From Wikipedia, the free encyclopedia
A member of the Local Group of galaxies, irregular galaxy
Sextans A is 4.3 million
light-years distant. The bright Milky Way foreground stars appear
yellowish in this view. Beyond them lie the stars of Sextans A with
young blue star clusters clearly visible.
Distribution of the
iron content
(in logarithmic scale) in four dwarf neighbouring galaxies of the
Milky Way.
The Local Group is the group of galaxies that includes our galaxy,
the Milky Way. The group
comprises about 30 galaxies (including dwarf galaxies),
with its gravitational center located somewhere between the Milky
Way and the Andromeda Galaxy. The galaxies of the
Local Group cover a 10 million light-year diameter (see 1 E+22
m for distance comparisons) and have a binary (dumbbell)[1]
shape. The group is estimated to have a total mass of (1.29 ±
0.14) × 1012M☉.[1]
The group itself is one of many within the Virgo
Supercluster (i.e. the Local Supercluster).[2]
The two most massive members of the group are the Milky Way and the Andromeda
Galaxy. These two Spiral Galaxies
each have a system of satellite galaxies.
- The Milky Way's satellite system
consists of Sagittarius Dwarf
Galaxy, Large Magellanic Cloud, Small
Magellanic Cloud, Canis Major Dwarf, Ursa Minor
Dwarf, Draco
Dwarf, Carina
Dwarf, Sextans Dwarf, Sculptor Dwarf, Fornax Dwarf, Leo
I, Leo II, and Ursa Major
Dwarf.
- Andromeda's satellite system
comprises M32, M110, NGC 147, NGC 185, And I, And II, And III, And IV, And V, Pegasus dSph, Cassiopeia
Dwarf, And
VIII, And IX,
and And
X.
- The Triangulum Galaxy, the third largest
and only other ordinary spiral galaxy in the Local Group, may or
may not be a companion to the Andromeda galaxy but probably has Pisces Dwarf as a
satellite.
The other members of the group are gravitationally secluded from
these large subgroups: IC10, IC1613, Phoenix Dwarf, Leo A, Tucana Dwarf, Cetus Dwarf, Pegasus Dwarf Irregular, Wolf-Lundmark-Melotte, Aquarius Dwarf,
and Sagittarius Dwarf Irregular.
History
The term "The Local Group" was introduced by Edwin Hubble in
Chapter VI of his book The Realm of the Nebulae (Hubble
1936, pp. 124–151). There he describes it as "a typical
small group of nebulae which is isolated in the general
field." In that book he delineated by decreasing luminosity
its members to be M31, the Milky Way, M33, the Large Magellanic Cloud, the Small
Magellanic Cloud, M32, NGC 205, NGC 6822, NGC 185, IC
1613 and NGC 147. He
also identified IC 10 as a
possible Local Group member. In the ~70 years since his work, the
number of known Local Group members has increased from his initial
twelve to thirty-six as of 2003, by way of the discovery of almost
two dozen low-luminosity galaxies.[3]
Component
galaxies
Maps
Local group (clickable map)
Galactic
bodies
Other
notable objects
Diagram
See also
References
- ^ a
b
Karachentsev, I. D.; Kashibadze, O.
G. (2006). "Masses of the local group
and of the M81 group estimated from distortions in the local
velocity field". Astrophysics 49 (1):
3–18. doi:10.1007/s10511-006-0002-6. http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2006Ap.....49....3K.
- ^ R. B. Tully (1982). "The Local Supercluster".
Astrophysical Journal 257: 389–422. doi:10.1086/159999. http://adsabs.harvard.edu/abs/1982ApJ...257..389T.
- ^ van den Bergh, Sidney (May 2003), "History of the Local
Group", To be published in: "The Local Group as an
Astrophysical Laboratory" (Cambridge University Press), http://adsabs.harvard.edu/abs/2003astro.ph..5042V
- ^
"Milky Way 'bigger than
thought'". BBC News. 2009-01-06. http://news.bbc.co.uk/2/hi/science/nature/7813635.stm.
- ^ van den Bergh, Sidney (April 2000), "Updated Information on the
Local Group", The Publications of the Astronomical Society
of the Pacific 112 (770): 529–536, doi:10.1086/316548, http://adsabs.harvard.edu/cgi-bin/nph-bib_query?bibcode=2000PASP..112..529V
- ^ Wakker, B. P. (2008). "Distances to
Galactic High‐Velocity Clouds. I. Cohen Stream, Complex GCP, Cloud
g1". The Astrophysical Journal 672: 298.
doi:10.1086/523845.
- ^
"Massive Gas Cloud Speeding
Toward Collision With Milky Way". http://www.nrao.edu/pr/2008/smithscloud/. Retrieved
2008-06-06.
External
links