M81 Group
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The M81 Group is a
galaxy group A galaxy group or group of galaxies (GrG) is an aggregation of galaxies comprising about 50 or fewer gravitationally bound members, each at least as luminous as the Milky Way (about 1010 times the luminosity of the Sun); collections of galaxi ...
in the
constellation A constellation is an area on the celestial sphere in which a group of visible stars forms Asterism (astronomy), a perceived pattern or outline, typically representing an animal, mythological subject, or inanimate object. The first constellati ...
s
Ursa Major Ursa Major, also known as the Great Bear, is a constellation in the Northern Sky, whose associated mythology likely dates back into prehistory. Its Latin name means "greater (or larger) bear", referring to and contrasting it with nearby Ursa M ...
and
Camelopardalis Camelopardalis is a large but faint constellation of the northern sky representing a giraffe. The constellation was introduced in 1612 or 1613 by Petrus Plancius. Some older astronomy books give Camelopardalus or Camelopardus as alternative form ...
that includes the galaxies
Messier 81 Messier 81 (also known as NGC 3031 or Bode's Galaxy) is a grand design spiral galaxy about 1 E22 m, 12 million light-years away in the constellation Ursa Major. It has a Galaxy#Isophotal diameter, D25 isophotal diameter of . Because of its rela ...
and
Messier 82 Messier 82 (also known as NGC 3034, Cigar Galaxy or M82) is a starburst galaxy approximately 12 million light-years away in the constellation Ursa Major. It is the second-largest member of the M81 Group, with the D25 isophotal diameter of . ...
, as well as several other galaxies with high apparent brightnesses. The approximate center of the group is located at a distance of 3.6 Mpc, making it one of the nearest groups to the
Local Group The Local Group is the galaxy group that includes the Milky Way, where Earth is located. It has a total diameter of roughly , and a total mass of the order of . It consists of two collections of galaxies in a " dumbbell" shape; the Milky Way ...
. The group is estimated to have a total mass of (1.03 ± 0.17). The M81 Group, the Local Group, and other nearby groups all lie within the
Virgo Supercluster The Local Supercluster (LSC or LS), or Virgo Supercluster is a formerly defined supercluster containing the Virgo Cluster and Local Group, which itself contains the Milky Way and Andromeda galaxies, as well as others. At least 100 galaxy group ...
(i.e. the Local Supercluster).


Members

The table below lists galaxies that have been identified as associated with the M81 Group by I. D. Karachentsev. Note that the object names used in the above table differ from the names used by Karachentsev.
NGC NGC may refer to: Companies * NGC Corporation, the name of US electric company Dynegy, Inc. from 1995 to 1998 * National Gas Company of Trinidad and Tobago, a state-owned natural gas company in Trinidad and Tobago * National Grid plc, a former nam ...
, IC, UGC, and PGC numbers have been used in many cases to allow for easier referencing.


Interactions within the group

Messier 81, Messier 82, and NGC 3077 are all strongly interacting with each other. Observations of the 21-centimeter
hydrogen line The hydrogen line, 21 centimeter line, or H I line is a spectral line that is created by a change in the energy state of solitary, electrically neutral hydrogen atoms. It is produced by a spin-flip transition, which means the dire ...
indicate how the galaxies are connected. The gravitational interactions have stripped some
hydrogen Hydrogen is a chemical element; it has chemical symbol, symbol H and atomic number 1. It is the lightest and abundance of the chemical elements, most abundant chemical element in the universe, constituting about 75% of all baryon, normal matter ...
gas away from all three galaxies, leading to the formation of filamentary gas structures within the group. Bridges of neutral hydrogen have been shown to connect M81 with M82 and NGC 3077. Moreover, the interactions have also caused some
interstellar gas The interstellar medium (ISM) is the matter and radiation that exists in the space between the star systems in a galaxy. This matter includes gas in ionic, atomic, and molecular form, as well as dust and cosmic rays. It fills interstellar spac ...
to fall into the centers of Messier 82 and NGC 3077, which has led to strong starburst activity (or the formation of many stars) within the centers of these two galaxies. Computer simulations of
tidal interactions The tidal force or tide-generating force is the difference in gravitational attraction between different points in a gravitational field, causing bodies to be pulled unevenly and as a result are being stretched towards the attraction. It is the d ...
have been used to show how the current structure of the group could have been created.


Gallery

The mysteries of UGC 8201.jpg, Galaxy UGC 8201 is a dwarf irregular galaxy member of the M81 galaxy group. M81+M82-and other galaxies.jpg, Amateur picture
Messier 81 Messier 81 (also known as NGC 3031 or Bode's Galaxy) is a grand design spiral galaxy about 1 E22 m, 12 million light-years away in the constellation Ursa Major. It has a Galaxy#Isophotal diameter, D25 isophotal diameter of . Because of its rela ...
+ 82 and NGC 3077 all of the M81 group, 33 frames stacked of 1 minute each. Image:M81m82 galex f.jpg, The spiral galaxies Messier 81 and 82 and the dwarf galaxy Holmberg IX from GALEX Image:M81 wide Galex.jpg, Close up view of Messier 81 from GALEX Image:Messier81 highres.jpg, The spiral galaxy Messier 81 from Spitzer Space Telescope Image:Ssc2003-06c.jpg, The spiral galaxy Messier 81 from Spitzer Space Telescope Image:M82 HST ACS 2006-14-a-large web.jpg, Starburst galaxy Messier 82 from Hubble Space Telescope Image:NGC2403 3.6 5.8 8.0 microns spitzer.png, NGC 2403 in mid-infrared view, combining the 3.6, 5.8 and 8.0 μm bands of the Spitzer Space Telescope Image:NGC2403 3.6 8.0 24 microns spitzer.png, NGC 2403 in Mid-infrared view, combining the 3.6, 8.0 and 24 μm bands of the Spitzer Space Telescope Image:NGC 2403HST.jpg, NGC 2403 from Hubble Space Telescope Image:NGC 2403HSTSN.jpg, NGC 2403 from Hubble Space Telescope illustrated Image:Galaxy-NGC-2403-with-SN2004DJ.jpeg, Supernova SN2004DJ in the spiral galaxy NGC 2403 Image:NGC2403-SN2004dj.jpg, Supernova 2004dj in NGC 2403 Image:NGC 4236 I FUV g2006.jpg, NGC 4236 from GALEX Image:NGC 2366HST.jpg, NGC 2366 from Hubble Space Telescope Image:NGC 2976SSTFull.jpg, Galaxy NGC 2976 from Spitzer Space Telescope in infrared Image:NGC2976.jpg, Galaxy NGC 2976 from an amateur Astronomer Image:NGC 4605 GALEX WikiSky.jpg, Galaxy NGC 4605 from GALEX Image:Ngc2363HST.jpg, NGC 2363 from Hubble Space Telescope Image:NGC 2537 I FUV g2006.jpeg, NGC 2537 from GALEX Image:Holmberg IISST.jpg, Holmberg II from Spitzer Space Telescope in infrared Image:M81DwarBSST.jpg, UGC 5423 / M81 dwarf B from Spitzer Space Telescope in infrared Image:NGC 3077 2MASS.jpg, NGC 3077 from 2MASS Image:IC 2574 Hubble WikiSky.jpg, IC 2574


See also

* UGC 5497


References


External links


M81 Group @ SEDS


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