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21 Aug, 2019
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File:WASP-12b.jpg

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	Date/Time	Thumbnail	Dimensions	User	Comment
current	09:32, 27 January 2013		3,300 × 2,550 (856 KB)	Stas1995	size
	20:28, 5 September 2012		3,300 × 2,475 (426 KB)	Stas1995	User created page with UploadWizard

File usage

The following pages on the English Wikipedia use this file (pages on other projects are not listed):

Global file usage

The following other wikis use this file:

Usage on af.wikipedia.org
- WASP-12
Usage on ar.wikipedia.org
- واسب-12b
- واسب-12
Usage on ca.wikipedia.org
- WASP-12b
Usage on de.wikipedia.org
- WASP-12b
Usage on es.wikipedia.org
- Auriga (constelación)
Usage on id.wikipedia.org
- WASP-12b
Usage on ja.wikipedia.org
- WASP-12b
Usage on ko.wikipedia.org
- WASP-12
Usage on pt.wikipedia.org
- WASP-12b
Usage on ro.wikipedia.org
- WASP-12b
- WASP-12
Usage on sk.wikipedia.org
- WASP-12
Usage on uz.wikipedia.org
- WASP-12b (ekzosayyora)
Usage on vi.wikipedia.org
- WASP-12b
Usage on zh.wikipedia.org
- WASP-12b

Metadata

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Image title	This plot of data from NASA's Spitzer Space Telescope indicates the presence of molecules in the planet WASP-12b -- a super-hot gas giant that orbits tightly around its star. Spitzer measurements suggest this planet's atmosphere has carbon monoxide, excess methane, and not much water vapor. The results demonstrate that WASP-12b is the first known carbon-rich planet. Spitzer made these measurements as the planet circled behind the star, in an event called the secondary eclipse. The telescope collected the infrared light from the star and the planet, then just the star as the planet disappeared behind the star. This allowed astronomers to calculate the amount of infrared light coming solely from the planet. The observations were performed at four different wavelengths of infrared light. These data were then combined with previously reported measurements taken by the Canada-France-Hawaii Telescope atop Mauna Kea, Hawaii, at shorter infrared wavelengths to create this plot. The yellow dots show the data, along with the observational uncertainties. The blue curve is a model of the planet's light, or spectrum, showing the fingerprints of chemicals in the atmosphere. The blue dots represent the blue model curve averaged to cover the same wavelengths as the data, as shown by the gray lines at the bottom of the plot.
Author	NASA/JPL-Caltech/N. Madhusudhan (Princeton University)
Copyright holder	http://www.spitzer.caltech.edu/Media/mediaimages/copyright.shtml
Short title	Signature of a Carbon-Rich Planet
Credit/Provider	NASA/JPL-Caltech/N. Madhusudhan (Princeton University)
Headline	This plot of data from NASA's Spitzer Space Telescope indicates the presence of molecules in the planet WASP-12b -- a super-hot gas giant that orbits tightly around its star.
Source	Spitzer Space Telescope
Date and time of data generation	8 December 2010
Width	3,300 px
Height	2,550 px
Bits per component	8 8 8
Compression scheme	LZW
Pixel composition	RGB
Orientation	Normal
Number of components	3
Horizontal resolution	300 dpi
Vertical resolution	300 dpi
Data arrangement	chunky format
Software used	Adobe Photoshop CS3 Macintosh
File change date and time	09:37, 8 December 2010
Color space	sRGB
Contact information	http://www.spitzer.caltech.edu 1200 E. California Blvd. Pasadena, CA, 91125 USA
Keywords	WASP-12b
IIM version	2

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