File:Sedswithholes.jpg
Sedswithholes.jpg (589 × 589 pixels, file size: 62 KB, MIME type: image/jpeg)
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current | 21:38, 12 March 2012 | 589 × 589 (62 KB) | Rebull (talk | contribs) |
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Image title |
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Author | Spitzer Space Telescope |
Copyright holder | http://www.spitzer.caltech.edu/Media/mediaimages/copyright.shtml |
Date and time of data generation | 27 May 2004 |
Width | 1,200 px |
Height | 1,200 px |
Bits per component |
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Compression scheme | LZW |
Pixel composition | RGB |
Orientation | Normal |
Number of components | 3 |
Horizontal resolution | 72 dpi |
Vertical resolution | 72 dpi |
Data arrangement | chunky format |
Software used | Adobe Photoshop CS3 Macintosh |
File change date and time | 14:40, 5 June 2009 |
Color space | Uncalibrated |
Contact information |
http://www.spitzer.caltech.edu 1200 E. California Blvd. Pasadena, CA, 91125 USA |
Short title |
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Credit/Provider | NASA/JPL-Caltech/D. Watson (University of Rochester) |
Headline | How can you tell if a star has a protoplanetary disc around it, when the disc is too small to image directly? Using the technique of spectroscopy, scientists can deduce the temperature and chemical composition of material around a star, even if they cannot see the disc itself. |
Source | Spitzer Space Telescope |
Usage terms |
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IIM version | 2 |