NGC 172
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Appearance
From Wikipedia, the free encyclopedia
Barred spiral galaxy in the constellation Cetus
NGC 172 | |
---|---|
NGC 172 as seen on SDSS | |
Observation data (J2000 epoch) | |
Constellation | Cetus |
Right ascension | 00h 37m 13.6s[1] |
Declination | −22° 35′ 13″[1] |
Redshift | 0.010164[1] |
Distance | 136 Mly [2] |
Apparent magnitude (V) | 15.09[1] |
Characteristics | |
Type | SB(r)bc?[1] |
Apparent size (V) | 2.0' ×ばつ 0.3'[1] |
Other designations | |
ESO 474- G 005, MCG -04-02-027, 2MASX J00371359-2235132, 2MASXi J0037135-223513, IRAS 00348-2251, IRAS F00347-2012, ESO-LV 4740050, 6dF J0037136-223513, PGC 2228.[1] |
NGC 172 is a barred spiral galaxy located around 136 million light-years away[2] in the constellation Cetus.[1] It was discovered in 1886 by astronomer Frank Muller.[3]
See also
[edit ]References
[edit ]- ^ a b c d e f g h "Results for NGC 0172". NASA/IPAC Extragalactic Database. Retrieved 2016年09月02日.
- ^ 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
- ^ "New General Catalog Objects: 150 - 199". cseligman.com. Retrieved 2018年02月13日.
External links
[edit ]- Media related to NGC 172 at Wikimedia Commons
- NGC 172 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
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