NGC 3777
| Galaxie NGC 3777 | |
|---|---|
| |
| AladinLite | |
| Sternbild | Becher |
| Position Äquinoktium: J2000.0, Epoche: J2000.0 | |
| Rektaszension | 11h 36m 06,8s [1] |
| Deklination | −12° 34′ 09″ [1] |
| Erscheinungsbild | |
| Morphologischer Typ | SAB(s)ab[1] |
| Helligkeit (visuell) | 13,5 mag[2] |
| Helligkeit (B-Band) | 14,3 mag[2] |
| Winkelausdehnung | 1,1' × 0,7'[2] |
| Positionswinkel | 35°[2] |
| Flächenhelligkeit | 13,1 mag/arcmin²[2] |
| Physikalische Daten | |
| Zugehörigkeit | LDCE 824[1] |
| Rotverschiebung | 0.014103 ± 0.000110[1] |
| Radialgeschwindigkeit | (4228 ± 33) km/s[1] |
| Hubbledistanz H0 = 73 km/(s • Mpc) |
(182 ± 13)e6 Lj (55,8 ± 3,9) Mpc [1] |
| Geschichte | |
| Entdeckung | Francis P. Leavenworth |
| Entdeckungsdatum | 26. Februar 1886 |
| Katalogbezeichnungen | |
| NGC 3777 • PGC 35879 • MCG -02-30-008 • 2MASX J11360684-1234087 • | |
NGC 3777 ist eine Balken-Spiralgalaxie vom Hubble-Typ Sab im Sternbild Becher am Südsternhimmel. Sie ist schätzungsweise 182 Millionen Lichtjahre von der Milchstraße entfernt.
Das Objekt wurde am 26. Februar 1886 von Francis Preserved Leavenworth entdeckt.[3]
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