NGC 2242
| Planetarischer Nebel NGC 2242 | |
|---|---|
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| AladinLite | |
| Sternbild | Fuhrmann |
| Position Äquinoktium: J2000.0 | |
| Rektaszension | 06h 34m 07,2s [1] |
| Deklination (Astronomie) | +44° 46′ 37″ [1] |
| Erscheinungsbild | |
| Scheinbare Helligkeit (visuell) | 15,0 mag [2] |
| Scheinbare Helligkeit (B-Band) | 15,1 mag [2] |
| Winkelausdehnung | 0,37′ × 0,37′ [2] |
| Zentralstern | |
| Bezeichnung | Gaia DR3 3336140414380977664 |
| Physikalische Daten | |
| Radialgeschwindigkeit | 38 km/s |
| Entfernung | 9.639 ± 1.900 Lj |
| Geschichte | |
| Entdeckung | Lewis A. Swift |
| Datum der Entdeckung | 24. November 1886 |
| Katalogbezeichnungen | |
| NGC 2242 • PK 170+15.1 • CGCG 204-5 | |
NGC 2242 bezeichnet einen planetarischen Nebel im Sternbild Fuhrmann.
Der Nebel wurde von dem Astronomen Lewis A. Swift am 24. November 1886 mithilfe eines 16-Zoll-Teleskops entdeckt und später von Johan Dreyer im New General Catalogue verzeichnet.[3]
Weblinks
Commons: NGC 2242 – Sammlung von Bildern, Videos und Audiodateien
Einzelnachweise
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