NGC 1484 | |
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![]() legacy surveys image of NGC 1460 | |
Observation data (J2000.0 epoch) | |
Constellation | Fornax |
Right ascension | 03h 54m 20.1s [1] |
Declination | −36° 58′ 08″ [1] |
Redshift | 0.003469 [1] |
Heliocentric radial velocity | 1040 km/s [1] |
Distance | 49 Mly (14.9 Mpc) [1] |
Apparent magnitude (V) | 13.93 [1] |
Absolute magnitude (B) | -19.21 ± 0.20 [1] |
Characteristics | |
Type | SB(s)b? [1] |
Mass | 3.8×109 (Stellar mass) [2] M☉ |
Size | 35,638 light years (estimated) [1] |
Apparent size (V) | 2.5 x 0.6 [1] |
Other designations | |
ESO 359- G 006, MCG -06-09-036, PGC 014071 [1] |
NGC 1484 is a barred spiral galaxy approximately 50 million light-years away [3] from Earth in the constellation of Fornax. It was discovered by astronomer John Herschel on November 28, 1837. [4] NGC 1484 is a member of the Fornax cluster. [5] [2]
Its distance and size on the night sky convert to an approximate size of 35,638 light years, only a third or one-quarter the size of the Milky Way Galaxy.
NGC 4706 is a lenticular galaxy located about 157 million light-years away in the constellation Centaurus. It was discovered by astronomer John Herschel on June 5, 1834. NGC 4706 is a member of the Centaurus Cluster.
NGC 4729 is an elliptical galaxy located about 160 million light-years away in the constellation Centaurus. NGC 4729 was discovered by astronomer John Herschel on June 8, 1834 and is a member of the Centaurus Cluster.
NGC 4730 is a lenticular galaxy located about 160 million light-years away in the constellation Centaurus. NGC 4730 was discovered by astronomer John Herschel on June 8, 1834. NGC 4730 is a member of the Centaurus Cluster.
NGC 4207 is a spiral galaxy located about 50 million light-years away in the constellation Virgo. The galaxy was discovered by astronomer Heinrich d'Arrest on March 23, 1865. NGC 4207 is a member of the Virgo Cluster.
NGC 679 is an elliptical or a lenticular galaxy located 210 million light-years away in the constellation Andromeda. The galaxy was discovered by astronomer William Herschel on September 13, 1784 and is a member of Abell 262.
NGC 688 is a barred spiral galaxy with starburst activity located 190 million light-years away in the constellation Triangulum. It was discovered by astronomer Heinrich d'Arrest on September 16, 1865 and is a member of the galaxy cluster Abell 262.
NGC 703 is a lenticular galaxy located 240 million light-years away in the constellation Andromeda. The galaxy was discovered by astronomer William Herschel on September 21, 1786 and is also a member of Abell 262.
NGC 709 is a lenticular galaxy located 150 million light-years away in the constellation Andromeda. It was discovered by the Irish engineer and astronomer Bindon Blood Stoney on October 28, 1850 and is a member of the galaxy cluster Abell 262.
NGC 714 is a lenticular galaxy located 190 million light-years away in the constellation Andromeda. The galaxy was discovered by astronomer Bindon Blood Stoney on October 28, 1850 and is a member of Abell 262.
NGC 717 is a lenticular galaxy located 210 million light-years away in the constellation Andromeda. The galaxy was discovered by astronomer Bindon Blood Stoney on October 28, 1850 and is a member of Abell 262.
NGC 753 is a spiral galaxy located 220 million light-years away in the constellation Andromeda. The galaxy was discovered by astronomer by Heinrich d'Arrest on September 16, 1865 and is a member of Abell 262.
NGC 759 is an elliptical galaxy located 230 million light-years away in the constellation Andromeda. NGC 759 was discovered by astronomer by Heinrich d'Arrest on September 17, 1865. It is a member of Abell 262.
NGC 4318 is a small lenticular galaxy located about 72 million light-years away in the constellation Virgo. It was discovered by astronomer John Herschel on January 18, 1828. NGC 4318 is a member of the Virgo W′ group, a group of galaxies in the background of the Virgo Cluster that is centered on the giant elliptical galaxy NGC 4365.
NGC 1460 is a barred lenticular galaxy with a peanut-shapped bar approximately 65 million light-years away from Earth in the constellation of Eridanus. It was discovered by astronomer John Herschel on November 28, 1837. It is a member of the Fornax cluster.
NGC 1369 is a barred lenticular galaxy located 59 millon light years away in constellation of Eridanus. The galaxy was discovered by astronomer Julius Schmidt on January 19, 1865, and is a member of the Fornax Cluster. NGC 1369 is a host to a supermassive black hole with an estimated mass of 1.8 millon solar masses.
NGC 1428 is a peculiar galaxy of an uncertain morphology; either an elliptical or lenticular galaxy located approximately 65 million light-years away from Earth.
The Telescopium−Grus Cloud is a galaxy filament in the constellations of Pavo, Indus, and Telescopium. It was first defined by astronomer Brent Tully in his book The Nearby Galaxies Atlas and its companion book The Nearby Galaxies Catalog.
NGC 4331 is an irregular galaxy located 74 million light-years away in the constellation Draco. The galaxy was discovered by astronomer William Herschel on December 12, 1797. The galaxy is host to a black hole with an estimated mass of 4.6×105 solar masses.
NGC 1396 is a dwarf elliptical galaxy located 61 millon light years away in the constellation of Fornax. The galaxy was discovered by astronomer Julius Schmidt on January 19, 1865, and is a member of the Fornax Cluster. Despite the fact that the galaxy PGC 13398 is most commonly identified as NGC 1396, there is uncertainty in its identification.
NGC 1419 is an elliptical galaxy located 62 millon light years away in the constellation of Eridanus. The galaxy was discovered by astronomer John Herschel on October 22, 1835, and is a member of the Fornax Cluster. NGC 1419 is a host to a supermassive black hole with an estimated mass of 25 millon solar masses.