NGC 3776
| Galaxie NGC 3776 | |
|---|---|
| SDSS-Aufnahme | |
| AladinLite | |
| Sternbild | Jungfrau |
| Position Äquinoktium: J2000.0, Epoche: J2000.0 | |
| Rektaszension | 11h 38m 18,0s [1] |
| Deklination | −03° 21′ 16″ [1] |
| Erscheinungsbild | |
| Morphologischer Typ | Sa Ring?[1] |
| Helligkeit (visuell) | 14,7 mag[2] |
| Helligkeit (B-Band) | 15,5 mag[2] |
| Winkelausdehnung | 0,3' × 0,2'[2] |
| Positionswinkel | 155°[2] |
| Flächenhelligkeit | 11,5 mag/arcmin²[2] |
| Physikalische Daten | |
| Rotverschiebung | 0.037829 ± 0.000094[1] |
| Radialgeschwindigkeit | (11341 ± 28) km/s[1] |
| Hubbledistanz H0 = 73 km/(s • Mpc) |
(501 ± 35)e6 Lj (153,6 ± 10,8) Mpc [1] |
| Geschichte | |
| Entdeckung | Ormond Stone |
| Entdeckungsdatum | 1886 |
| Katalogbezeichnungen | |
| NGC 3776 • PGC 36048 • CGCG 012-045 • 2MASX J11381802-0321162 • | |
NGC 3776 ist eine Spiralgalaxie vom Hubble-Typ Sb[2] im Sternbild Jungfrau. Sie ist schätzungsweise 501 Millionen Lichtjahre von der Milchstraße entfernt.
Das Objekt wurde im Jahre 1886 von Ormond Stone entdeckt.[3]
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