NGC 12

Last updated
NGC 12
NGC12 - SDSS DR14.jpg
Observation data (J2000 epoch)
Constellation Pisces
Right ascension 00h 08m 44.752s [1]
Declination +04° 36 45.12 [1]
Redshift 0.013049 [2]
Helio radial velocity 3886 ± 42 km/s [2]
Distance 183 Mly
Apparent magnitude  (V)13.18 [3]
Apparent magnitude  (B)13.84 [3]
Characteristics
Type SAB(rs)c: [4]
Apparent size  (V)1.7 × 1.35 [5]
Other designations
UGC 74, MCG +01-01-040, PGC 645 [2]

NGC 12 is an intermediate spiral galaxy in the Pisces constellation. It was discovered by William Herschel on December 6, 1790. [5]

Related Research Articles

<span class="mw-page-title-main">NGC 5886</span> Galaxy in the constellation Boötes

NGC 5886 is an +14 magnitude elliptical galaxy in the constellation Boötes. It was originally discovered by John Herschel in 1828 with an 18.7 inch reflector.

<span class="mw-page-title-main">NGC 5821</span> Galaxy in the constellation of Boötes

NGC 5821 is a spiral galaxy with a ring structure in the constellation Boötes. It lies near a similarly massed galaxy, NGC 5820, at the same redshift. Both galaxies were discovered by the astronomer William Herschel.

<span class="mw-page-title-main">NGC 31</span> Galaxy located in the constellation Phoenix

NGC 31 is a spiral galaxy located in the constellation Phoenix. It was discovered on October 28, 1834 by the astronomer John Herschel. Its morphological type is SB(rs)cd, meaning that it is a late-type barred spiral galaxy.

<span class="mw-page-title-main">NGC 3552</span> Galaxy in the constellation Ursa Major

NGC 3552 is a lenticular galaxy in the constellation Ursa Major. It was discovered on April 11, 1785 by William Herschel. It is a member of the galaxy cluster Abell 1185.

<span class="mw-page-title-main">NGC 38</span> Spiral galaxy in the constellation Pisces

NGC 38 is a spiral galaxy in the constellation Pisces. It was discovered in 1881.

<span class="mw-page-title-main">NGC 4780</span> Spiral galaxy in the constellation Virgo

NGC 4780 is an intermediate spiral galaxy within the constellation Virgo. It is located about 166 million light-years away from the Sun. It was discovered in 1880 by the astronomer Wilhelm Tempel.

<span class="mw-page-title-main">NGC 7499</span> Galaxy in the constellation Pisces

NGC 7499 is an unbarred lenticular galaxy within the constellation Pisces. NGC 7499 is its New General Catalogue designation. It was discovered on September 2, 1864 by the astronomer Albert Marth.

<span class="mw-page-title-main">NGC 42</span> Galaxy located in the constellation Pegasus

NGC 42 is a lenticular galaxy in the Pegasus constellation. It was discovered on October 30, 1864, by the German astronomer Albert Marth. It may be gravitationally interacting with the nearby NGC 41.

<span class="mw-page-title-main">NGC 1728</span> Spiral galaxy in the constellation Eridanus

NGC 1728 is a spiral galaxy in the constellation Eridanus. The galaxy is listed in the New General Catalogue. It was discovered on November 10, 1885 by the astronomer Edward Emerson Barnard.

<span class="mw-page-title-main">NGC 467</span> Galaxy in the constellation Pisces

NGC 467 is an unbarred lenticular galaxy in the constellation Pisces. It was discovered on 8 October 1785 by William Herschel.

<span class="mw-page-title-main">NGC 74</span> Galaxy in the constellation Andromeda

NGC 74 is a lenticular galaxy located in the Andromeda constellation. It was discovered on 7 October 1855 by Irish astronomer William Parsons.

<span class="mw-page-title-main">NGC 75</span> Galaxy in the constellation Pisces

NGC 75 is a lenticular galaxy estimated to be about 260 million light-years away in the constellation of Pisces. It was discovered by Lewis A. Swift from the USA in 1886 and its magnitude is 13.2.

NGC 7759 is a lenticular galaxy in the constellation Aquarius. It is located about 340 million light-years away from the Sun. It was discovered independently by American astronomers Lewis A. Swift and Francis Preserved Leavenworth.

<span class="mw-page-title-main">NGC 113</span> Galaxy in the constellation Cetus

NGC 113 is an unbarred lenticular galaxy located in the constellation Cetus. It was discovered by German astronomer, Ernst Wilhelm Leberecht Tempel, on August 27, 1876.

<span class="mw-page-title-main">NGC 115</span> Galaxy in the constellation of Sculptor

NGC 115 is a barred spiral galaxy located in the southern constellation of Sculptor. It was discovered by the British astronomer John Herschel on September 25, 1834. The galaxy is approximately 85 million light-years from the Sun, and is about 50,000 light-years in diameter, nearly half the size of our home galaxy, the Milky Way.

<span class="mw-page-title-main">NGC 116</span> Galaxy in the constellation Cetus

NGC 116 is a possibly lost or "non-existent" object in the constellation Cetus. This object is up for debate and has been considered to possibly be PGC 1671. The NED entry for this object contains the note NGC identification is very uncertain.

<span class="mw-page-title-main">NGC 479</span> Spiral galaxy in the constellation Pisces

NGC 479 is a spiral galaxy in the constellation Pisces. It was discovered by German astronomer Albert Marth on October 27, 1864. It is about 240 million light-years away from Earth.

NGC 7812 as is an intermediate spiral galaxy in the constellation Sculptor. The galaxy was discovered on 25 September 1865 by Sir John Hershel. At its widest, it measures approximately 100-thousand light years across, and is 315 million light years away from Earth.

<span class="mw-page-title-main">NGC 531</span> Galaxy in the constellation Andromeda

NGC 531 is a barred spiral galaxy in the constellation Andromeda with a visual magnitude of 10.51. It is a distance of 65.7 Mpc from the Sun. It is a member of the Hickson Compact Group HCG 10, and is interacting with the other members of the group.

<span class="mw-page-title-main">NGC 3902</span> Spiral galaxy in the constellation Leo

NGC 3902 is an intermediate spiral galaxy in the constellation Leo. It was discovered on April 6, 1785, by William Herschel and observed on February 19, 1827, by John Herschel. It is estimated to be 180 to 185 million light-years away, and its redshift-independent distance estimates to about 185 to 240 million light-years. It is around 75,000 light-years in diameter.

References

  1. 1 2 Skrutskie, Michael F.; Cutri, Roc M.; Stiening, Rae; Weinberg, Martin D.; Schneider, Stephen E.; Carpenter, John M.; Beichman, Charles A.; Capps, Richard W.; Chester, Thomas; Elias, Jonathan H.; Huchra, John P.; Liebert, James W.; Lonsdale, Carol J.; Monet, David G.; Price, Stephan; Seitzer, Patrick; Jarrett, Thomas H.; Kirkpatrick, J. Davy; Gizis, John E.; Howard, Elizabeth V.; Evans, Tracey E.; Fowler, John W.; Fullmer, Linda; Hurt, Robert L.; Light, Robert M.; Kopan, Eugene L.; Marsh, Kenneth A.; McCallon, Howard L.; Tam, Robert; Van Dyk, Schuyler D.; Wheelock, Sherry L. (1 February 2006). "The Two Micron All Sky Survey (2MASS)". The Astronomical Journal. 131 (2): 1163–1183. Bibcode:2006AJ....131.1163S. doi: 10.1086/498708 . ISSN   0004-6256. S2CID   18913331.
  2. 1 2 3 "NGC 12". SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 17 January 2017.
  3. 1 2 "Search specification: NGC 12". HyperLeda. Université Claude Bernard Lyon 1. Retrieved 2021-02-10.
  4. "Results for object NGC 0012 (NGC 12)". NASA/IPAC Extragalactic Database. California Institute of Technology. Retrieved 2021-02-10.
  5. 1 2 Seligman, Courtney. "NGC 12". Celestial Atlas. Retrieved 6 November 2018.