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NGC 2217

Coordinates:Sky map06h 21m 40.35s, −27° 13′ 56.90″
From Wikipedia, the free encyclopedia
Galaxy in the constellation Canis Major
NGC 2217
Credit:ESO
Observation data (J2000epoch)
ConstellationCanis Major
Right ascension06h 21m 40.35s[1]
Declination−27° 13′ 56.90″[1]
Redshift0.005400[2]
Heliocentric radial velocity1619 km/s[2]
Distance73Mly 22.4Mpc[2]
Apparent magnitude (V)11.71[2]
Characteristics
Type(R)SB0+(rs)[2]
Apparent size (V)4.44 × 4.84[1]
Other designations
MCG -05-15-010,PGC 18883[2]

NGC 2217 is a intergalactic celestial object of about 100 thousand light-years across that lies roughly 65 million light years from Earth in the constellation ofCanis Major. It is part of the NGC 2217 Group of galaxies. It is classified as abarred spiral galaxy.

A notable feature is the swirling shape of this galaxy. In its very concentrated central region we can see a distinctive, very luminous bar of stars within an oval ring. Further out, a set of tightly wound spiral arms almost form a circular ring around thegalaxy. The galaxy is not very known as of now.

Central bars play an important role in the development of a galaxy. They can, for example, funnel gas towards the center of the galaxy, helping to feed a centralblack hole, or to form new stars.[1]

Onesupernova, SN 2017fzw (type Ia, mag. 17.1), was discovered in NGC 2217 on 9 August, 2017.[3]

References

[edit]
  1. ^abcdhttp://www.eso.org/public/images/potw1204a/ "ESO"
  2. ^abcdef"NASA/IPAC Extragalactic Database".Results for NGC 2217. RetrievedDecember 26, 2016.
  3. ^Transient Name Server entry for SN 2017fzw. Retrieved 24 March 2023.

https://stardate.org/radio/program/2022-02-06

External links

[edit]
  • Media related toNGC 2217 at Wikimedia Commons


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