List of satellite galaxies of Andromeda
The Andromeda galaxy M31 has just like our home galaxy, the Milky Way and satellite galaxies. At least 37 galaxies are currently known, including Andromeda, which together form the Andromeda subgroup of the Local Group .
Among them are also galaxies like the elliptical galaxy M32 , which can already be seen with smaller hobby telescopes . The second brightest galaxy right next to it is M 110. NGC 185 was discovered on November 30, 1787 by Friedrich Wilhelm Herschel , the dwarf galaxy NGC 147 by his son John Frederick William Herschel on September 8, 1829.
The other galaxies are dwarf galaxies, clearly fainter, and were only discovered through photographic and later CCD images.
Current measurement results from 2006 now show that the faint satellite galaxies of Andromeda are in or near a plane through the center of their central galaxy. This unexpected result of the distribution raises a number of questions about the current approaches to the models of galaxy formation . The distribution plane points in the direction of a nearby galaxy group of the M81 group , which could possibly provide an indication of the large-scale distribution of dark matter .
Table of known satellites
![](https://upload.wikimedia.org/wikipedia/commons/thumb/2/2c/M33.jpg/220px-M33.jpg)
The satellites of the Andromeda Galaxy (M31) sorted by year of discovery.
Surname | Type | Distance to the sun (million light years ) |
Apparent brightness | Year of discovery |
Alternative name (s) | annotation |
---|---|---|---|---|---|---|
Triangle galaxy | SA (s) cd | 2.8 ± 0.8 | 6.27 | 1654 | M33, NGC 598, Triangulum Nebula | |
M32 | dE2 | 2.48 | 9.2 | 1749 | NGC 221, Andro-Beta | |
M110 | dE6 | 2.69 | 9.4 | 1773 | NGC 205, Andro-Alpha | |
NGC 185 | dE5 | 2.01 | 11 | 1787 | ||
NGC 147 | dE5 | 2.2 | 12 | 1829 | ||
Peg dig | dIm | 3.0 | 13.2 | 1950 | ||
Andromeda I | dSph | 2.43 | 13.2 | 1970 | ||
Andromeda II | dSph | 2.13 | 13 | 1970 | ||
Andromeda III | dSph | 2.44 | 10.3 | 1970 | ||
Andromeda IV | dIm | 21 ± 5 | 16.6 B | 1972 | Belonging to the Andromeda subgroup unclear | |
LGS 3 | dIm / dSph | 2.52 ± 0.07 | 14.3 | 1978 | Pisces dwarf galaxy | |
Andromeda V | dSph | 2.52 | 15.4 | 1998 | ||
Pegasus ii | dSph | 2.55 | 14.5 | 1998 | Andromeda VI, Peg dSph | |
Cassiopeia dwarf galaxy | dSph | 2.58 | 12.9 | 1998 | Andromeda VII | |
Andromeda VIII | dSph | 2.7 | 9.1 | 2003 | ||
Andromeda IX | dSph | 2.5 | 16.2 | 2004 | ||
Andromeda X | dSph | 2.9 | 16.1 ± 0.5 | 2005 | ||
Andromeda XI | dSph | 2.6 ± 0.2 | 17.2 ± 0.5 | 2006 | ||
Andromeda XII | dSph | 2.8 ± 0.1 | 16.3 ± 1.0 | 2006 | ||
Andromeda XIII | dSph | 2.92 ± 0.07 | 16.8 ± 1.0 | 2006 | ||
Andromeda XIV | dSph | 2.4 ± 0.5 | 2007 | |||
Andromeda XV | dSph | 2.3 ± 0.3 | 2007 | |||
Andromeda XVI | dSph | 1.72 ± 0.16 | 2007 | |||
Andromeda XVII | dSph | 2.58 ± 0.13 | 16.0 | 2008 | ||
Andromeda XVIII | dSph | 4.42 ± 0.29 | 16.0 | 2008 | ||
Andromeda XIX | dSph | 3.04 ± 0.20 | 15.6 ± 0.6 | 2008 | ||
Andromeda XX | dSph | 2.6 ± 0.7 | 18.2 ± 0.8 | 2008 | ||
Andromeda XXI | dSph | 2.80 ± 0.17 | 14.0 ± 0.6 | 2009 | ||
Andromeda XXII | dSph | 3.0 ± 0.4 | 18.0 ± 0.8 | 2009 | ||
Andromeda XXIII | dSph | 2.50 ± 0.14 | 14.2 ± 0.5 | 2011 | ||
Andromeda XXIV | dSph | 1.96 ± 0.11 | 16.3 ± 0.5 | 2011 | ||
Andromeda XXV | dSph | 2.65 ± 0.15 | 14.9 ± 0.5 | 2011 | ||
Andromeda XXVI | dSph | 2.48 ± 0.14 | 17.3 ± 0.5 | 2011 | ||
Andromeda XXVII | dSph | 2.47 ± 0.15 | 16.7 ± 0.5 | 2011 | ||
Andromeda XXVIII | dSph | 2.12 ± 0.38 | 15.6 ± 0.7 | 2011 | ||
Andromeda XXIX | dSph | 2.38 ± 0.24 | 16.3 ± 0.4 | 2011 | ||
Andromeda XXX | dSph | 2.22 ± 0.10 | 2012 | |||
Andromeda XXXI | dSph | 2.52 +0.20 −0.18 | 12.7 ± 0.7 | 2013 | Lacerta I | |
Andromeda XXXII | dSph | 2.46 +0.14 -0.09 | 12.2 ± 0.7 | 2013 | Cassiopeia III | |
Andromeda XXXIII | dSph | 2.56 ± 0.21 | 14.2 ± 0.2 | 2013 | Perseus I |
Tidal star currents
Surname | Type | Distance to the sun (million light years ) |
Apparent brightness | Year of discovery |
Alternative name (s) | annotation |
---|---|---|---|---|---|---|
Tidal Stream Northwest | 2009 | Tidal Stream E and F | ||||
Tidal Stream Southwest | 2009 |
Interaction with Andromeda
New images of the Spitzer Space Telescope of NASA shed light on the past, violent evolution of Andromeda. They show that a few million years ago one of the satellite galaxies, the elliptical galaxy M32, broke through one of the spiral arms of Andromeda. Infrared images showed on the one hand that the two spiral arms and the ring protruding from the formation of stars are separate structures, on the other hand this ring has a hole in its center where M32 pierced the disk of the Andromeda Galaxy.
Galaxy types
- dIm: Irregular dwarf galaxy (dwarf irregular galaxy)
- dE: dwarf elliptical galaxy
- dSph: Spheroid dwarf galaxy (dwarf spheroidal galaxy)
- SA (s) cd: open spiral galaxy without a ring
additional
Web links
- Andromeda's thin sheet of satellites - Dark matter filaments or galactic cannibalism?
- Strange Setup: Andromeda's Satellite Galaxies All Lined Up
Individual evidence
- ↑ a b c N. F. Martin, et al .: Discovery and analysis of three faint dwarf galaxies and a globular cluster in the outer halo of the Andromeda galaxy , 2006, arxiv : astro-ph / 0607472 .
- ↑ a b c d e f g h i j k l NASA / IPAC EXTRAGALACTIC DATABASE
- ↑ a b c d e f g h i j k l m n o p q r Discovery of the Local Group Galaxies
- ↑ a b
- ↑ a b c d e f g h i Jenny C. Richardson, Mike Irwin, Alan W. McConnachie, Nicolas F. Martin, Aaron Dotter, Annette MN Ferguson, Rodrigo A. Ibata, Scott Chapman, Geraint F. Lewis, Nial R Tanvir, R. Michael Rich: PAndAS 'progeny: extending the M31 dwarf galaxy cabal . In: Cosmology and Nongalactic Astrophysics . February 14, 2011. arxiv : 1102.2902 .
- ↑ a b Nicole Casal Moore: Newly found dwarf galaxies could help reveal the nature of dark matter . In: University of Michigan (Ed.): News Service . November 7, 2011. Retrieved December 10, 2011. ( reprinted in R&D Magazine )
- ↑ Colin T. Slater, Eric F. Bell, Nicolas F. Martin: Andromeda XXVIII: A Dwarf Galaxy More Than 350 kpc from Andromeda . In: Cornell University . October 26, 2011. arxiv : 1110.5903 .
- ↑ Eric F. Bell, Colin T. Slater (University of Michigan), Nicolas F. Martin (MPIA Heidelberg): Andromeda XXIX: A New Dwarf Spheroidal Galaxy 200kpc from Andromeda . In: Cornell University . October 26, 2011. arxiv : 1110.5906 .
- ↑ a b LACERTA I AND CASSIOPEIA III: TWO LUMINOUS AND DISTANT ANDROMEDA SATELLITE DWARF GALAXIES FOUND IN THE 3π PAN-STARRS1 SURVEY
- ↑ PERSEUS I: A DISTANT SATELLITE DWARF GALAXY OF ANDROMEDA
- ↑ a b New tidal streams found in Andromeda reveal history of galactic mergers