NGC 118

Last updated
NGC 118
NGC118 - SDSS DR14.jpg
SDSS image of NGC 118
Observation data (J2000 epoch)
Constellation Cetus
Right ascension 00h 27m 16.222s [1]
Declination −01° 46 48.50 [1]
Redshift 0.037329 [2]
Heliocentric radial velocity 10982 km/s [2]
Distance 524.5 ± 36.9  Mly (160.81 ± 11.30  Mpc) [1]
Apparent magnitude  (V)14.83 [3]
Apparent magnitude  (B)14.63 [3]
Characteristics
Type S(rs)a? pec [4]
Other designations
UGC 264, MCG +00-02-032, Mrk 947, PGC 1678 [2]

NGC 118 is a spiral galaxy of type S(rs)a? pec with an apparent magnitude of 13.6 located in the constellation Cetus. It was discovered on September 23, 1867, by the astronomer Truman Safford. [4]

Contents

See also

Related Research Articles

<span class="mw-page-title-main">NGC 13</span> Galaxy in the constellation Andromeda

NGC 13 is a spiral galaxy in the constellation Andromeda. It is estimated to be about 220 million light-years away from the Sun. It was discovered on November 26, 1790, by William Herschel.

<span class="mw-page-title-main">NGC 27</span> Galaxy in the constellation Andromeda

NGC 27 is a spiral galaxy located in the constellation Andromeda. It was discovered on 3 August 1884 by Lewis Swift. It forms a galaxy pair with the nearby UGC 95.

<span class="mw-page-title-main">NGC 1725</span> Elliptical galaxy in the constellation Eridanus

NGC 1725 is a lenticular 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 321</span> Elliptical galaxy in the Cetus constellation

NGC 321 is an elliptical galaxy located in the constellation Cetus. It was discovered on September 27, 1864, by the astronomer Albert Marth. Measurements of its redshift put it at a distance of about 217.4 ± 15.4 megalight-years (66.67 ± 4.73 Mpc), assuming a Hubble constant of H0 = 67.8 km/sec/Mpc.

<span class="mw-page-title-main">NGC 248</span> Emission nebula in the constellation Tucana

NGC 248 is an emission nebula in the constellation Tucana. It is in the Small Magellanic Cloud. It was discovered in 1834 by the astronomer John Frederick William Herschel. NGC 248 is about 60 light-years long and 20 light-years wide.

<span class="mw-page-title-main">NGC 63</span> Galaxy in the constellation Pisces

NGC 63 is a spiral galaxy in the constellation Pisces. NGC 63 is its New General Catalogue designation. It has an apparent V-band magnitude of 12.70.

<span class="mw-page-title-main">NGC 69</span> Galaxy in the constellation Andromeda

NGC 69 is a barred lenticular galaxy located in the constellation Andromeda. It is a member of the NGC 68 group. It was discovered in 1855 by R. J. Mitchell, who described it as "extremely faint, very small, round."

<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.

<span class="mw-page-title-main">NGC 117</span> Lenticular galaxy in the constellation Cetus

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.

<span class="mw-page-title-main">NGC 120</span> Galaxy in the constellation Cetus

NGC 120 is a lenticular galaxy of type SB0? pec? with an apparent magnitude of 13.4 located in the constellation Cetus. It was discovered on 27 September 1880 by Wilhelm Tempel.

<span class="mw-page-title-main">NGC 471</span> Galaxy in the constellation Pisces

NGC 471 is a lenticular galaxy located about 168 million light-years away from Earth in the constellation Pisces. It was discovered by the German astronomer Albert Marth on November 3, 1864.

<span class="mw-page-title-main">NGC 4469</span> Spiral galaxy in the constellation of Virgo

NGC 4469 is a nearly edge-on spiral galaxy located about 55 million light-years away in the constellation of Virgo. It is also classified as a LINER galaxy. NGC 4469 was discovered by astronomer William Herschel on April 15, 1784. It is a member of the Virgo Cluster.

<span class="mw-page-title-main">NGC 4074</span> Galaxy in the constellation Coma Berenices

NGC 4074 is a peculiar lenticular galaxy located 310 million light-years away in the constellation Coma Berenices. It was discovered by astronomer William Herschel on April 27, 1785 and is a member of the NGC 4065 Group.

<span class="mw-page-title-main">NGC 4086</span> Galaxy in the constellation Coma Berenices

NGC 4086 is a lenticular galaxy located 330 million light-years away in the constellation Coma Berenices. NGC 4086 was discovered by astronomer Heinrich d'Arrest on May 2, 1864 and is a member of the NGC 4065 Group.

<span class="mw-page-title-main">NGC 4090</span> Galaxy in the constellation Coma Berenices

NGC 4090 is a spiral galaxy located 340 million light-years away in the constellation Coma Berenices. The galaxy was discovered by astronomer Heinrich d'Arrest on May 2, 1864 and is a member of the NGC 4065 Group.

<span class="mw-page-title-main">NGC 4091</span> Galaxy in the constellation Coma Berenices

NGC 4091 is a spiral galaxy located 360 million light-years away in the constellation Coma Berenices. The galaxy was discovered by astronomer Heinrich d'Arrest on May 2, 1864. NGC 4091 is a member of the NGC 4065 Group and is a LINER galaxy.

<span class="mw-page-title-main">NGC 4092</span> Galaxy in the constellation Coma Berenices

NGC 4092 is a spiral galaxy located 310 million light-years away in the constellation Coma Berenices. It was discovered by astronomer Heinrich d'Arrest on May 2, 1864. NGC 4092 is a member of the NGC 4065 Group and hosts an AGN.

<span class="mw-page-title-main">NGC 4095</span> Galaxy in the constellation Coma Berenices

NGC 4095 is an elliptical galaxy located 330 million light-years away in the constellation Coma Berenices. The galaxy was discovered by astronomer William Herschel on April 26, 1785. NGC 4095 is a member of the NGC 4065 Group and is a LINER.

<span class="mw-page-title-main">NGC 4098</span> Interacting galaxies in the constellation Coma Berenices

NGC 4098 is an interacting pair of spiral galaxies located 330 million light-years away in the constellation Coma Berenices. NGC 4098 was discovered by astronomer William Herschel on April 26, 1785. It was then rediscovered by Hershel on December 27, 1786 was listed as NGC 4099. NGC 4098 is a member of the NGC 4065 Group.

References

  1. 1 2 3 "Results for object NGC 0118 (NGC 118)". NASA/IPAC Extragalactic Database. California Institute of Technology. Retrieved 2021-02-24.
  2. 1 2 3 "NGC 118". SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 2021-02-24.
  3. 1 2 "Search specification: NGC 118". HyperLeda. Université Claude Bernard Lyon 1. Retrieved 2021-02-24.
  4. 1 2 Seligman, Courtney. "New General Catalogue objects: NGC 100 - 149". cseligman.com. Retrieved 2021-02-24.