NGC 218
Appearance
(Redirected from UGC 480)
UGC 480 | |
---|---|
Observation data (J2000 epoch) | |
Constellation | Andromeda |
Right ascension | 00h 46m 32.0s[1] |
Declination | +36° 19′ 32″[1] |
Redshift | 0.037426[1] |
Distance | ~500 Mly[2] |
Apparent magnitude (V) | 13.50[1] |
Apparent magnitude (B) | 13.6[3] |
Characteristics | |
Type | S[1] |
Apparent size (V) | 1.5' × 1.2'[1] |
Other designations | |
UGC 480, UGC 480 W, CGCG 519-021, MCG +06-02-016, VV 527A, KPG 16A, 2MASX J00463200+3619318, 2MASXi J0046319+361932, IRAS 00438+3603, F00437+3603, PGC 2720.[1] |
NGC 218, also known as UGC 480, is a spiral galaxy located approximately 500 million light-years from the Sun[2] in the constellation Andromeda. It was discovered on October 17, 1876 by Édouard Stephan, and is interacting with the galaxy PGC 2726.[4]
See also
[edit]References
[edit]- ^ a b c d e f g "NASA/IPAC Extragalactic Database". Results for NGC 0218. Retrieved 2016-09-02.
- ^ a b An object's distance from Earth can be determined using Hubble's law: v=Ho is Hubble's constant (70±5 (km/s)/Mpc). The relative uncertainty Δd/d divided by the distance is equal to the sum of the relative uncertainties of the velocity and v=Ho
- ^ "UGC 480". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 21 February 2017.
- ^ "New General Catalog Objects: NGC 200 - 249". Cseligman. Retrieved September 10, 2016.
External links
[edit]- Media related to NGC 218 at Wikimedia Commons
- NGC 218 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
- SEDS