NGC 3718

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NGC 3718
NGC 3718 HST.jpg
NGC 3718
Observation data (J2000.0 epoch)
Constellation Ursa Major
Right ascension 11h 32m 34.940s [1]
Declination +53° 04 04.18 [1]
Redshift 0.003306 [2]
Distance 47.84 ± 8.54  Mly (14.667 ± 2.618  Mpc) [3]
Apparent magnitude  (V)10.61 [2]
Characteristics
Type SB(s)a pec [3]
Apparent size  (V)2.940″ × 2.352″ [1]
Other designations
Arp  214, UGC  6524, MCG+09-19-114, PGC  35616 [2]

NGC 3718, also called Arp 214, is a galaxy located approximately 52 million light years from Earth in the constellation Ursa Major. [4] [2] [5] It is either a lenticular or spiral galaxy. [6]

Contents

NGC 3718 exhibits a warped, S-shape similar to NGC 6872, possibly a result of gravitational interaction with NGC 3729, another spiral galaxy located 150,000 light-years away. [7]

NGC 3718 is a member of the Ursa Major Cluster. [8]

Hickson Compact Group

South of NGC 3718 the Hickson Compact Group #56 is located. HCG 56 is a compact group of galaxies of which 4 members are interacting with each other. This group is about 120 Mpc distant to our galaxy, [9] which is about 8 times more distant than NGC 3718.

Related Research Articles

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<span class="mw-page-title-main">NGC 1189</span> Galaxy in the constellation Eridanus

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<span class="mw-page-title-main">NGC 4607</span> Galaxy in the constellation Virgo

NGC 4607 is an edge-on spiral galaxy located about 56 million light-years away in the constellation Virgo. NGC 4607 was discovered by astronomer R. J. Mitchell on April 24, 1854. The galaxy is a member of the Virgo Cluster.

<span class="mw-page-title-main">NGC 6975</span> Galaxy in the constellation Aquarius

NGC 6975, also known as NGC 6976, is a spiral galaxy in the constellation Aquarius. The object was discovered on 12 July 1864 by the German astronomer Albert Marth.

<span class="mw-page-title-main">NGC 4222</span> Edge-on spiral galaxy in the constellation Coma Berenices

NGC 4222 is an edge-on spiral galaxy located about 60 million light-years away in the constellation Coma Berenices. It was discovered by astronomer William Herschel on April 8, 1784 and is often misidentified as IC 3087. NGC 4222 is a member of the Virgo Cluster and is a companion of NGC 4216 which lies about 180,000 ly (56 kpc) away. Despite this, the two galaxies are not interacting.

<span class="mw-page-title-main">NGC 2998</span> Galaxy in the constellation Ursa Major

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<span class="mw-page-title-main">NGC 753</span> Galaxy in the constellation Andromeda

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

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<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

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

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<span class="mw-page-title-main">NGC 3729</span> Galaxy in the constellation of Ursa Major

NGC 3729 is a barred spiral galaxy located in the constellation Ursa Major. It is located at a distance of circa 65 million light years from Earth, which, given its apparent dimensions, means that NGC 3729 is about 60,000 light years across. It was discovered by William Herschel on April 12, 1789.

<span class="mw-page-title-main">NGC 4294</span> Galaxy in the constellation Virgo

NGC 4294 is a barred spiral galaxy with flocculent spiral arms located about 55 million light-years away in the constellation Virgo. The galaxy was discovered by astronomer William Herschel on March 15, 1784 and is a member of the Virgo Cluster.

<span class="mw-page-title-main">NGC 4298</span> Galaxy in the constellation Coma Berenices

NGC 4298 is a flocculent spiral galaxy located about 53 million light-years away in the constellation Coma Berenices. The galaxy was discovered by astronomer William Herschel on April 8, 1784 and is a member of the Virgo Cluster.

<span class="mw-page-title-main">NGC 4299</span> Spiral galaxy in the constellation Virgo

NGC 4299 is a featureless spiral galaxy located about 55 million light-years away in the constellation Virgo. It was discovered by astronomer William Herschel on March 15, 1784 and is a member of the Virgo Cluster.

<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 5910</span> Galaxy in the constellation of Serpens

NGC 5910 is an elliptical galaxy located about 540 million light-years away in the constellation Serpens. It was discovered by astronomer William Hershel on April 13, 1785. NGC 5910 is also a strong radio source with a conspicuous nuclear jet.

References

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  2. 1 2 3 4 "NGC 3718". SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 8 December 2017.
  3. 1 2 "NED results for object NGC 3718". National Aeronautics and Space Administration / Infrared Processing and Analysis Center . Retrieved 8 December 2017.
  4. Nemiroff, R.; Bonnell, J., eds. (31 August 2006). "Extra Galaxies". Astronomy Picture of the Day . NASA.
  5. "Best of AOP: NGC 3718". noao.edu. Archived from the original on 2015-05-24. Retrieved 2015-01-26.
  6. "NGC 3718, Spiral Galaxy". kopernik.org.
  7. "APOD: 2013 August 3 - Twisting with NGC 3718".
  8. Tully, R. Brent; Verheijen, Marc A. W.; Pierce, Michael J.; Huang, Jia-Sheng; Wainscoat, Richard J. (December 1996). "The Ursa Major Cluster of Galaxies.I.Cluster Definition and Photometric Data". The Astronomical Journal. 112: 2471. arXiv: astro-ph/9608124 . Bibcode:1996AJ....112.2471T. doi:10.1086/118196. ISSN   0004-6256. S2CID   7875515.
  9. "By Name | NASA/IPAC Extragalactic Database". ned.ipac.caltech.edu. Retrieved 2023-08-06.