IC 5095
| Galaxie IC 5095 | |
|---|---|
| |
| Legacy Surveys DR11 | |
| AladinLite | |
| Sternbild | Pfau |
| Position Äquinoktium: J2000.0, Epoche: J2000.0 | |
| Rektaszension | 21h 17m 22,2s [1] |
| Deklination | −59° 56′ 51″ [1] |
| Erscheinungsbild | |
| Morphologischer Typ | (R)Sbc[1] |
| Helligkeit (visuell) | 14,7 mag[2] |
| Helligkeit (B-Band) | 15,4 mag[2] |
| Winkelausdehnung | 0,90' × 0,4'[2] |
| Positionswinkel | 70°[2] |
| Flächenhelligkeit | 13,4 mag/arcmin²[2] |
| Physikalische Daten | |
| Rotverschiebung | 0.041372 ± 0.000150[1] |
| Radialgeschwindigkeit | 12.403 ± 45 km/s[1] |
| Hubbledistanz H0 = 73 km/(s • Mpc) |
(551 ± 38)e6 Lj (168,9 ± 11,8) Mpc [1] |
| Geschichte | |
| Entdeckung | Royal H. Frost |
| Entdeckungsdatum | 19. September 1903 |
| Katalogbezeichnungen | |
| IC 5095 • PGC 66498 • ESO 145-002 • 2MASX J21172225-5956511 • GALEXASC J211722.09-595649.7 | |
IC 5095 ist eine Spiralgalaxie vom Hubble-Typ Sc[2] im Sternbild Pfau am Südsternhimmel. Sie ist schätzungsweise 551 Millionen Lichtjahre von der Milchstraße entfernt und hat einen Durchmesser von etwa 150.000 Lichtjahren.
Das Objekt wurde am 19. September 1903 von Royal Harwood Frost entdeckt.[3]
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