NGC 90

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NGC 90
N90s.jpg
NGC 90 (top center) and its spiral companion to the right, NGC 93
Observation data (J2000 epoch)
Constellation Andromeda
Right ascension 00h 21m 51.4s [1]
Declination +22° 24′ 00″ [1]
Redshift 0.017856 [2]
Helio radial velocity 5353 ± 10 km/s [2]
Distance 333.8 ± 146 Mly
(102.35 ± 44.76 Mpc) [2]
Apparent magnitude  (V)13.7 [3]
Characteristics
Type SAB(s)c pec [2]
Apparent size  (V)2.4' x 0.91' [2]
Other designations
UGC 208, MCG+04-02-011, PGC 1405, [2] Arp 65

NGC 90 is an interacting spiral galaxy estimated to be about 300 million light-years away in the constellation of Andromeda. It was discovered by R. J. Mitchell in 1854 and its apparent magnitude is 13.7. [3] The galaxy is currently interacting with NGC 93 and exhibits two highly elongated and distorted spiral arms with bright blue star clusters indicative of star formation, likely caused by the interaction with its neighbor.

NGC 90 and NGC 93 form the interacting galaxy pair Arp 65.

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<span class="mw-page-title-main">NGC 1134</span> Spiral galaxy in the constellation Aries

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<span class="mw-page-title-main">NGC 935 and IC 1801</span> Pair of interacting galaxies in the constellation Aries

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<span class="mw-page-title-main">NGC 5753</span> Galaxy in the constellation Boötes

NGC 5753 is a spiral galaxy in the constellation Boötes. This is a member of the Arp 297 interacting galaxies group of four: NGC 5752, NGC 5753, NGC 5754, NGC 5755.

<span class="mw-page-title-main">NGC 5614</span> Galaxy in the constellation Boötes

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<span class="mw-page-title-main">NGC 5613</span> Galaxy in the constellation Boötes

NGC 5613 is a lenticular galaxy in the constellation Boötes. It is part of the Arp 178 set of interacting galaxies, with NGC 5615 and NGC 5614.

<span class="mw-page-title-main">NGC 5545</span> Spiral galaxy in the constellation Boötes

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<span class="mw-page-title-main">NGC 5755</span> Galaxy in the constellation Boötes

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<span class="mw-page-title-main">NGC 5754</span> Galaxy in the constellation Boötes

NGC 5754 is a barred spiral galaxy located 218 million light years away in the constellation Boötes. It is a member of the Arp 297 interacting galaxies group, which consists of NGC 5752, NGC 5753, NGC 5754, NGC 5755. Along with NGC 2718 and UGC 12158, NGC 5754 is often considered a Milky Way-twin.

<span class="mw-page-title-main">NGC 5752</span> Galaxy in the constellation Boötes

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<span class="mw-page-title-main">NGC 5775</span> Spiral galaxy in the constellation Virgo

NGC 5775 is a spiral galaxy, a member of the Virgo Cluster, that lies at a distance of about 70 million light-years. Although the spiral is tilted away from us, with only a thin sliver in view, such a perspective can be advantageous for astronomers. For instance, astronomers have previously used the high inclination of this spiral to study the properties of the halo of hot gas that is visible when the galaxy is observed at X-ray wavelengths. It is a member of the NGC 5775 Group of galaxies, itself one of the Virgo III Groups strung out to the east of the Virgo Supercluster of galaxies.

<span class="mw-page-title-main">NGC 4634</span> Galaxy in the constellation Coma Berenices

NGC 4634 is an edge-on barred spiral galaxy located about 70 million light-years away in the constellation of Coma Berenices. NGC 4634 was discovered by astronomer William Herschel on January 14, 1787. It is interacting with the spiral galaxy NGC 4633. Both galaxies are members of the Virgo Cluster.

<span class="mw-page-title-main">NGC 80</span>

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

<span class="mw-page-title-main">NGC 78</span> A pair of spiral galaxies in the constellation Pisces

NGC 78 is a pair of galaxies in the constellation Pisces. NGC 78A, which is the more southern galaxy, is a barred spiral galaxy. NGC 78B, which is the more northern galaxy, is an elliptical galaxy. Although the designations NGC 78A and 78B are used today, the designation NGC 78 was formerly used mainly for the northern galaxy.

<span class="mw-page-title-main">NGC 3718</span> Galaxy in the constellation Ursa Major

NGC 3718, also called Arp 214, is a galaxy located approximately 52 million light years from Earth in the constellation Ursa Major. It is either a lenticular or spiral galaxy.

<span class="mw-page-title-main">NGC 85</span> Lenticular galaxy in the constellation Andromeda

NGC 85 is an interacting spiral or lenticular galaxy estimated to be about 200 million light-years away in the constellation of Andromeda. It was discovered by Ralph Copeland in 1873 and its apparent magnitude is 15.7. The galaxy appears to be interacting with the companion spiral IC 1546.

<span class="mw-page-title-main">NGC 93</span> Spiral galaxy in the constellation Andromeda

NGC 93 is an interacting spiral galaxy estimated to be about 260 million light-years away in the constellation of Andromeda. It was discovered by R. J. Mitchell in 1854. The galaxy is currently interacting with NGC 90 and has some signs of interacting with it.

<span class="mw-page-title-main">NGC 4402</span> Spiral galaxy in the constellation Virgo

NGC 4402 is a relatively near, edge-on spiral galaxy located around 50 million light-years from Earth. It is in the constellation of Virgo within the Virgo Cluster of galaxies. It can be seen when viewing Markarian's Chain.

<span class="mw-page-title-main">NGC 4861</span> Irregular galaxy in constellation Canes Venatici

NGC 4861, also known as Arp 266, is a galaxy in the constellation Canes Venatici. It was discovered by William Herschel on May 1, 1785.

<span class="mw-page-title-main">NGC 3921</span> Interacting galaxy in the constellation Ursa Major

NGC 3921 is an interacting galaxy in the northern constellation of Ursa Major. Estimates using redshift put it at about 59 million light years from Earth. It was discovered on 14 April 1789 by William Herschel, and was described as "pretty faint, small, round" by John Louis Emil Dreyer, the compiler of the New General Catalogue.

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 "NED results for object NGC 0090". National Aeronautics and Space Administration / Infrared Processing and Analysis Center. 2008. Retrieved 24 November 2008.
  3. 1 2 "NGC Objects: NGC 50 - 99".
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