| NGC 441 | |
|---|---|
 NGC 441 as seen by
DECam | |
| Observation data ( J2000 epoch) | |
| Constellation | Sculptor |
| Right ascension | 01h 13m 51.2s [1] |
| Declination | −31° 47′ 18″ [1] |
| Redshift | 0.018800 [1] |
| Heliocentric radial velocity | 5,636 km/s [1] |
| Apparent magnitude (V) | 13.62 [1] |
| Absolute magnitude (V) | -22.19 [1] |
| Characteristics | |
| Type | (R')SB(rs)0/a? [1] |
| Apparent size (V) | 1.4' × 1.1' [1] |
| Other designations | |
| ESO 412- G 019, MCG -05-04-016, 2MASX J01135125-3147180, 2MASXi J0113512-314718, IRAS F01115-3202, ESO-LV 4120190, PGC 4429, PGC 701033. [1] | |
NGC 441 is a lenticular galaxy of type (R')SB(rs)0/a? located in the constellation Sculptor. It was discovered on September 27, 1834, by John Herschel. It was described by Dreyer as "prety faint, small, round, gradually brighter middle." [2]
References
External links
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Media related to
NGC 441 at Wikimedia Commons
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.jpg){kind=small} | This lenticular galaxy article is a stub. You can help Wikipedia by expanding it. |
| NGC 441 | |
|---|---|
|
NGC 441 as seen by
DECam | |
| Observation data ( J2000 epoch) | |
| Constellation | Sculptor |
| Right ascension | 01h 13m 51.2s [1] |
| Declination | −31° 47′ 18″ [1] |
| Redshift | 0.018800 [1] |
| Heliocentric radial velocity | 5,636 km/s [1] |
| Apparent magnitude (V) | 13.62 [1] |
| Absolute magnitude (V) | -22.19 [1] |
| Characteristics | |
| Type | (R')SB(rs)0/a? [1] |
| Apparent size (V) | 1.4' × 1.1' [1] |
| Other designations | |
| ESO 412- G 019, MCG -05-04-016, 2MASX J01135125-3147180, 2MASXi J0113512-314718, IRAS F01115-3202, ESO-LV 4120190, PGC 4429, PGC 701033. [1] | |
NGC 441 is a lenticular galaxy of type (R')SB(rs)0/a? located in the constellation Sculptor. It was discovered on September 27, 1834, by John Herschel. It was described by Dreyer as "prety faint, small, round, gradually brighter middle." [2]
References
External links
-
Media related to
NGC 441 at Wikimedia Commons
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| Galaxies |
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| This lenticular galaxy article is a stub. You can help Wikipedia by expanding it. |