![File:A deep infrared view of the: Orion Nebula from HAWK-I - Eso1625a.jpg](https://upload.wikimedia.org/wikipedia/commons/thumb/d/d2/A_deep_infrared_view_of_the_Orion_Nebula_from_HAWK-I_-_Eso1625a.jpg/791px-A_deep_infrared_view_of_the_Orion_Nebula_from_HAWK-I_-_Eso1625a.jpg)
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DescriptionA deep infrared view of the Orion Nebula from HAWK-I - Eso1625a.jpg |
English: This spectacular image of the Orion Nebula star-formation region was obtained from multiple exposures using the HAWK-I infrared camera on ESO’s Very Large Telescope in Chile. This is the deepest view ever of this region. And reveals more very faint planetary-mass objects than expected.
Coordinates Position (RA): 5 35 16.58 Position (Dec): -5° 20' 19.53" Field of view: 29.11 x 22.07 arcminutes Orientation: North is 90.1° left of vertical Band Wavelength Telescope Infrared J 1.258 μm Very Large Telescope HAWK-I Infrared H 1.62 μm Very Large Telescope HAWK-IInfrared Ks 2.146 μm Very Large Telescope HAWK-I |
Date | (released) |
Source | http://www.eso.org/public/images/eso1625a/ (image link) |
Author | ESO/H. Drass et al. |
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Date/Time | Thumbnail | Dimensions | User | Comment | |
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current | 09:44, 13 July 2016 | ![]() | 16,373 × 12,412 (56.95 MB) | Fabian RRRR | =={{int:filedesc}}== {{Information |description={{en|1=This spectacular image of the Orion Nebula star-formation region was obtained from multiple exposures using the HAWK-I infrared camera on ESO’s Very Large Telescope in Chile. This is the deepest... |
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Credit/Provider | ESO/H. Drass et al. |
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Source | European Southern Observatory |
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Usage terms |
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Date and time of data generation | 12:00, 12 July 2016 |
Software used | Adobe Photoshop CC 2015 (Windows) |
File change date and time | 16:42, 6 July 2016 |
Date and time of digitizing | 23:22, 4 May 2016 |
Date metadata was last modified | 18:42, 6 July 2016 |
Unique ID of original document | xmp.did:1201a660-1724-cc4b-95dd-2a525607322c |
Keywords |
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Contact information |
Karl-Schwarzschild-Strasse 2 Garching bei München, , D-85748 Germany |
IIM version | 4 |