NGC 555 | |
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Observation data (J2000 epoch) | |
Constellation | Cetus |
Right ascension | 01h 27m 11.80s [1] |
Declination | −22° 45′ 43.00″ [1] |
Redshift | 0.034137 ± 1.50 [1] |
Distance | 479 Mly (147.04 Mpc) [1] |
Apparent magnitude (V) | 14.4 [1] |
Characteristics | |
Type | G [1] |
Size | 173,000 ly [1] |
Apparent size (V) | 0.759′ × 0.676′ [1] |
Notable features | Maybe evolving into a ring galaxy(?) |
Other designations | |
ESO 476-12, [1] PGC 5419, [1] 2MASX J01271185-2245439, [1] GSC 06426-00050, [1] MCG-04-04-014, [1] ESO-LV 476-0120, [1] SGC 012448-2301.3, [1] 6dFGS gJ012711.8-224544, [1] NPM1G -23.0003, [1] LEDA 5419, [1] APMBGC 476+036-111, [1] Gaia DR2 5042200315975022592 [1] |
NGC 555 is a lenticular galaxy located around 479 million light-years away in the constellation Cetus. [1] NGC 555 was discovered in 1886 by the American astronomer Frank Muller. [2] NGC 555 is not known to have much star formation, and it is not known to have an active galactic nucleus. [3] [1]
NGC 61 is a pair of lenticular galaxies, NGC 61-A and NGC 61-B in the constellation Cetus. Both were discovered on September 10, 1785, by William Herschel.
NGC 65 is a lenticular galaxy in the constellation Cetus. Its apparent magnitude is 13.4. It was first discovered in 1886, and is also known as PGC 1229.
NGC 114 is a barred lenticular galaxy located in the constellation Cetus. It was discovered by American astronomer Truman Henry Safford on September 23, 1867. The galaxy lies approximately 195 million light-years from Earth, and is about 55,000 light-years in diameter, nearly half the size of the Milky Way.
NGC 117 is a lenticular galaxy with a magnitude of 14.3 in the constellation Cetus. NGC 117 is its New General Catalogue designation. It was discovered on September 13, 1863, by the astronomer Albert Marth.
NGC 170 is a lenticular galaxy located in the constellation Cetus. It was discovered on 3 November 1863 by Albert Marth.
NGC 179 is a lenticular galaxy located 3.3 million light-years away in the constellation Cetus. It was discovered in 1886 by Francis Preserved Leavenworth.
NGC 197 is a lenticular galaxy located in the constellation Cetus. It was discovered on October 16, 1863 by Albert Marth.
NGC 357 is a barred lenticular or spiral galaxy in the constellation Cetus. It was discovered on September 10, 1785, by William Herschel. It was described by Dreyer as "faint, small, irregularly round, suddenly brighter middle, 14th magnitude star 20 arcsec to northeast."
NGC 4461 is a lenticular galaxy located about 50 million light-years away in the constellation of Virgo. It was discovered by astronomer William Herschel on April 12, 1784. NGC 4461 is a member of Markarian's Chain which is part of the Virgo Cluster.
NGC 4623 is an edge-on lenticular or elliptical galaxy located about 54 million light-years away in the constellation of Virgo. NGC 4623 is classified as an E7, a rare type of "late" elliptical that represents the first stage of transition into a lenticular galaxy. NGC 4623 was discovered by astronomer William Herschel on April 13, 1784. NGC 4623 is a member of the Virgo Cluster.
NGC 966 is an unbarred lenticular galaxy approximately 440 million light-years away from Earth in the constellation of Cetus. It was discovered by American astronomer Francis Preserved Leavenworth in 1886.
NGC 655 is a lenticular galaxy located 400 million light-years away in the constellation Cetus. It was discovered in a sky-survey by Ormond Stone on December 12, 1885.
NGC 830 is a barred lenticular galaxy in the constellation Cetus. It is estimated to be about 170 million light-years from the Milky Way and has a diameter of approximately 70,000 light years.
NGC 790 is a lenticular galaxy in the constellation Cetus. It is estimated to be 233 million light-years from the Milky Way and has a diameter of approximately 90,000 light years. NGC 790 was discovered on September 10, 1785 by the German-British astronomer William Herschel.
NGC 530, also known as IC 106, is a lenticular galaxy in the constellation Cetus. It is approximately 226 million light years from the Milky Way and has a diameter of around 100,000 light years. The object was discovered on November 20, 1886, by the American astronomer Lewis A. Swift, who listed it as NGC 530, and rediscovered on November 16, 1887, by Guillaume Bigourdan, who listed it as IC 106.
NGC 905 is a lenticular galaxy with an active nucleus in the constellation Cetus south. It is estimated to be 644 million light-years from the Milky Way and has a diameter of approximately 85,000 ly. NGC 905 was discovered by astronomer Francis Leavenworth.
NGC 814 is a lenticular galaxy in the constellation Cetus. It is estimated to be about 70 million light-years from the Milky Way and has a diameter of approximately 30,000 ly. NGC 814 was discovered on January 6, 1886, by the American astronomer Ormond Stone.
NGC 734 is a lenticular galaxy with a central bar in the constellation Cetus, which is about 538 million light years from the Milky Way. It was discovered on November 9, 1885, by the American astronomer Francis Preserved Leavenworth.
NGC 839 is a lenticular galaxy located in the constellation Cetus. It was discovered November 28, 1785 in a sky survey by Wilhelm Herschel. It is one of the galaxies that are part of the quadruplet family HGC 16, along with the unbarred lenticular galaxy NGC 838.
NGC 895 is a spiral galaxy located around 98 million light-years away in the constellation Cetus. NGC 895 was discovered November 28, 1856 by R. J. Mitchell. NGC 895 is not known to have much star-formation, and is not known to have an active galactic nuclei.