The Andromeda Galaxy (M31) has satellite galaxies just like the Milky Way. Orbiting M31 are at least 13 dwarf galaxies: the brightest and largest is M110, which can be seen with a basic telescope. The second-brightest and closest one to M31 is M32. The other galaxies are fainter, and were mostly discovered starting from the 1970s.
On January 11, 2006, it was announced that Andromeda Galaxy's faint companion galaxies lie on or close to a single plane running through the Andromeda Galaxy's center. This unexpected distribution is not obviously understood in the context of current models for galaxy formation. The plane of satellite galaxies points toward a nearby group of galaxies (M81 Group), possibly tracing the large-scale distribution of dark matter.
It is unknown whether the Triangulum Galaxy is a satellite of Andromeda.
Table of known satellites
Andromeda Galaxy's satellites are listed here by discovery (orbital distance is not known). Andromeda IV is not included in the list, as it was discovered to be roughly 10 times further than Andromeda from the Milky Way in 2014, and therefore a completely unrelated galaxy.
Name | Type | Distance from Sun (million ly) |
Right Ascension** | Declination** | Absolute Magnitude | Apparent magnitude | Mass-to-light ratio | 3D distance to M31 (kly) | Year discovered |
Notes |
---|---|---|---|---|---|---|---|---|---|---|
M32 | dE2 | 2.48 | 00 42 41.877 | +40° 51′ 54.71″ | +8.1 | 1749 | ||||
M110 | dE6 | 2.69 | 00 40 22.054 | +41° 41′ 08.04″ | −16.5 | +8.5 | 1773 | |||
NGC 185 | dE5 | 2.01 | 00 38 57.523 | +48° 20′ 14.86″ | +10.1 | 1787 | ||||
NGC 147 | dE5 | 2.2 | 00 33 12.131 | +48° 30′ 32.82″ | +10.5 | 1829 | ||||
Andromeda I | dSph | 2.43 | 00 45 39.264 | +38° 02′ 35.17″ | −11.8 | +13.6 | 31 ± 6 | 1970 | ||
Andromeda II*** | dSph | 2.13 | 01 16 28.136 | +33° 25′ 50.36″ | −12.6 | +13.5 | 13 ± 3 | 1970 | ||
Andromeda III | dSph | 2.44 | 00 35 31.777 | +36° 30′ 04.19″ | −10.2 | +15.0 | 19 ± 12 | 1970 | ||
Andromeda V | dSph | 2.52 | 01 10 16.952 | +47° 37′ 40.12″ | −9.6 | +15.9 | 78 ± 50 | 1998 | ||
Pegasus Dwarf Spheroidal (Andromeda VI) |
dSph | 2.55 | 23 51 46.516 | +24° 34′ 55.69″ | −11.5 | +14.2 | 12 ± 5 | 1998 | ||
Cassiopeia Dwarf (Andromeda VII) |
dSph | 2.49 | 23 26 33.321 | +50° 40′ 49.98″ | −13.3 | +12.9 | 7.1 ± 2.8 | 1998 | ||
Andromeda VIII | dSph | 2.7 | 00 42 06 | +40° 37′ 00″ | +9.1 | 2003 | Tidally disrupting; identification unclear | |||
Andromeda IX | dSph | 2.5 | 00 52 52.493 | +43° 11′ 55.66″ | −8.3 | +16.2 | 127.2 | 2004 | ||
Andromeda X | dSph | 2.9 | 01 06 34.740 | +44° 48′ 23.31″ | −8.1 | +16.1 | 63 ± 40 | 332.7 | 2005 | |
Andromeda XI | dSph | 00 46 20 | +33° 48′ 05″ | −7.3 | 2006 | |||||
Andromeda XII | dSph | 00 47 27 | +33° 22′ 29″ | −6.4 | 2006 | |||||
Andromeda XIII (Pisces III) | dSph | 00 51 49.555 | +33° 00′ 31.40″ | −6.9 | 2006 | |||||
Andromeda XIV (Pisces IV) | dSph | 00 41 35.219 | +29° 41′ 45.87″ | −8.3 | 102 ± 71 | 2007 | ||||
Andromeda XV | dSph | 01 14 18.7 | +38° 07′ 02.9″ | −9.4 | 2007 | |||||
Andromeda XVI (Pisces V) | dSph | 2.143 | 00 59 29.843 | +32° 22′ 27.96″ | −9.2 | 580.6 | 2007 | |||
Andromeda XVII | dSph | 00 37 07 | +44° 19′ 20″ | −8.5 | 313.1 | 2008 | ||||
Andromeda XVIII | dSph/Sm | 00 02 15.184 | +45° 05′ 19.78″ | 515.3 | 2008 | |||||
Andromeda XIX | dSph | 00 19 32.1 | +35° 02′ 37.1″ | −9.3 | 2008 | |||||
Andromeda XX | dSph | 00 07 30.530 | +35° 07′ 45.94″ | −6.3 | 512.1 | 2008 | ||||
Andromeda XXI | dSph | 23 54 47.7 | +42° 28′ 15″ | −9.9 | 472.9 | 2009 | ||||
Andromeda XXII | dSph | 00 27 40 | +28° 05′ 25″ | −7.0 | 910 | 2009 | ||||
Andromeda XXIII | dIrr | 01 29 21.944 | +38° 43′ 05.97″ | 427.3 | 2011 | |||||
Andromeda XXIV | 01 18 30 | +46° 21′ 58″ | 401.2 | 2011 | ||||||
Andromeda XXV | 00 30 08.9 | +46° 51′ 07″ | 319.6 | 2011 | ||||||
Andromeda XXVI | 00 23 45.6 | +47° 54′ 58″ | 489.2 | 2011 | ||||||
Andromeda XXVII | 00 37 27.1 | +45° 23′ 13″ | 2011 | Tidally disrupted | ||||||
Andromeda XXVIII | dSph | 22 32 41.449 | +31° 12′ 59.10″ | −8.8 | 2011 | |||||
Andromeda XXIX | dIrr | 23 58 55.440 | +30° 45′ 22.09″ | 636 | 2011 | |||||
Andromeda XXX (Cassiopeia II) | dSph? | 00 36 34.9 | +49° 38′ 48″ | |||||||
Andromeda XXXI (Lacerta I) | dSph? | 22 58 16.3 | +41° 17′ 28″ | 2013 | ||||||
Andromeda XXXII (Cassiopeia III) | dSph? | 2.74 | 00 35 59.4 | +51° 33′ 35″ | 508 | 2013 | ||||
Andromeda XXXIII (Perseus I) | dSph? | 2.41 | 03 01 23.6 | +40° 59′ 18″ | 1,140 | 2013 | ||||
Tidal Stream Northwest (Tidal Stream E and F) |
00 20 00 | +46° 00′ 00″ | 2009 | |||||||
Tidal Stream Southwest | 00 30 00 | +37° 30′ 00″ | 2009 | |||||||
Pegasus V galaxy (Peg V) | d | 682 kpc (2.22 Mly) | 23 18 27.8±0.1 | +33° 21′ 32″±3 | −6.3 | 245 kpc (800 kly) | 2022 | |||
Triangulum Galaxy* (M33) |
SA(s)cd | 2.59 | 01 33 50.883 | +30° 39′ 36.54″ | +6.27 | 1654? | It is around 750000 light years from Andromeda. Its relation to Andromeda is uncertain. |
It is uncertain whether it is a companion galaxy of the Andromeda Galaxy.
RA/DEC values marked in Italics are rough estimates.
Martin et al. (2009) gave aliases to several satellite galaxies of the Andromeda Galaxy that are located in Pisces. However, the name Pisces II was later used for a different galaxy that is a satellite of the Milky Way, so it is not used here.
See also
References
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- ^ Collins, M. L. M.; Chapman, S. C.; Rich, R. M.; Irwin, M. J.; Peñarrubia, J.; Ibata, R. A.; Arimoto, N.; Brooks, A. M.; Ferguson, A. M. N.; Lewis, G. F.; McConnachie, A. W.; Venn, K. (2011). "The scatter about the 'Universal' dwarf spheroidal mass profile: A kinematic study of the M31 satellites and V and VI". Monthly Notices of the Royal Astronomical Society. 417 (2): 1170. arXiv:1103.2121. Bibcode:2011MNRAS.417.1170C. doi:10.1111/j.1365-2966.2011.19342.x. S2CID 6345715.
- ^ Martin, N. F.; Ibata, R. A.; Irwin, M. J.; Chapman, S.; Lewis, G. F.; Ferguson, A. M. N.; Tanvir, N.; McConnachie, A. W. (2006). "Discovery and analysis of three faint dwarf galaxies and a globular cluster in the outer halo of the Andromeda galaxy". Monthly Notices of the Royal Astronomical Society. 371 (4): 1983–1991. arXiv:astro-ph/0607472. Bibcode:2006MNRAS.371.1983M. doi:10.1111/j.1365-2966.2006.10823.x. S2CID 20171599.
- ^ Discovery of the Local Group Galaxies
- Monelli, Matteo; Martínez-Vázquez, Clara E.; Bernard, Edouard J.; Gallart, Carme; Skillman, Evan D.; Weisz, Daniel R.; Dolphin, Andrew E.; Hidalgo, Sebastian L.; Cole, Andrew A.; Martin, Nicolas F.; Aparicio, Antonio; Cassisi, Santi; Boylan-Kolchin, Michael; Mayer, Lucio; McConnachie, Alan; McQuinn, Kristen B. W.; Navarro, Julio F. (2016). "The Islands Project. I. Andromeda Xvi, an Extremely Low Mass Galaxy Not Quenched by Reionization". The Astrophysical Journal. 819 (2): 147. arXiv:1603.00625. Bibcode:2016ApJ...819..147M. doi:10.3847/0004-637X/819/2/147. S2CID 32263075.
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- ^ Moore, Nicole Casal (7 Nov 2011), "Newly found dwarf galaxies could help reveal the nature of dark matter", News Service, University of Michigan, retrieved 10 Dec 2011 (reprinted in R&D Magazine)
- Fu, Sal Wanying; Weisz, Daniel R.; Starkenburg, Else; Martin, Nicolas; Collins, Michelle L. M.; Savino, Alessandro; Boylan-Kolchin, Michael; Côté, Patrick; Dolphin, Andrew E.; Longeard, Nicolas; Mateo, Mario L.; Mercado, Francisco J.; Sandford, Nathan R.; Skillman, Evan D. (2024). "Stellar Metallicities and Gradients in the Faint M31 Satellites Andromeda XVI and Andromeda XXVIII". The Astrophysical Journal. 975 (1): 2. arXiv:2407.04698. Bibcode:2024ApJ...975....2F. doi:10.3847/1538-4357/ad76a2.
- ^ McConnachie, Alan W. (2012). "The observed properties of dwarf galaxies in and around the Local Group". The Astronomical Journal. 144 (1): 4. arXiv:1204.1562. Bibcode:2012AJ....144....4M. doi:10.1088/0004-6256/144/1/4. S2CID 118515618.
- ^ Rhode, Katherine L.; Smith, Nicholas J.; Crnojevic, Denija; Sand, David J.; Lambert, Ryan A.; Vesperini, Enrico; Smith, Madison V.; Janowiecki, Steven; Salzer, John J.; Karunakaran, Ananthan; Spekkens, Kristine (2023). "Exploring the Structures and Substructures of the Andromeda Satellite Dwarf Galaxies Cassiopeia III, Perseus I, and Lacerta I". The Astronomical Journal. 166 (5): 180. arXiv:2309.01045. Bibcode:2023AJ....166..180R. doi:10.3847/1538-3881/acf859.
- ^ New tidal streams found in Andromeda reveal history of galactic mergers
- "Pegasus V: New Ultra-Faint Dwarf Galaxy Spotted in Outskirts of Andromeda". Sci-News. 1 July 2022.
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- "Messier Object 33". www.messier.seds.org. Retrieved 2021-05-21.
- Martin, Nicolas F.; McConnachie, Alan W.; Irwin, Mike; Widrow, Lawrence M.; Ferguson, Annette M. N.; Ibata, Rodrigo A.; Dubinski, John; Babul, Arif; et al. (1 November 2009). "PAndAS' CUBS: Discovery of Two New Dwarf Galaxies in the Surroundings of the Andromeda and Triangulum Galaxies". The Astrophysical Journal. 705 (1): 758–765. arXiv:0909.0399. Bibcode:2009ApJ...705..758M. doi:10.1088/0004-637X/705/1/758. S2CID 15277245.
- Belokurov, V.; Walker, M. G.; Evans, N. W.; Gilmore, G.; Irwin, M. J.; Just, D.; Koposov, S.; Mateo, M.; Olszewski, E.; Watkins, L.; Wyrzykowski, L. (2010). "Big Fish, Little Fish: Two New Ultra-Faint Satellites of the Milky Way". The Astrophysical Journal. 712 (1): L103–L106. arXiv:1002.0504. Bibcode:2010ApJ...712L.103B. doi:10.1088/2041-8205/712/1/L103. S2CID 29195107.
External links
- Andromeda's thin sheet of satellites – Dark matter filiments or galaxtic cannibalism?
- Strange Setup: Andromeda's Satellite Galaxies All Lined Up
Andromeda Galaxy | ||
---|---|---|
Location | Andromeda Galaxy → Andromeda subgroup →
Local Group → Local Sheet → Virgo Supercluster → Laniakea Supercluster → Local Hole → Observable universe → Universe Each → may be read as "within" or "part of". | |
Satellite galaxies |
*It is uncertain whether these are companion galaxies of the Andromeda Galaxy | |
Catalogued stars | ||
Other | ||