NGC 2803

Last updated
NGC 2803
NGC 2802 NGC 2803 legacy dr10.jpg
legacy surveys image of NGC 2802 (upper right) and NGC 2803 (lower left)
Observation data (J2000 epoch)
Constellation Cancer
Right ascension 09h 16m 43.86892s [1]
Declination +18° 57 16.4866 [1]
Redshift 0.030158 [2]
Heliocentric radial velocity 8905 km/s [2]
Distance 411.1  Mly (126.04  Mpc) [3]
Apparent magnitude  (V)15.16 [4]
Characteristics
Type E-SB0 [4]
Other designations
UGC 4898, MCG +03-24-027, PGC 26181 [2]

NGC 2803, also known as PCG 26181, [2] is an elliptical or lenticular galaxy in the zodiac constellation Cancer. It was discovered March 21, 1784, by William Herschel. It is interacting with NGC 2802. [5]

One supernova has been observed in NGC 2803: SN 2017ilf (type Ia, mag. 18). [6]

Related Research Articles

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<span class="mw-page-title-main">NGC 5034</span> Spiral galaxy in the constellation Ursa Minor

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<span class="mw-page-title-main">NGC 3258</span> Galaxy in the constellation Antlia

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<span class="mw-page-title-main">NGC 3260</span> Galaxy in the constellation Antlia

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<span class="mw-page-title-main">NGC 151</span> Galaxy in the constellation Cetus

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<span class="mw-page-title-main">NGC 119</span> Unbarred lenticular galaxy in Phoenix

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<span class="mw-page-title-main">NGC 214</span> Galaxy in the constellation Andromeda

NGC 214 is a spiral galaxy in the northern constellation of Andromeda, located at a distance of 194 megalight-years from the Milky Way. It was discovered on September 10, 1784 by William Herschel. The shape of this galaxy is given by its morphological classification of SABbc, which indicates a weak bar-like structure (SAB) at the core and moderate to loosely-wound spiral arms (bc).

<span class="mw-page-title-main">NGC 4424</span> Spiral galaxy in the constellation Virgo

NGC 4424 is a spiral galaxy located in the equatorial constellation of Virgo. It was discovered February 27, 1865 by German astronomer Heinrich Louis d'Arrest. This galaxy is located at a distance of 13.5 million light years and is receding with a heliocentric radial velocity of 442 km/s. It has a morphological class of SB(s)a, which normally indicates a spiral galaxy with a barred structure (SB), no inner ring feature (s), and tightly-wound spiral arms (a). The galactic plane is inclined at an angle of 62° to the line of sight from the Earth. It is a likely member of the Virgo Cluster of galaxies.

<span class="mw-page-title-main">NGC 4500</span> Galaxy in the constellation Ursa Major

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<span class="mw-page-title-main">NGC 7199</span> Galaxy in the constellation Indus

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<span class="mw-page-title-main">NGC 1310</span> Galaxy in the constellation Fornax

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<span class="mw-page-title-main">NGC 999</span> Galaxy in the constellation Andromeda

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<span class="mw-page-title-main">NGC 995</span> Galaxy in the constellation Andromeda

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<span class="mw-page-title-main">NGC 940</span> Galaxy in the constellation Triangulum

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<span class="mw-page-title-main">NGC 938</span> Galaxy in the constellation Aries

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<span class="mw-page-title-main">NGC 823</span> Galaxy in the constellation Fornax

NGC 823, also known as IC 1782, is an unbarred lenticular galaxy in the constellation Fornax. It is estimated to be 194 million light-years from the Milky Way and has a diameter of approximately 100,000 light years. NGC 823 was discovered on October 14, 1830, by astronomer John Herschel.

<span class="mw-page-title-main">NGC 1325</span> Galaxy in the constellation Eridanus

NGC 1325 is a flocculent spiral galaxy situated in the constellation of Eridanus. Located about 75 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 19 December 1799.

<span class="mw-page-title-main">NGC 4614</span> Galaxy in the constellation Coma Berenices

NGC 4614 is a barred lenticular galaxy in the New General Catalog. It is located in the constellation of Coma Berenices. It was discovered in 1864 by the German astronomer Heinrich d'Arrest with a 11.9 inch diameter lens type telescope.

<span class="mw-page-title-main">NGC 1001</span> Galaxy in the constellation Perseus

NGC 1001 is an unbarred spiral galaxy in the constellation Perseus. It was discovered on December 8, 1871 by the astronomer Édouard Stephan.

References

  1. 1 2 Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics . 616. A1. arXiv: 1804.09365 . Bibcode: 2018A&A...616A...1G . doi: 10.1051/0004-6361/201833051 .
  2. 1 2 3 4 "NGC 2803". SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 2021-02-14.
  3. Crook, Aidan C.; Huchra, John P.; Martimbeau, Nathalie; Masters, Karen L.; Jarrett, Tom; Macri, Lucas M. (2007). "Groups of Galaxies in the Two Micron All Sky Redshift Survey". The Astrophysical Journal. 655 (2): 790–813. arXiv: astro-ph/0610732 . Bibcode:2007ApJ...655..790C. doi:10.1086/510201. S2CID   11672751.
  4. 1 2 "Search specification: NGC 2803". HyperLeda. Université Claude Bernard Lyon 1. Retrieved 2021-02-14.
  5. Seligman, Courtney. "New General Catalogue objects: NGC 2800 - 2849". cseligman.com. Retrieved 2021-02-14.
  6. Transient Name Server entry for SN 2017ilf. Retrieved 25 March 2023.