NGC 3308

In this article, we will delve into the fascinating world of NGC 3308. From its origins to its relevance today, we will explore all aspects related to this topic. We will analyze its impact on society, its implications in different areas and the challenges it poses. Additionally, we will examine the latest trends, discoveries, and milestone advances in NGC 3308. Through this journey, we aim to provide a comprehensive and updated vision of NGC 3308, in order to enrich our knowledge and understanding of this exciting topic.
NGC 3308
legacy surveys image of NGC 3308
Observation data (J2000 epoch)
ConstellationHydra
Right ascension10h 36m 22.4s[1]
Declination−27° 26′ 17″[1]
Redshift0.011855[1]
Heliocentric radial velocity3554 km/s[1]
Distance174 Mly (53.3 Mpc)[1]
Group or clusterHydra Cluster
Apparent magnitude (V)12.94[1]
Characteristics
TypeSAB0-(s)?[1]
Size~108,100 ly (33.15 kpc) (estimated)[1]
Apparent size (V)1.7 x 1.3[1]
Other designations
ESO 501-34, MCG -4-25-32, PGC 31438[1]

NGC 3308 is a lenticular galaxy with a faint bar[2] located about 174 million light-years away[3] in the constellation Hydra.[4] NGC 3308 was discovered by astronomer John Herschel on March 24, 1835.[5][6] It is a member of the Hydra Cluster.[7]

See also

References

  1. ^ a b c d e f g h i j "NASA/IPAC Extragalactic Database". Results for NGC 3308. Retrieved 2018-05-03.
  2. ^ "Detailed Object Classifications". ned.ipac.caltech.edu. Retrieved 2018-05-04.
  3. ^ "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2018-05-04.
  4. ^ "Revised NGC Data for NGC 3308". spider.seds.org. Retrieved 2018-05-04.
  5. ^ Gottlieb, Steve. "Astronomy-Mall: Adventures In Deep Space NGC objects 3001-3999". Astronomy-Mall. Retrieved 2018-04-27.
  6. ^ "New General Catalog Objects: NGC 3300 - 3349". cseligman.com. Retrieved 2018-05-04.
  7. ^ Richter, O.-G. (February 1989). "The Hydra I cluster of galaxies. V - A catalogue of galaxies in the cluster area" (PDF). Astronomy and Astrophysics Supplement Series. 77: 237–256. Bibcode:1989A&AS...77..237R.


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