|Observation data (J2000 epoch)|
|Right ascension||03h 09m 45.5s|
|Declination||−20° 34′ 46″|
|Helio radial velocity||1603 ± 1 km/s|
|Distance||61 ± 8.5 Mly
(18.7 ± 2.6 Mpc)
|Apparent magnitude (V)||10.9|
|Apparent size (V)||7′.4 × 6′.5|
|Notable features||large satellite|
|PGC 11819, Arp 41|
It is dominated by millions of bright stars and dark dust, in spiral arms rotating about the center. Open clusters containing bright blue stars are sprinkled along these spiral arms, with dark lanes of dense interstellar dust between. Less visible are dim normal stars and interstellar gas, producing such high mass that they dominate the dynamics of the inner galaxy. Not visible is matter of unknown form called dark matter, needed to explain the motions of the visible material in the outer galaxy. The galaxy is approximately 200,000 light-years across, in between the sizes of the Andromeda Galaxy and our home galaxy, the Milky Way.
NGC 1232A is a satellite galaxy of NGC 1232. It is thought to be the cause of unusual bending in the spiral arms. In 1988, NGC 1232A was estimated to be 68 million light-years away while NGC 1232 was estimated to be 65 million light-years away.
- "NASA/IPAC Extragalactic Database". Results for NGC 1232. Retrieved 2006-11-25.
- "Distance Results for NGC 1232". NASA/IPAC Extragalactic Database. Retrieved 2010-06-22.
- "NASA/IPAC Extragalactic Database". Results for NGC 1232A. Retrieved 2010-06-22.
- "Distance Results for NGC 1232A". NASA/IPAC Extragalactic Database. Retrieved 2010-06-22.
|Wikimedia Commons has media related to NGC 1232.|
- NGC 1232 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
- SIMBAD: NGC 1232
- SIMBAD: NGC 1232A
- Antilhue-Chile: NGC 1232 in Eridanus
- The Scale of the Universe (Astronomy Picture of the Day 2012 March 12)