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Satellite galaxies of the Milky Way
Galaxies bound to the Milky Way
Galaxies bound to the Milky Way
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.
There are 61 small galaxies confirmed to be within 420 kpc of the Milky Way, 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. Of the galaxies confirmed to be in orbit, the largest is the Sagittarius Dwarf Spheroidal Galaxy, which has a diameter of 2.6 kpc{{cite journal
Characteristics
Satellite galaxies that orbit from 1000 ly of the edge of the disc of the Milky Way Galaxy to the edge of the dark matter halo of the Milky Way at from the center of the galaxy, 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.
List
The Milky Way's satellite galaxies include the following:
| Name | Diameter (kpc) | Distance | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| (kpc) | Absolute visual magnitude | Type | Discovered | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| Large Magellanic Cloud | 4 | 48.5 | −18.1 | SBm | prehistoric | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| Antlia 2 | 2.9 | 130 | −8.5 | Irr? | 2018 | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| Sagittarius Dwarf | 2.6 | 20 | −13.5 | E | 1994 | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| Crater II | 2.2 | 117.5 | −8.2 | dSph | title=The feeble giant. Discovery of a large and diffuse Milky Way dwarf galaxy in the constellation of Crater | author1=Torrealba, G. | author2=Koposov, S.E. | author3=Belokurov, V. | author4=Irwin, M. | journal=Monthly Notices of the Royal Astronomical Society | doi=10.1093/mnras/stw733 | date=13 April 2016 | bibcode=2016MNRAS.459.2370T | volume=459 | issue=3 | pages=2370–2378 | doi-access=free | arxiv=1601.07178}} | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| Small Magellanic Cloud | 2 | 61 | −16.8 | Irr | prehistoric | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| Canes Venatici I | 1.1 | 220 | −8.6 | dSph | 2006 | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| Canis Major Dwarf | 1.5 | 8 | −14.4 | Irr | 2003 | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| Boötes III | 1.0 | 46 | −5.75 | dSph? | 2009 | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| Sculptor Dwarf | 0.8 | 90 | −11.1 | dE3 | 1937 | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| Draco Dwarf | 0.7 | 80 | −8.8 | dE0 | 1954 | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| Hercules | 0.7 | 135 | −6.6 | dSph | 2006 | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| Leo II | 0.7 | 210 | −9.8 | dE0 | 1950 | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| Fornax Dwarf | 0.6 | 140 | −13.4 | dE2 | 1938 | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| title=Deep imaging of Eridanus II and its lone star cluster | journal=The Astrophysical Journal | volume=824 | issue=1 | page=L-14 | first1=D. | last1=Crnojević | first2=D.J. | last2=Sand | first3=D. | last3=Zaritsky | author4-link=Kristine Spekkens | first4=K. | last4=Spekkens | first5=B. | last5=Willman | first6=J.R. | last6=Hargis | arxiv=1604.08590 | bibcode=2016ApJ...824L..14C | doi=10.3847/2041-8205/824/1/L14 | year=2016 | s2cid=2202492 | doi-access=free }} | 0.55 | 366 | −7.1 | dSph | 2015 | ||||||||||||||||||||||||||||||||||||||||||||||||
| Sextans Dwarf Spheroidal | 0.5 | 90 | −9.3 | dE3 | 1990 | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| Carina Dwarf Spheroidal | 0.5 | 100 | −9.1 | dE3 | 1977 | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| Leo I | 0.5 | 250 | −12.0 | dE3 | 1950 | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| Ursa Minor Dwarf | 0.4 | 60 | −8.8 | dE4 | 1954 | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| Leo T | 0.34 | 420 | −8.0 | dSph/dIrr | 2006 | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| Aquarius II | 0.32 | 108 | −4.2 | dSph | title=At the survey limits: Discovery of the Aquarius 2 dwarf galaxy in the VST ATLAS and the SDSS data | first1=G. | last1=Torrealba | first2=S.E. | last2=Koposov | first3=V. | last3=Belokurov | first4=M. | last4=Irwin | first5=M. | last5=Collins | first6=M. | last6=Spencer | first7=R. | last7=Ibata | first8=M. | last8=Matteo | first9=A. | last9=Bonaca | first10=P. | last10=Jethwa | arxiv=1605.05338 | doi=10.1093/mnras/stw2051 | volume=463 | issue=1 | journal=Monthly Notices of the Royal Astronomical Society | pages=712–722 | bibcode=2016MNRAS.463..712T | year=2016 | doi-access=free }} | ||||||||||||||||||||||||||||||||||||||||||
| Boötes I | 0.30 | 60 | −6.3 | dSph | 2006 | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| Canes Venatici II | 0.30 | 155 | −4.9 | dSph | 2006 | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| Leo IV | 0.30 | 160 | −5.8 | dSph | 2006 | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| Tucana IV | 0.25 | 48 | −3.5 | dSph | 2015 | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| Columba I | 0.21 | 182 | −4.5 | dSph | 2015 | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| Ursa Major II Dwarf | 0.20 | 30 | −4.25 | dG D | 2006 | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| Grus II | 0.19 | 53 | −3.9 | dSph | title=Eight ultra-faint galaxy candidates discovered in Year Two of the Dark Energy Survey | author1=Drlica-Wagner, A. | display-authors=etal | journal=The Astrophysical Journal | volume=813 | issue=2 | page=109 | doi=10.1088/0004-637X/813/2/109 | date=4 November 2015 | arxiv = 1508.03622 | bibcode=2015ApJ...813..109D | s2cid=55909299 }} | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| Cetus III | 0.18 | 251 | −2.4 | dSph? | last1=Homma | first1=Daisuke | last2=Chiba | first2=Masashi | last3=Okamoto | first3=Sakurako | last4=Komiyama | first4=Yutaka | last5=Tanaka | first5=Masayuki | last6=Tanaka | first6=Mikito | last7=Ishigaki | first7=Miho N. | last8=Hayashi | first8=Kohei | last9=Arimoto | first9=Nobuo | date=2017-04-19 | title=Searches for New Milky Way Satellites from the First Two Years of Data of the Subaru/Hyper Suprime-Cam Survey: Discovery of Cetus III | journal=Publications of the Astronomical Society of Japan | volume=70 | pages=S18 | arxiv=1704.05977 | doi=10.1093/pasj/psx050 | bibcode=2018PASJ...70S..18H }} | ||||||||||||||||||||||||||||||||||||||||||||||
| Coma Berenices | 0.14 | 42 | −4.1 | dG D | 2006 | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| Hydra II | 0.14 | 128 | −4.8 | dSph | title=Hydra II: A faint and compact Milky Way dwarf galaxy found in the survey of the Magellanic stellar history | first=Nicolas F. | last=Martin | collaboration=Survey of the Magellanic Stellar History | journal=The Astrophysical Journal Letters | date=23 April 2015 | volume=804 | issue=1 | pages=L5 | doi=10.1088/2041-8205/804/1/L5 | arxiv = 1503.06216 | bibcode = 2015ApJ...804L...5M | s2cid=7814048 }} | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| Reticulum III | 0.13 | 92 | −3.3 | dSph | 2015 | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| Pisces II | 0.12 | 180 | −5.0 | Sph | 2010 | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| Pegasus III | 0.11 | 215 | −3.4 | dSph | title=A hero's dark horse: Discovery of an ultra-faint Milky Way satellite in Pegasus | first1=Dongwon | last1=Kim | first2=Helmut | last2=Jerjen | first3=Dougal | last3=Mackey | first4=Gary S. | last4=Da Costa | first5=Antonino P. | last5=Milone | journal=The Astrophysical Journal Letters | date=12 May 2015 | volume=804 | issue=2 | page=L-44 | doi=10.1088/2041-8205/804/2/L44 | arxiv=1503.08268 | bibcode=2015ApJ...804L..44K | s2cid=119302178 }} | ||||||||||||||||||||||||||||||||||||||||||||||||||||
| Hydrus I | 0.10 | 28 | −4.7 | dSph | last1=Koposov | first1=Sergey E. | last2=Walker | first2=Matthew G. | last3=Belokurov | first3=Vasily | last4=Casey | first4=Andrew R. | last5=Geringer-Sameth | first5=Alex | last6=Mackey | first6=Dougal | last7=Da Costa | first7=Gary | last8=Erkal | first8=Denis | last9=Jethwa | first9=Prashin | date=2018-10-01 | title=Snake in the Clouds: a new nearby dwarf galaxy in the Magellanic bridge* | journal=Monthly Notices of the Royal Astronomical Society | language=en | volume=479 | issue=4 | pages=5343–5361 | doi=10.1093/mnras/sty1772 | doi-access=free | issn=0035-8711 | arxiv=1804.06430 | bibcode=2018MNRAS.479.5343K }} | ||||||||||||||||||||||||||||||||||||||||||
| Boötes II | 0.10 | 42 | −2.7 | dSph | 2007 | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| Tucana III | 0.09 | 25 | −2.4 | dSph | 2015 | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| Virgo I | 0.09 | 91 | −0.3 | dSph | 2016 | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| Horologium II | 0.09 | 78 | −2.6 | dSph | title=Horologium II: A second ultra-faint Milky Way satellite in the Horologium constellation | date=28 July 2015 | author1=Kim, Dongwon | author2=Jerjen, Helmut | name-list-style=amp | journal=The Astrophysical Journal Letters | volume=808 | issue=2 | page=L–39 | doi=10.1088/2041-8205/808/2/L39 | arxiv=1505.04948 | bibcode=2015ApJ...808L..39K | s2cid=117190468 }} | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| Sagittarius II | 0.08 | 67 | −5.2 | dSph | 2015 | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| Leo V | 0.08 | 180 | −5.2 | dSph | 2007 | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| Triangulum II | 0.07 | 30 | −1.8 | dSph | 2015 | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| Segue 2 | 0.07 | 35 | −2.5 | dSph | 2007 | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| Segue 1 | 0.06 | 23 | −1.5 | dSph | 2007 | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| Draco II | 0.04 | 20 | −2.9 | dSph | title=Sagittarius II, Draco II and Laevens 3: Three new Milky Way satellites discovered in the PAN-STARRS 1 3π survey | last1=Laevens | first1=B.P.M | last2=Martin | first2=N.F. | last3=Bernard | first3=E.J. | last4=Schlafly | first4=E.F. | last5=Sesar | first5=B. | journal=The Astrophysical Journal | date=1 November 2015 | volume=813 | issue=1 | page=44 | doi=10.1088/0004-637X/813/1/44 | arxiv=1507.07564 | bibcode=2015ApJ...813...44L | s2cid=54042426 }} | ||||||||||||||||||||||||||||||||||||||||||||||||||||
| Tucana V | 0.03 | 55 | −1.6 | dSph | 2015 | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| Cetus II | 0.03 | 30 | 0.0 | dSph? | 2015 | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| Reticulum II | 0.064 | 30 | −3.6 | dSph | title=Beasts of the Southern Wild. Discovery of a large number of ultra faint satellites in the vicinity of the Magellanic Clouds | author1=Koposov, Sergey E. | author2=Belokurov, Vasily | author3=Torrealba, Gabriel | author4=Evans, N. Wyn | date=10 March 2015 | arxiv=1503.02079 | journal=The Astrophysical Journal | bibcode=2015ApJ...805..130K | doi=10.1088/0004-637X/805/2/130 | volume=805 | issue=2 | pages=130 | s2cid=118267222 }} | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| Tucana II | 0.33 | 70 | −3.9 | dSph | 2015 | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| Pisces Overdensity | 1.5 | 80 | −13 | dSph? | 2009 | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| DES 1 | 0.02 | 82 | −3.05 | dSph? | title=Digging deeper into Southern skies: A compact Milky Way companion discovered in first-year Dark Energy Survey data | author1=Luque, E. | display-authors=etal | journal=Monthly Notices of the Royal Astronomical Society | volume=458 | issue=1 | pages=603–612 | doi=10.1093/mnras/stw302 | date=9 February 2016 | doi-access=free | arxiv=1508.02381 | bibcode=2016MNRAS.458..603L}} | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| Eridanus III | 0.028 | 90 | −2.4 | dSph? | 2015 | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| Horologium I | 0.06 | 100 | −3.5 | dSph? | 2015 | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| Kim 2/Indus I | 0.074 | 100 | −3.5 | GC/dSph | 2015 | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| Phoenix II | 0.0521 | 100 | −3.7 | dSph? | 2015 | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| Ursa Major I Dwarf | 0.64 | 100 | −5.5 | dG Sph | 2005 | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| Pictoris I | 0.058 | 115 | −3.7 | dSph? | 2015 | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| Grus I | 0.12 | 120 | −3.4 | dSph | 2015 | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| Pegasus IV | 0.082 | 90 | −4.25 | dSph | arxiv=2203.11788 | doi=10.3847/1538-4357/aca1c3 | title=Pegasus IV: Discovery and Spectroscopic Confirmation of an Ultra-faint Dwarf Galaxy in the Constellation Pegasus | year=2023 | last1=Cerny | first1=W. | last2=Simon | first2=J. D. | last3=Li | first3=T. S. | last4=Drlica-Wagner | first4=A. | last5=Pace | first5=A. B. | last6=Martínez-Vázquez | first6=C. E. | last7=Riley | first7=A. H. | last8=Mutlu-Pakdil | first8=B. | last9=Mau | first9=S. | last10=Ferguson | first10=P. S. | last11=Erkal | first11=D. | last12=Munoz | first12=R. R. | last13=Bom | first13=C. R. | last14=Carlin | first14=J. L. | last15=Carollo | first15=D. | last16=Choi | first16=Y. | last17=Ji | first17=A. P. | last18=Manwadkar | first18=V. | last19=Martínez-Delgado | first19=D. | last20=Miller | first20=A. E. | last21=Noël | first21=N. E. D. | last22=Sakowska | first22=J. D. | last23=Sand | first23=D. J. | last24=Stringfellow | first24=G. S. | last25=Tollerud | first25=E. J. | last26=Vivas | first26=A. K. | last27=Carballo-Bello | first27=J. A. | last28=Hernandez-Lang | first28=D. | last29=James | first29=D. J. | last30=Nidever | first30=D. L. | journal=The Astrophysical Journal | volume=942 | issue=2 | page=111 | bibcode=2023ApJ...942..111C | s2cid=247597301 | display-authors=1 | doi-access=free }} |
| Carina II | 0.182 | 36 | −4.5 | dSph | last1=Torrealba | first1=G. | last2=Belokurov | first2=V. | last3=Koposov | first3=S. E. | last4=Bechtol | first4=K. | last5=Drlica-Wagner | first5=A. | last6=Olsen | first6=K. A. G. | last7=Vivas | first7=A. K. | last8=Yanny | first8=B. | last9=Jethwa | first9=P. | date=2018-01-22 | title=Discovery of two neighbouring satellites in the Carina constellation with MagLiteS | journal=Monthly Notices of the Royal Astronomical Society | volume=475 | issue=4 | pages=5085–5097 | doi=10.1093/mnras/sty170 | doi-access=free | arxiv=1801.07279 | df=dmy-all}} | ||||||||||||||||||||||||||||||||||||||||||||
| Carina III | 0.06 | 28 | −2.4 | GC? | 2018 | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| Boötes IV | 0.28 | 209 | −4.53 | dSph | title=Boötes. IV. A new Milky Way satellite discovered in the Subaru Hyper Suprime-Cam Survey and implications for the missing satellite problem | last=Homma | year=2019 | journal=Publications of the Astronomical Society of Japan | volume=71 | issue=5 | page=94 | doi=10.1093/pasj/psz076 | url=https://academic.oup.com/pasj/article-abstract/71/5/94/5539816 | arxiv=1906.07332 | bibcode=2019PASJ...71...94H }} | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| Centaurus I | 0.076 | 116 | −5.55 | dSph | title=Two Ultra-faint Milky Way Stellar Systems Discovered in Early Data from the DECam Local Volume Exploration Survey | last=Mau | year=2020 | journal=The Astrophysical Journal | volume=890 | issue=2 | page=136 | doi=10.3847/1538-4357/ab6c67 | arxiv=1912.03301 | bibcode=2020ApJ...890..136M | s2cid=208857609 | doi-access=free }} | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| Pictor II | 0.046 | 46 | −3.2 | dSph | author=Drlica-Wagner | title=An Ultra-Faint Galaxy Candidate Discovered in Early Data from the Magellanic Satellites Survey | year=2016 | journal=The Astrophysical Journal | volume=833 | issue=1 | pages=L5 | doi=10.3847/2041-8205/833/1/L5 | arxiv=1609.02148 | bibcode=2016ApJ...833L...5D | hdl=1885/153579 | s2cid=56071154 | doi-access=free }} | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| Boötes V | 0.0194 | 102 | −3.2 | dSph? | doi=10.3847/1538-4357/acdd78 | doi-access=free | title=Six More Ultra-faint Milky Way Companions Discovered in the DECam Local Volume Exploration Survey | date=2023 | last1=Cerny | first1=W. | last2=Martínez-Vázquez | first2=C. E. | last3=Drlica-Wagner | first3=A. | last4=Pace | first4=A. B. | last5=Mutlu-Pakdil | first5=B. | last6=Li | first6=T. S. | last7=Riley | first7=A. H. | last8=Crnojević | first8=D. | last9=Bom | first9=C. R. | last10=Carballo-Bello | first10=J. A. | last11=Carlin | first11=J. L. | last12=Chiti | first12=A. | last13=Choi | first13=Y. | last14=Collins | first14=M. L. M. | last15=Darragh-Ford | first15=E. | last16=Ferguson | first16=P. S. | last17=Geha | first17=M. | last18=Martínez-Delgado | first18=D. | last19=Massana | first19=P. | last20=Mau | first20=S. | last21=Medina | first21=G. E. | last22=Muñoz | first22=R. R. | last23=Nadler | first23=E. O. | last24=Noël | first24=N. E. D. | last25=Olsen | first25=K. A. G. | last26=Pieres | first26=A. | last27=Sakowska | first27=J. D. | last28=Simon | first28=J. D. | last29=Stringfellow | first29=G. S. | last30=Tollerud | first30=E. J. | journal=The Astrophysical Journal | volume=953 | issue=1 | page=1 | arxiv=2209.12422 | bibcode=2023ApJ...953....1C | display-authors=1 }} | |
| Leo Minor I | 0.0897 | 82 | −2.4 | dSph | 2022 | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| Virgo II | 0.07 | 72 | −1.6 | dSph | 2022 | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| Willman 1 | 0.02 | 38 | −2.53 | dSph | title=A MegaCam Survey of Outer Halo Satellites. III. Photometric and Structural Parameters | last=Muñoz | year=2018 | journal=The Astrophysical Journal | volume=860 | issue=1 | page=66 | doi=10.3847/1538-4357/aac16b | arxiv=1806.06891 | bibcode=2018ApJ...860...66M | s2cid=118978019 | doi-access=free }} | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| Ursa Major III | 0.003 | 10 | +2.2 | dSph | 2023 | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| Leo K | 0.0087 | 434 | −4.86 | dSph | doi=10.3847/1538-4357/ad429b | doi-access=free | title=Discovery and Characterization of Two Ultrafaint Dwarfs outside the Halo of the Milky Way: Leo M and Leo K | date=2024 | last1=McQuinn | first1=Kristen. B. W. | last2=Mao | first2=Yao-Yuan | last3=Tollerud | first3=Erik J. | last4=Cohen | first4=Roger E. | last5=Shih | first5=David | last6=Buckley | first6=Matthew R. | last7=Dolphin | first7=Andrew E. | journal=The Astrophysical Journal | volume=967 | issue=2 | page=161 | arxiv=2307.08738 | bibcode=2024ApJ...967..161M }} | ||||||||||||||||||||||||||||||||||||||||||||||||
| Leo M | 0.009 | 459 | −5.77 | dSph | 2024 | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| Sextans II | 0.024? | – | – | dSph | author1=Robert Lea | date=2024-07-02 | title=Scientists finally found 2 of the Milky Way's missing satellite galaxies. What could this mean for astronomy? | url=https://www.space.com/milky-way-satellite-dwarf-galaxies-found | access-date=2024-07-04 | website=Space.com | language=en}} | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| Virgo III | 0.015 | 154 | – | dSph | 2024 | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| Pegasus W | 0.01 | 227 | +1 | dSph | 2020 | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| Eridanus IV | 0.034 | 59.7 | +0.2 | dSph? | 2021 | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| Laevens 1 (Crater 1) | 0.09 | 26.8 | +0.8 | dG D | 2014 | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| Leo VI | 0.28 | 111 | −3.56 | dSph | 2024 | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| Aquarius III | 0.102 | 85 | −2.5 | dSph | 2024 |
Map with clickable regions
Image:Satellite_Galaxies.svg|frame|center|Milky Way's satellite galaxies (clickable map)
rect 289 219 352 251 Milky Way rect 319 252 380 281 Sagittarius Dwarf Elliptical Galaxy rect 187 81 229 113 Sextans Dwarf rect 168 273 249 318 Large Magellanic Cloud rect 229 326 288 368 Small Magellanic Cloud rect 297 376 352 407 Sculptor Dwarf rect 183 446 234 476 Fornax Dwarf rect 107 297 150 332 Carina Dwarf rect 296 107 339 144 Bootes Dwarf rect 336 180 408 196 Ursa Major II rect 357 40 423 59 Ursa Major I rect 370 110 428 142 Ursa Minor Dwarf rect 430 119 470 154 Draco Dwarf
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.
Notes
References
References
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- Muñoz. (2018). "A MegaCam Survey of Outer Halo Satellites. III. Photometric and Structural Parameters". The Astrophysical Journal.
- (2024). "Discovery and Characterization of Two Ultrafaint Dwarfs outside the Halo of the Milky Way: Leo M and Leo K". The Astrophysical Journal.
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- (2024). "Discovery of RR Lyrae in the Ultra-faint-dwarf Galaxy Virgo III". The Astronomical Journal.
- (2025). "A Pride of Satellites in the Constellation Leo? Discovery of the Leo VI Milky Way Satellite Ultra-faint Dwarf Galaxy with DELVE Early Data Release 3". The Astrophysical Journal.
- (2025). "Discovery and Spectroscopic Confirmation of Aquarius III: A Low-mass Milky Way Satellite Galaxy". The Astrophysical Journal.
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