NGC 2014
 (c) ESA/Hubble, CC BY 4.0 | |
| Der Sternhaufen NGC 2014 (rechts) begleitet von einem rötlichen Nebel und NGC 2020 (bläulich, links) in einer Aufnahme des Hubble-Weltraumteleskops. | |
| AladinLite | |
| Sternbild | Schwertfisch |
| Position Äquinoktium: J2000.0 | |
|---|---|
| Rektaszension | 05h 32m 19,9s [1] |
| Deklination | -67° 41′ 23″ [1] |
| Erscheinungsbild | |
| Helligkeit (visuell) | 9,0 mag [2] |
| Helligkeit (B-Band) | 9,2 mag [2] |
| Winkelausdehnung | 1,8' [2] |
| Physikalische Daten | |
| Zugehörigkeit | Große Magellansche Wolke |
| Geschichte | |
| Entdeckt von | James Dunlop |
| Entdeckungszeit | 3. August 1826 |
| Katalogbezeichnungen | |
| NGC 2014 • ESO 56-SC146 • GC 1217 • h 2900 • | |
NGC 2014 ist ein Emissionsnebel in der Großen Magellanschen Wolke mit einem eingebetteten offenen Sternhaufen. Er liegt im Sternbild Schwertfisch. Das Objekt wurde am 3. August 1826 von James Dunlop mit einem 23-cm-Teleskop entdeckt.[3]
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NGC 2014, NGC 2020 - HST - Heic2007a.jpg
(c) ESA/Hubble, CC BY 4.0
This image is one of the most photogenic examples of the many turbulent stellar nurseries the NASA/ESA Hubble Space Telescope has observed during its 30-year lifetime. The portrait features the giant nebula NGC 2014 and its neighbour NGC 2020 which together form part of a vast star-forming region in the Large Magellanic Cloud, a satellite galaxy of the Milky Way, approximately 163 000 light-years away. The image is nicknamed the “Cosmic Reef” because it resembles an undersea world.
(c) ESA/Hubble, CC BY 4.0
This image is one of the most photogenic examples of the many turbulent stellar nurseries the NASA/ESA Hubble Space Telescope has observed during its 30-year lifetime. The portrait features the giant nebula NGC 2014 and its neighbour NGC 2020 which together form part of a vast star-forming region in the Large Magellanic Cloud, a satellite galaxy of the Milky Way, approximately 163 000 light-years away. The image is nicknamed the “Cosmic Reef” because it resembles an undersea world.