NGC 80

Last updated

"Legacy Survey Sky Browser". www.legacysurvey.org. Retrieved 2023-05-19.

NGC 80
NGC80 - SDSS DR14.jpg
SDSS image of NGC 80
Observation data (J2000 epoch)
Constellation Andromeda
Right ascension 00h 21m 10.865s [1]
Declination +22° 21 26.11 [1]
Redshift 0.019006
Heliocentric radial velocity 5698 [2]
Distance 260.76 ± 66.60  Mly (79.950 ± 20.421  Mpc) [2]
Group or cluster NGC 80 group [3]
Apparent magnitude  (V)12.07 [2]
Apparent magnitude  (B)13.7 [4]
Absolute magnitude  (V)−22.38 [2]
Characteristics
Type SA0 [2]
Size166,900  ly (51,160  pc) [2]
Apparent size  (V)2.2 × 2.002 [2]
Other designations
UGC 203, MCG+04-02-004, PGC 1351 [4]

NGC 80 is a lenticular galaxy located in the constellation Andromeda. It is interacting with NGC 47 and NGC 68, and is the brightest cluster galaxy of the NGC 80 group, a galaxy group named after it. [3]

NGC 80 group members: [5]

Image of the NGC 80 group taken by amateur astronomers at the Observatory of Saint-Veran. NGC80 Galaxy Group.png
Image of the NGC 80 group taken by amateur astronomers at the Observatory of Saint-Veran.

Related Research Articles

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<span class="mw-page-title-main">NGC 950</span> Galaxy in the constellation Cetus

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<span class="mw-page-title-main">NGC 810</span> Elliptical galaxy in the constellation Cetus

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<span class="mw-page-title-main">NGC 790</span> Galaxy in the constellation Cetus

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.

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<span class="mw-page-title-main">NGC 906</span> Galaxy in the constellation Andromeda

NGC 906 is a barred spiral galaxy in the constellation Andromeda in the northern sky. It is estimated to be 215 million light years from the Milky Way and has a diameter of approximately 110,000 ly. NGC 906 was discovered on October 30, 1878 by astronomer Édouard Stephan.

<span class="mw-page-title-main">NGC 813</span> Lenticular galaxy in the constrellation Hydrus

NGC 813 is a lenticular galaxy in the constellation Hydrus. It is estimated to be 390 million light-years from the Milky Way and has a diameter of approximately 140,000 ly. NGC 813 was discovered on November 24, 1834 by the British astronomer John Herschel.

<span class="mw-page-title-main">NGC 804</span> Lenticular galaxy in the constellation Triangulum

NGC 804 is a lenticular galaxy located in the Triangulum constellation about 231 million light-years from the Milky Way. It was discovered by the American astronomer Lewis Swift in 1885. This galaxy was also observed by the French astronomer Guillaume Bigourdan on December 24, 1897, and it has been added to the Index Catalogue under the symbol IC 1773.

<span class="mw-page-title-main">NGC 941</span> Spiral galaxy in the constellation Triangulum

NGC 941 is an intermediate spiral galaxy in the constellation Triangulum. It is an estimated 55 million light-years from the Milky Way and has a diameter of approximately 55,000 light years. The galaxies NGC 926, NGC 934, NGC 936, NGC 955 are located in the same sky area. NGC 941 was discovered by the astronomer William Herschel on 6 January 1785.

<span class="mw-page-title-main">NGC 821</span> Galaxy in the constellation Aries

NGC 821 is an elliptical galaxy in the constellation Aries. It is estimated to be about 80 million light-years from the Milky Way and has a diameter of approximately 55,000 light years. NGC 821 was discovered on September 4, 1786, by astronomer Wilhelm Herschel.

<span class="mw-page-title-main">NGC 736</span> Galaxy in the constellation Triangulum

NGC 736 is an elliptical galaxy in the constellation Triangulum. It is an estimated 200 million light years from the Milky Way and has a diameter of approximately 85,000 light years. NGC 736 was discovered on September 12, 1784 by the German-British astronomer William Herschel.

<span class="mw-page-title-main">NGC 766</span> Galaxy in the constellation Pisces

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<span class="mw-page-title-main">NGC 644</span> Galaxy in the constellation of Phoenix

NGC 644 is a barred spiral galaxy in the constellation Phoenix in the southern sky. It is estimated to be 270 million light-years from the Milky Way and has a diameter of approximately 130,000 light-years. Together with NGC 641, it probably forms a gravitationally bound pair of galaxies. The object was discovered on September 5, 1834 by John Herschel.

<span class="mw-page-title-main">NGC 623</span> Large elliptical galaxy in the constellation Sculptor

NGC 623 is a large elliptical galaxy located in the Sculptor constellation at a distance of about 400 million light-years away from the Milky Way. It was discovered by British astronomer John Herschel in 1837.

<span class="mw-page-title-main">NGC 861</span> Spiral galaxy in the constellation Triangulum

NGC 861 is a spiral galaxy in the constellation Triangulum. It is estimated to be 360 million light-years from the Milky Way and has a diameter of approximately 165,000 light-years. The object was discovered on September 18, 1865 by Heinrich d'Arrest.

<span class="mw-page-title-main">NGC 6375</span> Galaxy in the constellation Hercules

NGC 6375 is a galaxy in the New General Catalog. It is located in the sky within the constellation Hercules. It is an E0 type lenticular, elliptical galaxy. It was discovered by German astronomer Albert Marth in 1864 with a mirror type telescope with a diameter of 121.92 cm.

<span class="mw-page-title-main">NGC 3818</span> Elliptical galaxy in the constellation Virgo

NGC 3818 is an elliptical galaxy in the Constellation Virgo. It is at a distance of about 118 million light-years away from Earth. In the center of NGC 3818 lies a supermassive black hole. NGC 3818 was discovered by William Herschel on March 5, 1785.

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 4 5 6 7 "NED Results for NGC 0080". NASA/IPAC Extragalactic Database. Retrieved 18 February 2017.
  3. 1 2 Silchenko, Olga K.; Afanasiev, Victor L. (2008). "Stellar populations and galaxy evolution in the NGC 80 group". arXiv: 0807.0334 [astro-ph].
  4. 1 2 "NGC 80". SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 18 February 2017.
  5. "Legacy Survey Sky Browser". www.legacysurvey.org. Retrieved 2023-05-19.