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| NGC 277 | |
|---|---|
 SDSS image of NGC 277 | |
| Observation data (J2000epoch) | |
| Constellation | Cetus |
| Right ascension | 00h 51m 17.2s[1] |
| Declination | −08° 35′ 49″[1] |
| Redshift | 0.014283[1] |
| Heliocentric radial velocity | 4,282 km/s[1] |
| Apparent magnitude (V) | 14.31[1] |
| Characteristics | |
| Type | S0[1] |
| Apparent size (V) | 1.4' × 1.2'[1] |
| Other designations | |
| MCG -02-03-028,2MASX J00511725-0835485,6dF J0051172-083549,PGC 2995.[1] | |
NGC 277 is alenticular galaxy located in the constellationCetus. It was discovered on October 8, 1864, by the German astronomerHeinrich Louis d'Arrest.[2] The galaxy is situated near the celestial equator, making it observable from both the Northern and Southern Hemispheres at various times of the year. With an apparent B magnitude of 13, NGC 277 requires a telescope with an aperture of at least 10 inches (250 mm) for proper observation.
As a lenticular galaxy, NGC 277 exhibits characteristics between those ofelliptical andspiral galaxies, featuring a prominent central bulge and a disk-like structure but lacking significant spiral arm features. Its precise distance fromEarth is not well-documented in readily available sources, which is common for many galaxies cataloged in the 19th century. The galaxy's position and brightness make it a subject of interest for amateur astronomers equipped with sufficiently powerful telescopes.
For those interested in observing NGC 277, it is recommended to consult star charts and plan observations during times when Cetus is prominently positioned in the night sky, typically during the months of October through December. Due to its faintness, observing from a location with minimal light pollution will enhance visibility.[3]
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