NGC 54
NGC 54 is an edge-on spiral galaxy in the constellation of Cetus. The galaxy was discovered by Wilhelm Tempel in 1886, and he defined it as "very faint, pretty small, round."[2] The galaxy is 90,000 light years in diameter,[2] making it slightly smaller than the Milky Way.
NGC 54 | |
---|---|
Observation data (2000.0 epoch) | |
Constellation | Cetus[1] |
Right ascension | 00h 15m 07.6s[2] |
Declination | 00° 07′ 58″[2] |
Redshift | 0.017802 [3] |
Heliocentric radial velocity | 5335 km/s[2] |
Distance | 240,000,000 ly[2] (78,000,000 Parsecs)[4] |
Apparent magnitude (V) | 13.7 [5] |
Characteristics | |
Type | SB(r)a [5] |
Size | 90,000[2] |
Apparent size (V) | 1.445' x 0.525' [6] |
Other designations | |
MCG -01-01-060 2MASX J00150767-070624 2MASXi J0015076-070623 IRAS F00125-0723 AKARI J0015076-070623 6dF J0015076-070624 6dF J0015077-070624 LDCE 0010 NED004 HDCE 0009 NED004 USGC S005 NED03 GSC 4670 00994 PGC 1011 NVSS J001507-070622[3] |
References
- "Category:NGC 54 - Wikimedia commons". Retrieved 2013-08-30.
- "New General Catalog Objects: NGC 50 - 99". Retrieved 2013-08-30.
- "NED search results for NGC 0054". Retrieved 2013-09-05.
- "Parsecs to Light Years Conversion Calculator". Retrieved 2013-09-05.
- "NGC 54 - DeepSkyPedia :: Astronomy". Archived from the original on 2016-03-03. Retrieved 2013-09-05.
- "NGC 54 - Galaxy - WIKISKY". Retrieved 2013-09-05.
External links
- Media related to NGC 54 at Wikimedia Commons
- NGC 54 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
- SEDS
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