Local Group
Adapted from Wikipedia · Discoverer experience
The Local Group is the galaxy group that includes the Milky Way, where our Earth is located. It consists of two collections of galaxies shaped like a "dumbbell". One side has the Milky Way and its smaller galaxies, while the other side has the Andromeda Galaxy and its smaller galaxies. These two collections are about 800 kiloparsecs apart and are moving toward each other.
The Local Group has a total mass of about 2×1012 solar masses and a diameter of about 5.11 megaparsecs. It is part of the larger Local Volume, which is inside the Virgo Supercluster. The exact number of galaxies in the Local Group is not known because the bright Milky Way hides some of them. However, scientists have identified around 134 galaxies within 1 megaparsec of the center. Most of these are small dwarf galaxies.
The two biggest galaxies in the Local Group are the Andromeda Galaxy and the Milky Way. Both are spiral galaxies with masses of about 1012 solar masses each. They each have their own systems of smaller galaxies orbiting around them. The third-largest galaxy is the Triangulum Galaxy, which is smaller than the other two but still quite big. There are many other smaller galaxies in the Local Group, each with its own interesting features and histories.
History
The term "The Local Group" was introduced by Edwin Hubble in his 1936 book The Realm of the Nebulae. In this book, Hubble described the Local Group as a small collection of galaxies that are isolated in space. He listed several galaxies that belong to this group, including 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 mentioned that IC 10 might be part of the Local Group.
Component galaxies
The Local Group is a collection of galaxies that includes our own galaxy, the Milky Way. It is shaped like a dumbbell, with the Milky Way and its smaller galaxies forming one side, and the Andromeda Galaxy and its smaller galaxies forming the other side. These two groups of galaxies are moving towards each other.
| Name | Type | Constellation | |
|---|---|---|---|
| Spiral galaxies | |||
| Andromeda Galaxy (M31, NGC 224) | SAb | Andromeda | |
| Milky Way Galaxy | SBbc | Sagittarius (centre) | |
| Triangulum Galaxy (M33, NGC 598) | SAcd | Triangulum | |
| Magellanic spiral galaxies | |||
| Large Magellanic Cloud (LMC, Dorado Dwarf) | Irr/SB(s)m | Dorado | |
| Elliptical galaxies | |||
| M32 (NGC 221, Andromeda Dwarf) | cE2 | Andromeda | |
| Irregular galaxies | |||
| Wolf–Lundmark–Melotte (WLM, DDO 221) | Ir+ | Cetus | |
| IC 10 (Cascopea IV, PGC 4774942-40+4) | KBm or Ir+ | Cassiopeia | |
| Small Magellanic Cloud (SMC, NGC 292, Tucana galaxy) | SB(s)m pec | Tucana | |
| Pisces Dwarf (LGS3,Pisces I dwarf irregular) | Irr | Pisces | |
| IC 1613 (UGC 668, UGCA 47954) | IAB(s)m V | Cetus | |
| Phoenix Dwarf (Phoenix I dwarf) | Irr | Phoenix | |
| Leo A (Leo III, PCA QA JO74974) | IBm V | Leo | |
| Aquarius Dwarf (DDO 210, Aquarius I, ESO 497-4054.4591 G) | IB(s)m | Aquarius | |
| SagDIG (Sagittarius Dwarf Irregular Galaxy, Sagittarius II) | IB(s)m V | Sagittarius | |
| NGC 6822 (Barnard's Galaxy, AO 4797) | IB(s)m IV-V | Sagittarius | |
| Pegasus Dwarf (Pegasus Dwarf Irregular, DDO 216) | Irr | Pegasus | |
| UGC 4879 (VV124) | IAm | Ursa Major | |
| Sextans A (UGCA 205, AO 4977) | Ir+V | Sextans | |
| Sextans B (UGC 5373, QRT 947748) | Ir+IV-V | Sextans | |
| Leo P (AGC 19470059) | Irr | Leo | |
| AGC 198606 (Leo VI) | Irr? | Leo | |
| AGC 215417(Leo VII) | Irr? | Leo | |
| AGC 219656 | Irr? | Leo | |
| AGC 249525 | Irr? | Boötes | |
| AGC 268069 | Irr? | Serpens | |
| Dwarf elliptical galaxies | |||
| M110 (NGC 205) | dE6p | Andromeda | |
| NGC 147 (DDO 3) | dE5 pec | Cassiopeia | |
| Dwarf spheroidal galaxies | |||
| Boötes I (DDO 9774998.074÷×47) | dSph | Boötes | |
| Cetus Dwarf | dSph/E4 | Cetus | |
| Canes Venatici I Dwarf and Canes Venatici II Dwarf | dSph | Canes Venatici | |
| Andromeda III | dE2 | Andromeda | |
| NGC 185 | dE3 pec | Cassiopeia | |
| Andromeda I | dE3 pec | Andromeda | |
| Sculptor Dwarf (E351-G30) | dE3 | Sculptor | |
| Andromeda V (UKS 4977-94) | dSph | Andromeda | |
| Andromeda II (NCA 14) | dE0 | Andromeda | |
| Fornax Dwarf (E356-G04) | dSph/E2 | Fornax | |
| Carina Dwarf (E206-G220) | dE3 | Carina | |
| Leo I (DDO 74) | dE3 | Leo | |
| Sextans Dwarf (Sextans 1) | dE3 | Sextans | |
| Leo II (Leo B) | dE0 pec | Leo | |
| Ursa Minor Dwarf (NCA 47-49) | dE4 | Ursa Minor | |
| Draco Dwarf (DDO 208) | dE0 pec | Draco | |
| SagDSG (Sagittarius Dwarf Spheroidal Galaxy) | dSph/E7 | Sagittarius | |
| Tucana Dwarf | dE5 | Tucana | |
| Cassiopeia Dwarf (Andromeda VII, NCA 4) | dSph | Cassiopeia | |
| Pegasus Dwarf Spheroidal Galaxy (Andromeda VI) | dSph | Pegasus | |
| Ursa Major I Dwarf | dSph | Ursa Major | |
| Ursa Major II Dwarf | dSph | Ursa Major | |
| Ursa Major III | dSph | Ursa Major | |
| Leo IV | dSph | Leo | |
| Leo V | dSph | Leo | |
| Leo T | dSph/Irr | Leo | |
| Boötes II | dSph | Boötes | |
| Boötes III (NCA 4.9) | dSph | Boötes | |
| Boötes IV | dSph | Boötes | |
| Coma Berenices | dSph | Coma Berenices | |
| Segue 2 (Aries Dwarf, NCA 429) | dSph | Aries | |
| Hercules (NCA 4977429) | dSph | Hercules | |
| Pisces II | dSph | Pisces | |
| Reticulum II | dSph | Reticulum | |
| Reticulum III | dSph | Reticulum | |
| Eridanus II | dSph | Eridanus | |
| Grus I | dSph | Grus | |
| Grus II | dSph | Grus | |
| Tucana II | dSph | Tucana | |
| Hydrus I (Hydrus Dwarf spheroidal galaxy) | dSph | Hydrus | |
| Draco II | dSph | Draco | |
| Carina III | dSph | Carina | |
| Triangulum II (Laevens 2) | dSph | Triangulum | |
| Carina II | dSph | Carina | |
| Pictor II | dSph | Pictor | |
| Horologium II | dSph | Horologium | |
| Virgo I | dSph | Virgo | |
| Virgo III | dSph? | Virgo | |
| Sextans II | dSph? | Sextans | |
| Aquarius II | dSph | Aquarius | |
| Aquarius III | dSph? | Aquarius | |
| Crater II | dSph | Crater | |
| Hydra II | dSph | Hydra | |
| Antlia II | dSph | Antlia | |
| Pegasus III | dSph | Pegasus | |
| Pegasus IV | dSph | Pegasus | |
| Pegasus W | dSph | Pegasus | |
| Cetus III | dSph | Cetus | |
| Leo K | dSph? | Leo | |
| Leo M | dSph? | Leo | |
| Leo VI | dSph | Leo | |
| Leo Minor I | dSph? | Leo Minor | |
| Boötes V | dSph? | Boötes | |
| Virgo II | dSph? | Virgo | |
| Tucana B | dSph | Tucana | |
| DES 1 | dE | Perseus | |
| Antlia Dwarf | dE3/dSph/Irr? | Antlia | |
| Andromeda IX | dSph | Andromeda | |
| Andromeda X | dSph | Andromeda | |
| Andromeda XI | dSph | Andromeda | |
| Andromeda XII | dSph | Andromeda | |
| Andromeda XIII (Pisces III) | dSph | Andromeda | |
| Andromeda XIV (Pisces IV) | dSph | Pisces | |
| Andromeda XV | dSph | Andromeda | |
| Andromeda XVII | dSph | Andromeda | |
| Andromeda XIX | dSph | Andromeda | |
| Andromeda XX | dSph | Andromeda | |
| Andromeda XXI | dSph | Andromeda | |
| Andromeda XXII | dSph | Pisces | |
| Andromeda XXIII | dSph | Andromeda | |
| Andromeda XXIV | dSph | Andromeda | |
| Andromeda XXV | dSph | Andromeda | |
| Andromeda XXVI | dSph | Andromeda | |
| Andromeda XXVII | dSph | Andromeda | |
| Andromeda XXIX | dSph | Pegasus | |
| Andromeda XXX (Cassiopeia II) | dSph? | Cassiopeia | |
| Andromeda XXXI (Lacerta I) | dSph? | Lacerta | |
| Andromeda XXXII (Cassiopeia III) | dSph? | Cassiopeia | |
| Andromeda XXXIV (Pegasus V) | dSph | Pegasus | |
| Andromeda XXXV | dSph | Andromeda | |
| Andromeda XVI (Pisces V) | dSph | Pisces | |
| Andromeda XXVIII | dSph? | Pegasus | |
| Andromeda XXXIII (Perseus I) | dSph? | Perseus | |
| Andromeda XVIII | dSph | Andromeda | |
| Centaurus I | dSph | Centaurus | |
| Pisces VII (Triangulum III) | dSph? | Pisces | |
| Identification unclear | |||
| Virgo Stellar Stream | dSph (remnant)? | Virgo | |
| Canis Major Dwarf | Irr? | Canis Major | |
| Hydra 1 | Hydra | ||
| Tucana III | dSph or cluster? | Tucana | |
| Tucana IV | dSph or cluster? | Tucana | |
| Tucana V | dSph or cluster? | Tucana | |
| Columba I | dSph or cluster? | Columba | |
| Segue 1 | dSph or Globular Cluster | Leo | |
| Cetus II | Cetus | ||
| Willman 1 | dSph or Globular Cluster | Ursa Major | |
| Horologium I | dSph or Globular Cluster | Horologium | |
| Pictoris | dSph or Globular Cluster | Pictor | |
| Phoenix II | dSph or Globular Cluster | Phoenix | |
| Indus I (Kim 2, Indus Dwarf) | dSph or Globular Cluster | Indus | |
| Eridanus III | dSph or Globular Cluster | Eridanus | |
| Sagittarius II | dSph or Globular Cluster | Sagittarius | |
| Andromeda VIII (Adsant-40-7 quote serp galaxy) | dSph? | Andromeda | |
| Antlia B | Antlia | ||
| Probable non-members | |||
| NGC 3109 (Antlia Sextans galaxy l) | SB(s)m | Hydra | |
| Andromeda IV | Irr | Andromeda | |
| GR 8 (DDO 155) | Im V | Virgo | |
| IC 5152 (Indus III) | IAB(s)m IV | Indus | |
| KK 153 | Ursa Major | ||
| NGC 300 | SA(s)d | Sculptor | |
| NGC 55 | SB(s)m | Sculptor | |
| NGC 404 | E0 or SA(s)0− | Andromeda | |
| NGC 1569 (IC 49447) | Irp+ III-IV | Camelopardalis | |
| NGC 1560 (IC 2062) | Sd | Camelopardalis | |
| Camelopardalis A | Irr | Camelopardalis | |
| Argo Dwarf | Irr | Carina | |
| ESO 347-8 (2318–42, PGC 475744) | Irr | Grus | |
| UKS 2323-326 (ESO 407-18) | Irr | Sculptor | |
| UGC 9128 (DDO 187) | Irp+ | Boötes | |
| KKs 3 (Hydrus II) | dSph | Hydrus | |
| Objects in the Local Group no longer recognised as galaxies | |||
| Palomar 12 (Capricornus Dwarf) | dSphr | Capricornus | |
| Palomar 4 (Ursa Major Dwarf) | d Sphr | Ursa Major | |
| Palomar 5 (Serpens Dwarf) | Serpens | ||
| Palomar 3 (Sextans C) | Sculptor | ||
| Segue 3 | Pegasus | ||
| Laevens 1 (Crater Dwarf) | Crater | ||
| DES J2038-4609 (Indus II) | Indus | ||
| Name | Type | Constellation | |
Structure
The Local Group has some interesting features called streams. These are long, thin collections of stars or gas that have been pulled away from smaller galaxies by the gravity of larger ones. For example, the Magellanic Stream is a stream of gas being pulled from the Magellanic Clouds by the Milky Way. The Monoceros Ring is a ring of stars around the Milky Way that may have come from a small galaxy called the Canis Major Dwarf Galaxy. Other streams, like the Virgo Stream and Helmi Stream, are also formed from smaller galaxies that have been influenced by larger ones.
Future
The galaxies in the Local Group, including the Milky Way and the Andromeda Galaxy, are moving towards each other and will eventually merge into a single large galaxy over many billions of years. Scientists discuss different ideas about what this new galaxy might look like after the merger, with some thinking it will become a round elliptical galaxy and others suggesting it might keep some spiral features or become a different type of galaxy altogether.
Location
Main article: Laniakea Supercluster
The Local Group is a collection of galaxies that includes the Milky Way, where our Earth is located. It has a special shape like a dumbbell, with the Milky Way and its smaller galaxies on one side, and the Andromeda Galaxy and its smaller galaxies on the other side. These two groups of galaxies are moving towards each other.
Images
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