Local galaxy group

[běn xīng xì qún]
A typical open galaxy cluster
Collection
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book Galaxy Local Group of Galaxies Galaxy And adjacent Andromeda galaxy Magellanic Clouds 50 galaxies formed a smaller group, including the Milky Way. All galaxies in the Local Group of Galaxies cover an area about 10 million light-years in diameter. The local galaxy group belongs to the larger Virgo supercluster [1]
Chinese name
Local galaxy group
Foreign name
Local Group of Galaxies
Local Group
Alias
Local Group
leading member
Galaxy Andromeda galaxy Triangle galaxy Magellanic Clouds M32 and M110 And dozens of other galaxies

Introduction to galaxies

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Local galaxy group
The Local Group of Galaxies is a typical Open galaxy cluster There is no obvious trend of gathering towards the center. Member galaxy About 50. Galaxy and Andromeda galaxy They are the largest two of the member galaxies of the local galaxy group, and they are generally located in the center of the local galaxy group. Except the Milky Way and Andromeda Galaxy, most of the member galaxies are Dwarf galaxy
The radius of the local galaxy group is about one million Second gap With a mass of about 6.5 trillion Solar mass Most of them are concentrated in the Milky Way and Andromeda Galaxy. There is not much gas in the group, accounting for about Total mass 2%.

Subgroup

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The local galaxy group has two subgroups: Galaxy And large and small Magellanic clouds Andromeda galaxy Centric, including M 32 NGC 205 NGC147, NGC185, Fairy Dwarf galaxy and Triangular galaxy (M33). The local galaxy group is Local supercluster A member of.
The so-called local galaxy group refers to the general name of galaxies in space with a radius of about one million seconds (more than 3 million light years), including the Milky Way where the Earth is located. Some people also define the center of the local galaxy group as the Milky Way and Andromeda galaxy (M31). Known local galaxy group Member galaxy And about 50 possible member galaxies. All galaxies in the Local Group of Galaxies cover an area about 10 million light-years in diameter (please refer to 1E23m for a detailed concept of this distance). The local galaxy group belongs to the larger Virgo supercluster

Typical members

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Local Galaxy Group - Triangle Galaxy
The two most massive members of the local galaxy cluster are Galaxy And andromeda Galaxy. these two items. Galaxy And each has its own Satellite galaxy System. The satellite galaxy system of the Milky Way includes Sgr DEG( Sagittarius ), the Large Magellanic Galaxy, the Magellanic Galaxy, Canis Major dwarf galaxy Ursa Minor Dwarf the dragon Dwarf galaxy, Carina dwarf galaxy Sextant dwarf galaxy Sculptor dwarf galaxy Fornax dwarf galaxy , Leo I, Leo II, and Rhododendron dwarf galaxy Andromeda galaxy The satellite galaxy system of M32 M110 , NGC147, NGC185, And I (Andromeda), And II (Andromeda), And III (Andromeda), and And IV (Andromeda). M33 It is the third largest galaxy in the local galaxy group. It may or may not belong to the Andromeda galaxy Companion galaxy But LGS3 may be its satellite galaxy.
The mass of other members of the local galaxy group is far less than that of these large ones subgroup The local galaxy group is a huge open group, and has no tendency to concentrate toward the center. However, members three and five of them are grouped into subgroups, at least with Galaxy and Andromeda galaxy Is the center of two subgroups. The total mass of the local galaxy group is 65600 trillion solar mass, and the sum of the masses of the Milky Way and Andromeda Galaxy accounts for the vast majority.
a little distance Galaxy cluster The spatial distribution of virgo cluster Higher level centered Galaxy clustering Phenomenon, with a size of about 100 million light-years and a length diameter of about 30-75 million seconds, including about 500 galaxy clusters and Galaxy cluster , called Local supercluster The local galaxy group is a member of it.
It is speculated that the main members of the local galaxy group Andromeda galaxy And our Milky Way will soon fall into the destiny of integration. However, since the two galaxies are 2.5 million light-years away, it may take a long time for the two galaxies to merge. But in the distant future, billions of years later, two giant galaxies will merge into one and grow into even larger galaxies. And Andromeda galaxy And our Galaxy Like merging, other galaxies may also be close to each other and merge into one. With the passage of billions of years, all the galaxies in the local galaxy group will merge with each other and eventually form a giant galaxy. The rotational motion of galaxies will gradually disappear with the merger, and eventually a huge Elliptical galaxy

Typical galaxy

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Barred Galaxy
Galaxy -SB type galaxy
Andromeda Galaxy (M31, NGC 224 )-Andromeda Sb type galaxy
Triangle galaxy (M33, NGC 598) - Triangle Sc type galaxy
Elliptical galaxy
M110 (NGC 205) - Andromeda E6p type galaxy
M32 (NGC 221) - Andromeda E2 type galaxy
KKs3 - Hydra E7 type galaxy
Wolf Landmark Melotte (WLM, DDO221) - Ir type galaxy in the constellation Cetus
IC 10 - Cassiopeia KBm or Ir type galaxies
Magellanic nebula (SMC, NGC292) - SB (s) m pec type galaxy in the constellation Rhododendron
Local galaxy group
Pisces dwarf galaxy (LGS3) - Irr type galaxy in Pisces IC1613 (DDO 8) - IAB (s) m V type galaxy in Cetus
Phoenix Dwarf - phoenix Irr type galaxy
Large Magellanic Cloud (LMC) - Irr/SB (s) m type galaxy in Doradus
Leo A (Leo III) - IBm V type galaxy in Leo
Sextant B (DDO 70) - Sextant Ir+IV-V type galaxy
NGC 3109 - hydra Ir+IV-V type galaxy
Sextant base A (DDO 75) - Sextant Ir+V type galaxy
NGC 147 (DDO 3)- Cassiopeia DE5 pec type galaxy
GR 8 (DDO 155) - Im V type galaxy
Sgr DIG ( Sagittarius Short and irregular Dwarf galaxy )-IB (s) m V type galaxy in Sagittarius
NGC 6822 ( Barnard's Galaxy )-IB (s) m Ⅳ - V type galaxy in Sagittarius
Aquarius Dwarf galaxy (DDO 210) - Im V type galaxy in Aquarius
IC 5152 IAB (s) m IV type galaxy in Indian
Pegasus Dwarf galaxy or Pegasus irregular dwarf galaxy (DDO 216) - Irr type galaxy in Pegasus
Globular dwarf galaxy
Cetus Dwarf galaxy -DSph/E4 type galaxy in Cetus
Andromeda III Andromeda dE2 type galaxy
NGC185- Cassiopeia DE3 pec type galaxy
Andromeda I - Andromeda dE3 pec? Type galaxy
Sculptor dwarf galaxy (E351-G30) - dE3 type galaxy in the constellation Yufu
Andromeda V - Andromeda dSph type galaxy
Andromeda II Andromeda dE0 type galaxy
Fornax dwarf galaxy (E356-G04) - dSph/E2 type galaxy in the constellation Fornix
Carina dwarf galaxy (E206-G220)- Ship base DE3 type galaxy
Pump base Dwarf galaxy -DE3 type galaxy of the pump constellation
LEO I (DDO 74) - LEO dE3 type galaxy
Sextant dwarf galaxy -Sextant dE3 type galaxy
LEO II (LEO B) - LEO dE0 pec type galaxy
Ursa Minor Dwarf galaxy - dE4 type galaxy in Ursa Minor
the dragon Dwarf galaxy (DDO 208) - Draco dE0 pec type galaxy
Sag DEG ( Sagittarius Elliptical dwarf galaxy) - dSph/E7 type galaxy in Sagittarius
Rhododendron dwarf galaxy - dE5 type galaxy in Rhododendron
Cassiopeia Dwarf galaxy (Andromeda VII) - Cassiopeia dSph type galaxy
Pegasus Globular dwarf galaxy (Andromeda VI) - dSph type galaxy in Pegasus
UMa dSph -DSph type galaxy in Ursa Major
Galaxies of unspecified type
Andromeda IV - Andromeda Irregular galaxy Or nebula (Irr? Type)
UGC-A 86 (0355+66) - Leopard irregular, elliptical or Lenticular galaxy (Irr, dE or S0 type)
UGC-A 92 (EGB0427+63) - Leopard irregular or lenticular galaxy (Irr or S0 type)
Galaxies that may not be members of the local galaxy group
NGC 404 -Andromeda Oval or Lenticular galaxy (E0 or SA (s) 0-type)
NGC 1569 - Deer and Leopard Irregular galaxy (Irp+Ⅲ - Ⅳ type)
NGC 1560 (IC 2062) - Deer and Leopard spiral galaxy (Sd type)
Deer Leopard A - Deer Leopard irregular galaxy (Irr type)
Ship base Dwarf galaxy -Carina Irregular Galaxy (Irr Type)
2318-42 - Crane Irregular galaxy (Irr type)
UKS 2323-326 - Irregular galaxy in the constellation Yufu (Irr type)
UGC 9128 (DDO 187) - Herdsman Irregular galaxy (Irp+type)
Capricornus The dwarf galaxy (Palomar 12) is a Galaxy Globular clusters, formerly classified as Capricorn Globular galaxy
original UMa dSph (Palomar 4) is a globular cluster of galaxies, previously classified as a globular dwarf galaxy in the constellation Ursa Major
Sextant base C
Local galaxy group
The general name of galaxies in space with a radius of about one million seconds (more than 3 million light years) centered on the Milky Way. Some people also define the center of the local galaxy group as the Milky Way and Andromeda galaxy (M31). There are about 500 known member galaxies and possible member galaxies of the local galaxy group. There are two giant Spiral galaxy (Galaxy and Andromeda), a medium-sized spiral galaxy( Triangular galaxy ), a dwarf Barred spiral galaxy Large Magellanic Cloud ), may also include a lens type Giant galaxy Mafei 1 ), the rest are Dwarf elliptical galaxy and Irregular galaxy
The local galaxy group is a typical open group, and has no tendency to concentrate toward the center. However, the members three and five of them converge into sub groups, and there are at least two sub groups centered on the Milky Way and Andromeda Galaxy. The total mass of the local galaxy group is 650000 trillion times the mass of the sun, and the sum of the masses of the Milky Way and Andromeda Galaxy accounts for most of it. The spatial distribution of close galaxy clusters shows that virgo cluster The cluster phenomenon of higher level galaxies at the center is about 100 million light-years in size and about 30-75 million seconds in length and diameter, including about 500 galaxy clusters and galaxy clusters, called Local supercluster The local galaxy group is a member of it.