NGC 1406 | |
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![]() Hubble Space Telescope image of NGC 1406 | |
Observation data (J2000 epoch) | |
Constellation | Fornax |
Right ascension | 03h 39.2m [1] |
Declination | −31° 19′ [1] |
Redshift | 1076 ± 10 |
Distance | 15.3 megaparsecs (50 Mly) |
Apparent magnitude (V) | 11.8 [1] |
Characteristics | |
Type | SBbc [1] |
Apparent size (V) | 3.9′ × 0.7′ [1] |
Notable features | Edge-on barred spiral galaxy |
Other designations | |
ESO 418-15, IRAS 03373-3129, MCG -5-9-20, PGC 13458, UGCA 83 |
NGC 1406 is almost edge-on barred spiral galaxy in constellation Fornax. [2] [3] [4] [5] It was discovered by John Herschel on 18 November 1835.
It is a member of Fornax Cluster, a cluster of 200 galaxies. At a distance of 50 million light-years, it is one of the closest members of the Fornax cluster. NGC 1406 has a Hubble classification of SBbc, which indicates it is a barred spiral galaxy. It is also edge-on, making its bar hard to see. NGC 1406 has much dust in its disc, which is visible on the Hubble image in the box upper right.
Its size on night sky is 3.9' x 0.7' which is proportional to real size of 57,000 light-years. This means NGC 1406 is one of the larger galaxies in Fornax Cluster. It is north and distant from central galaxy NGC 1399, so it positions in the Fornax Cluster is at the edge of it.
Fornax is a constellation in the southern celestial hemisphere, partly ringed by the celestial river Eridanus. Its name is Latin for furnace. It was named by French astronomer Nicolas Louis de Lacaille in 1756. Fornax is one of the 88 modern constellations.
Messier 61 is an intermediate barred spiral galaxy in the Virgo Cluster of galaxies. It was first discovered by Barnaba Oriani on May 5, 1779, six days before Charles Messier discovered the same galaxy. Messier had observed it on the same night as Oriani but had mistaken it for a comet. Its distance has been estimated to be 45.61 million light years from the Milky Way Galaxy. It is a member of the M61 Group of galaxies, which is a member of the Virgo II Groups, a series of galaxies and galaxy clusters strung out from the southern edge of the Virgo Supercluster.
NGC 1365, also known as the Great Barred Spiral Galaxy, is a double-barred spiral galaxy about 75 million light-years away in the constellation Fornax.
NGC 1427A is an irregular galaxy in the constellation Fornax. Its distance modulus has been estimated using the globular cluster luminosity function to be 31.01 ± 0.21 which is about 52 Mly. It is the brightest dwarf irregular member of the Fornax cluster and is in the foreground of the cluster's central galaxy NGC 1399.
NGC 495, also occasionally referred to as PGC 5037, UGC 920 or GC 278, is a barred spiral galaxy in the constellation Pisces. It is located approximately 184 million light-years from the Solar System and was discovered on 12 September 1784 by astronomer William Herschel.
NGC 1436 is a barred spiral galaxy approximately 58 million light-years away from Earth in the constellation of Eridanus. It is a member of the Fornax I cluster.
NGC 521, also occasionally referred to as PGC 5190 or UGC 962, is a barred spiral galaxy located approximately 224 million light-years from the Solar System in the constellation Cetus. It was discovered on 8 October 1785 by astronomer William Herschel.
NGC 522, also occasionally referred to as PGC 5218 or UGC 970, is a spiral galaxy located approximately 122 million light-years from the Solar System in the constellation Pisces. It was discovered on 25 September 1862 by astronomer Heinrich Louis d'Arrest.
NGC 1374 is a low-luminosity elliptical galaxy in the southern constellation Fornax. It was discovered by John Herschel on November 29, 1837.
NGC 1375 is a barred lenticular galaxy in the constellation Fornax discovered by John Herschel on November 29, 1837. It is believed to be a member of the Fornax Cluster.
NGC 1317 is a barred spiral galaxy in the constellation Fornax, in the Fornax cluster. It was discovered by Julius Schmidt on January 19, 1865. It appears to be interacting with the much larger NGC 1316, but uncertainty in distance estimates and scales of tidal distortions make this uncertain. It is a member of the NGC 1316 subgroup, part of the Fornax Cluster. Its size is 2.8' x 2.4' which, at the average distance, gives a diameter of 55,000 light-years.
NGC 1460 is a barred lenticular galaxy in the constellation Eridanus. It was discovered by John Herschel on November 28, 1837. It is moving away from the Milky Way at 1341 km/s.
IC 1993 is an intermediate spiral galaxy in the constellation Fornax. It was discovered by Lewis Swift on November 19, 1897. At a distance of about 50 million light-years, and redshift of 1057 km/s, it is one of the closest to us of the 200 galaxies in the Fornax Cluster.
NGC 1379 is a low-luminosity elliptical galaxy in the southern constellation Fornax. It was discovered by William Herschel on December 25, 1835.
NGC 1353 is a flocculent spiral galaxy situated in the constellation of Eridanus. Located about 70 million light years away, it is a member of the Eridanus cluster of galaxies, a cluster of about 200 galaxies. It was discovered by William Herschel on 9 December 1784.
NGC 1332 is an almost edge-on elliptical galaxy located in constellation of Eridanus. Situated about 70 million light years away, it is a member of the Eridanus cluster of galaxies, a cluster of about 200 galaxies. It is also the brightest member of the NGC 1332 Group. It was discovered by William Herschel on 9 December 1784.
NGC 1347 is a barred spiral galaxy situated in the constellation of Eridanus. It is at a distance of 81 million light years and is a member of the Eridanus cluster, a cluster of about 200 galaxies.
NGC 1369 is a spiral galaxy situated in constellation of Eridanus. Located about 65 million light years away, it is a member of the Fornax cluster of galaxies, a cluster of about 200 galaxies. It was discovered by Julius Schmidt on 19 January 1865.
PGC 13809 is a spiral, almost edge-on galaxy in the constellation Fornax. It was discovered by the European Southern Observatory and it is a member of the Fornax Cluster.
NGC 1484 is a barred spiral galaxy in the constellation Eridanus, 48 million light-years from Earth. It is part of the Fornax Cluster, that contains approximately 200 galaxies, making it the second richest galaxy cluster in 100 million light-years after the Virgo Cluster.