Messier 77
(Redirected from Spiral Galaxy M77)
| Galaxy | List of galaxies |
|---|---|
 Spiral Galaxy M77 | |
| Observation data (Epoch J2000) | |
| Constellation | Cetus |
| Right ascension | 2h 42m 40.7s[1] |
| Declination | -00° 00′ 48″[1] |
| Redshift | 1137 ± 3 km/s[1] |
| Distance | 47.0 Mly[2] |
| Type | (R)SA(rs)b[1] |
| Apparent dimensions (V) | 7′.1 × 6′.0[1] |
| Apparent magnitude (V) | 9.6[1] |
| Notable features | One of the biggest galaxies of Messier's catalog. Inclination estimated to be 40°.[3] |
| Other designations | |
| | |
Messier 77 (also known as NGC 1068) is a barred spiral galaxy about 47.0 million light-years away in the constellation Cetus. It was discovered by Pierre Méchain in 1780. M77 is an active galaxy with an Active Galactic Nucleus (AGN), which is obscured from view by astronomical dust at visible wavelengths. The diameter of the molecular disk and hot plasma associated with the obscuring material was first measured at radio wavelengths by the VLBA and VLA. The hot dust around the nucleus was subsequently measured in the mid-infrared by the MIDI instrument at the VLTI.
External links
- Spiral Galaxy M77 @ SEDS Messier pages
- VLBA image of the month: radio continuum and water masers of NGC 1068
- Press release about VLTI observations of NGC 1068
- WIKISKY.ORG: SDSS image M77
References
- ^ a b c d e f g NASA/IPAC Extragalactic Database. Results for NGC 1068. Retrieved on 2006-11-18.
- ^ Pattern Speeds BIMA-SONG Galaxies with Molecule-Dominated ISMs Using the Tremaine-Weinberg Method. Bland-Hawthorn et al. (1997). Retrieved on 2006-08-31.
- ^ Pattern Speeds BIMA-SONG Galaxies with Molecule-Dominated ISMs Using the Tremaine-Weinberg Method. (Schinnerer et al. 2000). Retrieved on 2006-08-31.
Categories
Spiral galaxies | Unbarred spiral galaxies | Cetus constellation | Messier objects | NGC objects | UGC objects | PGC objects | Arp objects