N. Wyn (10 March 2015). "Beasts of the Southern Wild. Discovery of a large number of ultra faint satellites in the vicinity of the Magellanic Clouds". The Astrophysical Journal. 805 (2): 130. arXiv:1503.02079. Bibcode:2015ApJ...805..130K. doi:10.1088/0004-637X/805/2/130. S2CID 118267222.
    11. 1 2 3 4 5 6 7 8 DES Collaboration (10 March 2015). "Eight New Milky Way companions discovered in first-year Dark Energy Survey data". The Astrophysical Journal. 807 (1): 50. arXiv:1503.02584. Bibcode:2015ApJ...807...50B. doi:10.1088/0004-637X/807/1/50. S2CID 12011753.
    12. ↑ Torrealba, G.; Koposov, S.E.; Belokurov, V.; Irwin, M.; Collins, M.; Spencer, M.; Ibata, R.; Matteo, M.; Bonaca, A.; Jethwa, P. (2016). "At the survey limits: Discovery of the Aquarius 2 dwarf galaxy in the VST ATLAS and the SDSS data". Monthly Notices of the Royal Astronomical Society. 463 (1): 712–722. arXiv:1605.05338. Bibcode:2016MNRAS.463..712T. doi:10.1093/mnras/stw2051.
    13. 1 2 3 4 5 6 7 Drlica-Wagner, A.; et al. (4 November 2015). "Eight ultra-faint galaxy candidates discovered in Year Two of the Dark Energy Survey". The Astrophysical Journal. 813 (2): 109. arXiv:1508.03622. Bibcode:2015ApJ...813..109D. doi:10.1088/0004-637X/813/2/109. S2CID 55909299.
    14. 1 2 Homma, Daisuke; Chiba, Masashi; Okamoto, Sakurako; Komiyama, Yutaka; Tanaka, Masayuki; Tanaka, Mikito; Ishigaki, Miho N.; Hayashi, Kohei; Arimoto, Nobuo (2017-04-19). "Searches for New Milky Way Satellites from the First Two Years of Data of the Subaru/Hyper Suprime-Cam Survey: Discovery of Cetus III". Publications of the Astronomical Society of Japan. 70: S18. arXiv:1704.05977. Bibcode:2018PASJ...70S..18H. doi:10.1093/pasj/psx050.
    15. ↑ Martin, Nicolas F.; et al. (Survey of the Magellanic Stellar History) (23 April 2015). "Hydra II: A faint and compact Milky Way dwarf galaxy found in the survey of the Magellanic stellar history". The Astrophysical Journal Letters. 804 (1): L5. arXiv:1503.06216. Bibcode:2015ApJ...804L...5M. doi:10.1088/2041-8205/804/1/L5. S2CID 7814048.
    16. ↑ Kim, Dongwon; Jerjen, Helmut; Mackey, Dougal; Da Costa, Gary S.; Milone, Antonino P. (12 May 2015). "A hero's dark horse: Discovery of an ultra-faint Milky Way satellite in Pegasus". The Astrophysical Journal Letters. 804 (2): L-44. arXiv:1503.08268. Bibcode:2015ApJ...804L..44K. doi:10.1088/2041-8205/804/2/L44. S2CID 119302178.
    17. ↑ Kim, Dongwon; Jerjen, Helmut; Geha, Marla; Chiti, Anirudh; Milone, Antonino P.; Mackey, Dougal; da Costa, Gary; Frebel, Anna; Conn, Blair (2016). "Portrait of a dark horse: Photometric properties and kinematics of the ultra-faint Milky Way satellite Pegasus III". The Astrophysical Journal. 833 (1): 16. arXiv:1608.04934. Bibcode:2016ApJ...833...16K. doi:10.3847/0004-637X/833/1/16. S2CID 73677994.
    18. ↑ Koposov, Sergey E.; Walker, Matthew G.; Belokurov, Vasily; Casey, Andrew R.; Geringer-Sameth, Alex; Mackey, Dougal; Da Costa, Gary; Erkal, Denis; Jethwa, Prashin (2018-10-01). "Snake in the Clouds: a new nearby dwarf galaxy in the Magellanic bridge*". Monthly Notices of the Royal Astronomical Society. 479 (4): 5343–5361. arXiv:1804.06430. doi:10.1093/mnras/sty1772. ISSN 0035-8711.
    19. ↑ Kim, Dongwon & Jerjen, Helmut (28 July 2015). "Horologium II: A second ultra-faint Milky Way satellite in the Horologium constellation". The Astrophysical Journal Letters. 808 (2): L-39. arXiv:1505.04948. Bibcode:2015ApJ...808L..39K. doi:10.1088/2041-8205/808/2/L39. S2CID 117190468.
    20. 1 2 Laevens, B.P.M; Martin, N.F.; Bernard, E.J.; Schlafly, E.F.; Sesar, B. (1 November 2015). "Sagittarius II, Draco II and Laevens 3: Three new Milky Way satellites discovered in the PAN-STARRS 1 3π survey". The Astrophysical Journal. 813 (1): 44. arXiv:1507.07564. Bibcode:2015ApJ...813...44L. doi:10.1088/0004-637X/813/1/44. S2CID 54042426.
    21. ↑ Luque, E.; et al. (9 February 2016). "Digging deeper into Southern skies: A compact Milky Way companion discovered in first-year Dark Energy Survey data". Monthly Notices of the Royal Astronomical Society. 458 (1): 603–612. arXiv:1508.02381. Bibcode:2016MNRAS.458..603L. doi:10.1093/mnras/stw302.
    22. ↑ Cerny, W.; et al. (2023). "Pegasus IV: Discovery and Spectroscopic Confirmation of an Ultra-faint Dwarf Galaxy in the Constellation Pegasus". The Astrophysical Journal. 942 (2): 111. arXiv:2203.11788. Bibcode:2023ApJ...942..111C. doi:10.3847/1538-4357/aca1c3. S2CID 247597301.
    23. 1 2 Torrealba, G.; Belokurov, V.; Koposov, S. E.; Bechtol, K.; Drlica-Wagner, A.; Olsen, K. A. G.; Vivas, A. K.; Yanny, B.; Jethwa, P. (22 January 2018). "Discovery of two neighbouring satellites in the Carina constellation with MagLiteS". Monthly Notices of the Royal Astronomical Society. 475 (4): 5085–5097. arXiv:1801.07279. doi:10.1093/mnras/sty170.
    24. ↑ Homma (2019). "Boötes. IV. A new Milky Way satellite discovered in the Subaru Hyper Suprime-Cam Survey and implications for the missing satellite problem". Publications of the Astronomical Society of Japan. 71 (5). arXiv:1906.07332. doi:10.1093/pasj/psz076.
    25. ↑ Mau (2020). "Two Ultra-faint Milky Way Stellar Systems Discovered in Early Data from the DECam Local Volume Exploration Survey". The Astrophysical Journal. 890 (2): 136. arXiv:1912.03301. Bibcode:2020ApJ...890..136M. doi:10.3847/1538-4357/ab6c67. S2CID 208857609.
    26. ↑ Drlica-Wagner (2016). "An Ultra-Faint Galaxy Candidate Discovered in Early Data from the Magellanic Satellites Survey". The Astrophysical Journal. 833 (1): L5. arXiv:1609.02148. Bibcode:2016ApJ...833L...5D. doi:10.3847/2041-8205/833/1/L5. hdl:1885/153579. S2CID 56071154.
    27. ↑ Muñoz (2018). "A MegaCam Survey of Outer Halo Satellites. III. Photometric and Structural Parameters". The Astrophysical Journal. 860 (1): 66. arXiv:1806.06891. Bibcode:2018ApJ...860...66M. doi:10.3847/1538-4357/aac16b. S2CID 118978019.

    Further reading

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