File:Eta Carinae Homunculus Nebula (gemini1001a).jpg
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[edit]DescriptionEta Carinae Homunculus Nebula (gemini1001a).jpg |
English: Eta Carinae as imaged by the Gemini South telescope in Chile with the Near Infrared Coronagraphic Imager (NICI) using adaptive optics to reduce blurring by turbulence in the Earth’s atmosphere. In this image the bipolar lobes of the Homunculus Nebula are visible with the never-before imaged “Little Homunculus Nebula” visible as a faint blue glow, mostly in the lower lobe. The Butterfly Nebula is visible (region circled) as the yellowish glow with dark filamentary structure close to, and mostly below/left, of the central star system (the central star system appears as a dark spot due to the coronagraphic blocking (occulting) disk used to eliminate the star’s bright glare). See Image Release for details Technical Details: This image is a color composite using three infrared filters: [Fe II] (1.644 micron) – blue layer; H2 2-1 S(1) (2.2465 micron) – green layer; Br(gamma) (2.1686 micron) – red layer. The field of view for the image is 16.0 x 15.4 arcseconds and is oriented with north up and east to the left. |
Date | 4 January 2010 (upload date) |
Source | Eta Carinae Homunculus Nebula |
Author | International Gemini Observatory |
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Author | Peter Michaud |
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Label | In Web Gallery |
Credit/Provider | International Gemini Observatory |
Source | NSF's NOIRLab |
Online copyright statement | http://www.gemini.edu/index.php?q=node/14 |
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Copyright holder |
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City shown | La Serena |
Date and time of data generation | 20:00, 4 January 2010 |
JPEG file comment | Image Credit:J.C. Martin et. al., Gemini Observatory/AURA
Eta Carinae as imaged by the Gemini South telescope in Chile with the Near Infrared Coronagraphic Imager (NICI) using adaptive optics to reduce blurring by turbulence in the Earth’s atmosphere. In this image the bipolar lobes of the Homunculus Nebula are visible with the never-before imaged “Little Homunculus Nebula” visible as a faint blue glow, mostly in the lower lobe. The Butterfly Nebula is visible (region circled) as the yellowish glow with dark filamentary structure close to, and mostly below/left, of the central star system (the central star system appears as a dark spot due to the coronagraphic blocking (occulting) disk used to eliminate the star’s bright glare). This image is a color composite using three infrared filters: [Fe II] (1.644 micron) – blue layer; H2 2-1 S(1) (2.2465 micron) – green layer; Br(gamma) (2.1686 micron) – red layer. The field of view for the image is 16.0 x 15.4 arcseconds and is oriented with north up and east to the left. |
Software used | Adobe Photoshop CS3 Macintosh |
File change date and time | 22:32, 14 April 2020 |
Date and time of digitizing | 23:39, 16 July 2009 |
Date metadata was last modified | 00:32, 15 April 2020 |
Unique ID of original document | uuid:2B8C4C254674DE11A53BBB7B782F44CF |
Type of item | Science & Technology |
Copyright status | Copyright status not set |
Keywords | Eta Carinae |
Contact information | @ gemini.edu pmichaud @ gemini.edu
950 North Cherry Ave. Tucson, AZ, 85719 USA |
Country shown | Chile |
Province or state shown | Region 4 |
Sublocation of city shown | Cerro Pachón |
Code for country shown | CL |
IIM version | 4 |