NGC 7291
| Galaxie NGC 7291 | |
|---|---|
| SDSS-Aufnahme | |
| AladinLite | |
| Sternbild | Pegasus |
| Position Äquinoktium: J2000.0, Epoche: J2000.0 | |
| Rektaszension | 22h 28m 26,4s [1] |
| Deklination | +16° 46′ 59″ [1] |
| Erscheinungsbild | |
| Morphologischer Typ | S0[1] |
| Helligkeit (visuell) | 13,5 mag[2] |
| Helligkeit (B-Band) | 14,5 mag[2] |
| Winkelausdehnung | 1,8′ × 1,7′[2] |
| Positionswinkel | 54°[2] |
| Flächenhelligkeit | 14,6 mag/arcmin²[2] |
| Physikalische Daten | |
| Rotverschiebung | 0,034377 ± 0,000097[1] |
| Radialgeschwindigkeit | (10306 ± 29) km/s[1] |
| Hubbledistanz H0 = 73 km/(s • Mpc) |
(469 ± 33)e6 Lj (143,7 ± 10,1) Mpc [1] |
| Geschichte | |
| Entdeckung | Truman Safford |
| Entdeckungsdatum | 1. Oktober 1866 |
| Katalogbezeichnungen | |
| NGC 7291 • UGC 12047 • PGC 68944 • CGCG 452-015 • MCG +03-57-008 • 2MASX J22282953+1646598 • | |
NGC 7291 ist eine linsenförmige Galaxie vom Hubble-Typ S0 im Sternbild Pegasus am Nordsternhimmel. Sie ist schätzungsweise 469 Millionen Lichtjahre von der Milchstraße entfernt.
Das Objekt wurde am 1. Oktober 1866 von dem Astronomen Truman Henry Safford entdeckt und später von Johan Dreyer in seinen New General Catalogue aufgenommen.[3]
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