NGC 327
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NGC 327 | |
---|---|
Observation data (J2000 epoch) | |
Constellation | Cetus |
Right ascension | 00h 57m 55.3s[1] |
Declination | −05° 07′ 50″[1] |
Redshift | 0.018239[1] |
Heliocentric radial velocity | 5,468 km/s[1] |
Apparent magnitude (V) | 14.5b[1] |
Characteristics | |
Type | SBbc[1] |
Apparent size (V) | 1.6' × 0.7'[1] |
Other designations | |
MCG -01-03-047, 2MASX J00575536-0507495, 2MASXi J0057553-050749, IRAS F0053-0524, 6dF J0057554-050750, PGC 3462.[1] |
NGC 327 is a spiral galaxy in the constellation Cetus. Also known as "The Jamie Smith Star" (ISD0534203) and was discovered on September 27, 1864 by Albert Marth. It is described by Dreyer as "faint, small, extended."[2] It is nearby galaxies NGC 329, NGC 325 and NGC 321.
References
External links
- Media related to NGC 327 at Wikimedia Commons
Categories:
- Articles with short description
- Short description is different from Wikidata
- Use mdy dates from October 2016
- Commons category link from Wikidata
- NGC objects
- Astronomical objects discovered in 1864
- Cetus
- Barred spiral galaxies
- Discoveries by Albert Marth
- Principal Galaxies Catalogue objects
- All stub articles
- Spiral galaxy stubs