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Andromeda galaxy | | | celestial sphere | | | Messier object | | | | | or center of gravity | | Subdivided according to the openness of the spiral arms as Sa spiral, Sb spiral or Sc spiral. | determined from Cepheid period-luminosity relation | | | | | | | | | Messier catalog | | | | | | 1010 to 1012 Msun | | | M 31 | The largest member of the local group. It is a giant spiral galaxy that lies 2.4 million light-years away. | | 106 to 1012 |
Crab Nebula | | 1 | gas | 947 years | | Messier object | | | | | or center of gravity | | | 2 kpc | 10000 km s-1 | SNR | | | | | | | Messier catalog | | enhanced with heavy elements relative to the interstellar medium | radio | | | | | synchrotron radiation | 2U 0531+22 | A chaotic, expanding mass of gas in Taurus, the remnant of a Type I supernova whose light reached Earth in 1054. It is an intense radio source, and its visible light is strongly polarized. It is also a source of X-rays and gamma-rays. Its total mass is about 1 Msun, but the total energy radiated by the Crab is 1037-1038 ergs s-1. It is periodically occulted by the Moon, and every June its radio spectrum is occulted by the solar corona. | | |
Dumbbell Nebula | | 27 | gas | | | Messier object | | typically 10 km/s | | | or center of gravity | | | 220 pc | | | | | | | | | planetary nebula catalog | | enhanced with heavy elements relative to the interstellar medium | | | | | | | NGC 6853 | A planetary nebula of large apparent diameter and low surface brightness. | | |
Lagoon Nebula | | 8 | gas | | | Messier object | | | | | or center of gravity | | | 5000 light years | | | | | | | | | gaseous nebula catalog | | ionized hydrogen | | | | | | | NGC 6523 | An emission nebula in Sagittarius 2 kpc distant. | | |
M 10 | NED, SIMBAD | 10 | halo | oldest stellar formation in the Galaxy | about 100 light-years | Messier object | very high | | | | most are in the halo some are members of the thick disk | elongated, around the galactic center | | from Earth | | | | low abundances of heavy elements | | | Charles Messier | | Messier catalog | | | | | | 104 to 106 Msun | | | NGC 6254 | | 1764 | 105 to 106 |
M 100 | | 100 | celestial sphere | | | Messier object | | | | | or center of gravity | | Subdivided according to the openness of the spiral arms as Sa spiral, Sb spiral or Sc spiral. | from Earth | | | | | | | Pierre Mechain | | Messier catalog | | | | | | 1010 to 1012 Msun | | | NGC 4321 | | 1781 | 106 to 1012 |
M 107 | NED, SIMBAD | 107 | halo | oldest stellar formation in the Galaxy | about 100 light-years | Messier object | very high | | | | most are in the halo some are members of the thick disk | elongated, around the galactic center | | from Earth | | | | low abundances of heavy elements | | | Pierre Mechain | | Messier catalog | | | | | | 104 to 106 Msun | | | NGC 6171 | | 1782 | 105 to 106 |
M 12 | NED, SIMBAD | 12 | halo | oldest stellar formation in the Galaxy | about 100 light-years | Messier object | very high | | | | most are in the halo some are members of the thick disk | elongated, around the galactic center | | from Earth | | | | low abundances of heavy elements | | | Charles Messier | | Messier catalog | | | | | | 104 to 106 Msun | | | NGC 6218 | | 1764 | 105 to 106 |
M 13 | NED, SIMBAD | 13 | halo | oldest stellar formation in the Galaxy | about 100 light-years | Messier object | very high | | | | most are in the halo some are members of the thick disk | elongated, around the galactic center | | from Earth | | | | low abundances of heavy elements | | | Edmond Halley | | Messier catalog | | | | | | 104 to 106 Msun | | | NGC 6205 | | 1714. | 105 to 106 |
M 14 | NED, SIMBAD | 14 | halo | oldest stellar formation in the Galaxy | about 100 light-years | Messier object | very high | | | | most are in the halo some are members of the thick disk | elongated, around the galactic center | | from Earth | | | | low abundances of heavy elements | | | Charles Messier | | Messier catalog | | | | | | 104 to 106 Msun | | | NGC 6402 | | 1764 | 105 to 106 |
M 15 | NED, SIMBAD | 15 | halo | oldest stellar formation in the Galaxy | about 100 light-years | Messier object | very high | | | | most are in the halo some are members of the thick disk | elongated, around the galactic center | | from Earth | | | | low abundances of heavy elements | | | Jean-Dominique Maraldi | | Messier catalog | | | | | | 104 to 106 Msun | | | NGC 7078 | | 1746 | 105 to 106 |
M 19 | NED, SIMBAD | 19 | halo | oldest stellar formation in the Galaxy | about 100 light-years | Messier object | very high | | | | most are in the halo some are members of the thick disk | elongated, around the galactic center | | from Earth | | | | low abundances of heavy elements | | | Charles Messier | | Messier catalog | | | | | | 104 to 106 Msun | | | NGC 6273 | | 1764 | 105 to 106 |
M 2 | NED, SIMBAD | 2 | halo | oldest stellar formation in the Galaxy | about 100 light-years | Messier object | very high | | | | most are in the halo some are members of the thick disk | elongated, around the galactic center | | from Earth | | | | low abundances of heavy elements | | | Jean-Dominique Maraldi | | Messier catalog | | | | | | 104 to 106 Msun | | | NGC 7089 | | 11 September 1746 | 105 to 106 |
M 22 | NED, SIMBAD | 22 | halo | oldest stellar formation in the Galaxy | about 100 light-years | Messier object | very high | | | | most are in the halo some are members of the thick disk | elongated, around the galactic center | | from Earth | | | | low abundances of heavy elements | | | Abraham Ihle | | Messier catalog | | | | | | 104 to 106 Msun | | | NGC 6656 | | 1665 | 105 to 106 |
M 28 | NED, SIMBAD | 28 | halo | oldest stellar formation in the Galaxy | about 100 light-years | Messier object | very high | | | | most are in the halo some are members of the thick disk | elongated, around the galactic center | | from Earth | | | | low abundances of heavy elements | | | Charles Messier | | Messier catalog | | | | | | 104 to 106 Msun | | | NGC 6626 | | 1764 | 105 to 106 |
M 3 | NED, SIMBAD | 3 | halo | oldest stellar formation in the Galaxy | about 100 light-years | Messier object | very high | | | | most are in the halo some are members of the thick disk | elongated, around the galactic center | | from Earth | | | | low abundances of heavy elements | | | Charles Messier | | Messier catalog | | | | | | 104 to 106 Msun | | | NGC 5272 | | 3 May 1764 | 105 to 106 |
M 30 | NED, SIMBAD | 30 | halo | oldest stellar formation in the Galaxy | about 100 light-years | Messier object | very high | | | | most are in the halo some are members of the thick disk | elongated, around the galactic center | | from Earth | | | | low abundances of heavy elements | | | Charles Messier | | Messier catalog | | | | | | 104 to 106 Msun | | | NGC 7099 | | 1764 | 105 to 106 |
M 32 | | 32 | celestial sphere | | | Messier object | | | | | or center of gravity | | | from Earth | | | | | | Andromeda galaxy | | | Messier catalog | | | | | | | | | | An elliptical galaxy that orbits the Andromeda galaxy. | | 106 to 1012 |
M 4 | NED, SIMBAD | 4 | halo | oldest stellar formation in the Galaxy | about 100 light-years | Messier object | very high | | | | most are in the halo some are members of the thick disk | elongated, around the galactic center | | from Earth | | | | low abundances of heavy elements | | | Philippe Loys de Cheseaux | | Messier catalog | | | | | | 104 to 106 Msun | | | NGC 6121 | | 1746 | 105 to 106 |
M 5 | NED, SIMBAD | 5 | halo | oldest stellar formation in the Galaxy | about 100 light-years | Messier object | very high | | | | most are in the halo some are members of the thick disk | elongated, around the galactic center | | from Earth | | | | low abundances of heavy elements | | | Gottfried Kirch | | Messier catalog | | | | | | 104 to 106 Msun | | | NGC 5904 | | 1702 | 105 to 106 |
M 53 | NED, SIMBAD | 53 | halo | oldest stellar formation in the Galaxy | about 100 light-years | Messier object | very high | | | | most are in the halo some are members of the thick disk | elongated, around the galactic center | | from Earth | | | | low abundances of heavy elements | | | Johan Elert Bode | | Messier catalog | | | | | | 104 to 106 Msun | | | NGC 5024 | | 1775 | 105 to 106 |
M 54 | NED, SIMBAD | 54 | halo | oldest stellar formation in the Galaxy | about 100 light-years | Messier object | very high | | | | most are in the halo some are members of the thick disk | elongated, around the galactic center | | from Earth | | | | low abundances of heavy elements | | | Charles Messier | | Messier catalog | | | | | | 104 to 106 Msun | | | NGC 6715 | | 1778 | 105 to 106 |
M 55 | NED, SIMBAD | 55 | halo | oldest stellar formation in the Galaxy | about 100 light-years | Messier object | very high | | | | most are in the halo some are members of the thick disk | elongated, around the galactic center | | from Earth | | | | low abundances of heavy elements | | | Abbe Nicholas Louis de la Caille | | Messier catalog | | | | | | 104 to 106 Msun | | | NGC 6809 | | 1751 | 105 to 106 |
M 56 | NED, SIMBAD | 56 | halo | oldest stellar formation in the Galaxy | about 100 light-years | Messier object | very high | | | | most are in the halo some are members of the thick disk | elongated, around the galactic center | | from Earth | | | | low abundances of heavy elements | | | Charles Messier | | Messier catalog | | | | | | 104 to 106 Msun | | | NGC 6779 | | 1779 | 105 to 106 |
M 62 | NED, SIMBAD | 62 | halo | oldest stellar formation in the Galaxy | about 100 light-years | Messier object | very high | | | | most are in the halo some are members of the thick disk | elongated, around the galactic center | | from Earth | | | | low abundances of heavy elements | | | Charles Messier | | Messier catalog | | | | | | 104 to 106 Msun | | | NGC 6266 | | 1771 | 105 to 106 |
M 68 | NED, SIMBAD | 68 | halo | oldest stellar formation in the Galaxy | about 100 light-years | Messier object | very high | | | | most are in the halo some are members of the thick disk | elongated, around the galactic center | | from Earth | | | | low abundances of heavy elements | | | Pierre Mechain | | Messier catalog | | | | | | 104 to 106 Msun | | | NGC 4590 | | 1780 | 105 to 106 |
M 69 | NED, SIMBAD | 69 | halo | oldest stellar formation in the Galaxy | about 100 light-years | Messier object | very high | | | | most are in the halo some are members of the thick disk | elongated, around the galactic center | | from Earth | | | | low abundances of heavy elements | | | Abbe Nicholas Louis de la Caille | | Messier catalog | | | | | | 104 to 106 Msun | | | NGC 6637 | | 1751 | 105 to 106 |
M 70 | NED, SIMBAD | 70 | halo | oldest stellar formation in the Galaxy | about 100 light-years | Messier object | very high | | | | most are in the halo some are members of the thick disk | elongated, around the galactic center | | from Earth | | | | low abundances of heavy elements | | | Charles Messier | | Messier catalog | | | | | | 104 to 106 Msun | | | NGC 6681 | | 1780 | 105 to 106 |
M 71 | NED, SIMBAD | 71 | halo | oldest stellar formation in the Galaxy | about 100 light-years | Messier object | very high | | | | most are in the halo some are members of the thick disk | elongated, around the galactic center | | from Earth | | | | low abundances of heavy elements | | | Philippe Loys de Cheseaux | | Messier catalog | | | | | | 104 to 106 Msun | | | NGC 6838 | | 1745 | 105 to 106 |
M 72 | NED, SIMBAD | 72 | halo | oldest stellar formation in the Galaxy | about 100 light-years | Messier object | very high | | | | most are in the halo some are members of the thick disk | elongated, around the galactic center | | from Earth | | | | low abundances of heavy elements | | | Pierre Mechain | | Messier catalog | | | | | | 104 to 106 Msun | | | NGC 6981 | | 1780 | 105 to 106 |
M 75 | NED, SIMBAD | 75 | halo | oldest stellar formation in the Galaxy | 6.0 arc min | Messier object | very high | | | | most are in the halo some are members of the thick disk | elongated, around the galactic center | | 57.7 kly | | | | low abundances of heavy elements | | | Pierre Mechain | | Messier catalog | | | | | 8.5 (V) | 104 to 106 Msun | | | NGC 6864 | | 1780 | 105 to 106 |
M 79 | NED, SIMBAD | 79 | halo | oldest stellar formation in the Galaxy | about 100 light-years | Messier object | very high | | | | most are in the halo some are members of the thick disk | elongated, around the galactic center | | from Earth | | | | low abundances of heavy elements | | | Pierre Mechain | | Messier catalog | | | | | | 104 to 106 Msun | | | NGC 1904 | | 1780 | 105 to 106 |
M 80 | NED, SIMBAD | 80 | halo | oldest stellar formation in the Galaxy | about 100 light-years | Messier object | very high | | | | most are in the halo some are members of the thick disk | elongated, around the galactic center | | 28000 light years | | | | low abundances of heavy elements | | | Charles Messier | | Messier catalog | | | | | | 104 to 106 Msun | | | NGC 6093 | | 1781 | 105 to 106 |
M 81 | | 81 | celestial sphere | | | Messier object | | | | | or center of gravity | | Subdivided according to the openness of the spiral arms as Sa spiral, Sb spiral or Sc spiral. | from Earth | | | | | | | Johan Elert Bode | | Messier catalog | | | | | | 1010 to 1012 Msun | | | NGC 3031 | A giant spiral galaxy 11 million light-years away in the constellation Ursa Major. It rules the M81 group, the second nearest galaxy group to the Local Group. | 1774 | 106 to 1012 |
M 87 | | 87 | celestial sphere | | | Messier object | | | | | or center of gravity | | | from Earth | | | | | E0 (spherical) to E7 (greatest eccentricity) | | | | Messier catalog | | | X-ray | | | 1013 Msun (most massive galaxies known) | | | Virgo X-1 | A strong radio source. Optically, it is an elliptical galaxy with a luminous blue jet about 1500 pc long. It is also one of the most powerful extragalactic sources of radiation at infrared wavelengths. | | 106 to 1012 |
M 9 | NED, SIMBAD | 9 | halo | oldest stellar formation in the Galaxy | about 100 light-years | Messier object | very high | | | | most are in the halo some are members of the thick disk | elongated, around the galactic center | | from Earth | | | | low abundances of heavy elements | | | Charles Messier | | Messier catalog | | | | | | 104 to 106 Msun | | | NGC 6333 | | 1764 | 105 to 106 |
M 92 | NED, SIMBAD | 92 | halo | oldest stellar formation in the Galaxy | about 100 light-years | Messier object | very high | | | | most are in the halo some are members of the thick disk | elongated, around the galactic center | | from Earth | | | | low abundances of heavy elements | | | Johan Elert Bode | | Messier catalog | | | | | | 104 to 106 Msun | | | NGC 6341 | | 1777 | 105 to 106 |
Omega Nebula | | 17 | gas | | | Messier object | | | | 1745 | or center of gravity | | | from Earth | | | | | | | Philippe Loys de Cheseaux | | gaseous nebula catalog | | ionized hydrogen | | | | | | | NGC 6618 | A bright H II region. It is a double radio source. | | |
Orion Nebula | | 42 | gas | 20000 years | | Messier object | | | | | or center of gravity | | | 500 pc | | | | | | | | | gaseous nebula catalog | trapezium | ionized hydrogen | | | | | | | M 42 | The Orion Nebula, a star-forming region in the constellation Orion. | | |
Owl Nebula | | 97 | gas | | | Messier object | | typically 10 km/s | | | or center of gravity | | | 600 pc | | | | | | | | | planetary nebula catalog | | enhanced with heavy elements relative to the interstellar medium | | | | | | | NGC 3587 | A planetary nebula. | | |
Pinwheel galaxy | | 33 | celestial sphere | | | Messier object | | | | | or center of gravity | | Subdivided according to the openness of the spiral arms as Sa spiral, Sb spiral or Sc spiral. | 800 kpc from Milky Way galaxy | | | | | | | Hodierna | | Messier catalog | | | | | | 1010 to 1012 Msun | | | Triangulum galaxy | A Sc II-III spiral galaxy, a satellite of the Andromeda galaxy, about 700 kpc distant. Mv = - 18.9. | 1654 | 106 to 1012 |
Pleiades | | 45 | disk | very young | | Messier object | | | | | or center of gravity | | | 125 pc | | | | | | | | | open cluster catalog | | B star, late star | | | | | | | NGC 1432 | | | several hundred |
Praesepe | | 44 | disk | varies widely | | naked eye object | | | | | or center of gravity | | | 160 pc | | | | | | | | | open cluster catalog | | | | | | | | | NGC 2632 | | | |
Ring Nebula | | 57 | gas | | | Messier object | | typically 10 km/s | | | or center of gravity | | | 2000 light years | | | | | | | | | planetary nebula catalog | | enhanced with heavy elements relative to the interstellar medium | | | | | | | M 57 | A famous planetary nebula (M57, NGC 6720) in the constellation Lyra. | | |
Sombrero galaxy | | 104 | celestial sphere | | | Messier object | | | | | or center of gravity | | Subdivided according to the openness of the spiral arms as Sa spiral, Sb spiral or Sc spiral. | from Earth | | | | | | | | | Messier catalog | | | | | | 1010 to 1012 Msun | | | NGC 4594 | A spiral galaxy in the constellation Virgo. It was the first galaxy whose rotation was detected. | | 106 to 1012 |
Trifid Nebula | | 20 | gas | | | Messier object | | | | | or center of gravity | | | 9000 light years | | | | | | | | | gaseous nebula catalog | | ionized hydrogen | | | | | | | NGC 6514 | An emission nebula in Sagittarius. | | |
Whirlpool galaxy | | 51 | celestial sphere | | | Messier object | | | | | or center of gravity | | Subdivided according to the openness of the spiral arms as Sa spiral, Sb spiral or Sc spiral. | from Earth | | | | | | | Charles Messier | | Messier catalog | | | | | | 1010 to 1012 Msun | | | NGC 5194 | | 1773 | 106 to 1012 |