Lêer:WASP-12b.jpg

Oorspronklike lêer ‎(3 300 × 2 550 piksels, lêergrootte: 856 KG, MIME-tipe: image/jpeg)

Hierdie lêer kom vanaf Wikimedia Commons en kan ook in ander projekte gebruik word. Die beskrywing op die lêer se inligtingsblad word hieronder weergegee.

Opsomming

BeskrywingWASP-12b.jpg	English: 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
Datum	6 September 2012, 00:25:57
Bron	http://www.nasa.gov/mission_pages/spitzer/multimedia/pia13690.html
Outeur	NASA/JPL-Caltech/CFHT/MIT/Princeton/UCF
Ander weergawes

Lisensiëring

	This file is in the public domain in the United States because it was solely created by NASA. NASA copyright policy states that "NASA material is not protected by copyright unless noted". (See Template:PD-USGov, NASA copyright policy page or JPL Image Use Policy.)
	Warnings: Use of NASA logos, insignia and emblems is restricted per U.S. law 14 CFR 1221. The NASA website hosts a large number of images from the Soviet/Russian space agency, and other non-American space agencies. These are not necessarily in the public domain. Materials based on Hubble Space Telescope data may be copyrighted if they are not explicitly produced by the STScI.[1] See also {{PD-Hubble}} and {{Cc-Hubble}}. The SOHO (ESA & NASA) joint project implies that all materials created by its probe are copyrighted and require permission for commercial non-educational use. [2] Images featured on the Astronomy Picture of the Day (APOD) web site may be copyrighted. [3] The National Space Science Data Center (NSSDC) site has been known to host copyrighted content. Its photo gallery FAQ states that all of the images in the photo gallery are in the public domain "Unless otherwise noted."

Lêergeskiedenis

Klik op die datum/tyd om te sien hoe die lêer destyds gelyk het.

	Datum/Tyd	Duimnael	Dimensies	Gebruiker	Opmerking
huidig	09:32, 27 Januarie 2013		3 300 × 2 550 (856 KG)	Stas1995	size
	20:28, 5 September 2012		3 300 × 2 475 (426 KG)	Stas1995	User created page with UploadWizard

Lêergebruik

Die volgende bladsy gebruik dié lêer:

WASP-12

Globale lêergebruik

Die volgende ander wiki's gebruik hierdie lêer:

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

Metadata

Die lêer bevat aanvullende inligting wat moontlik deur 'n digitale kamera of skandeerder bygevoeg is.

As die lêer verander is, sal sekere inligting dalk nie meer ooreenkom met dié van die gewysigde lêer nie.

Beeldtitel	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.
Outeur	NASA/JPL-Caltech/N. Madhusudhan (Princeton University)
Kopiereghouer	http://www.spitzer.caltech.edu/Media/mediaimages/copyright.shtml
Kort titel	Signature of a Carbon-Rich Planet
Krediet/Verskaffer	NASA/JPL-Caltech/N. Madhusudhan (Princeton University)
Opskrif	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.
Bron	Spitzer Space Telescope
Gegewens opgestel op	8 Desember 2010
Breedte	3 300 px
Hoogte	2 550 px
Grepe per komponent	8 8 8
Kompressiemetode	LZW
Piksel-komposisie	RGB
Oriëntasie	Normaal
Aantal komponente	3
Horisontale resolusie	300 dpi
Vertikale resolusie	300 dpi
Datastruktuur	chunky dataformaat
Sagteware gebruik	Adobe Photoshop CS3 Macintosh
Tydstip laaste lêerwysiging	09:37, 8 Desember 2010
Kleurruimte	sRGB
Kontak inligting	http://www.spitzer.caltech.edu 1200 E. California Blvd. Pasadena, CA, 91125 USA
Sleutelwoorde	WASP-12b
IIM-weergawe	2

Lêer:WASP-12b.jpg

Opsomming

Lisensiëring

Captions

Items portrayed in this file

uitbeelding

datum van stigting of ontstaan

6 September 2012

Lêergeskiedenis

Lêergebruik

Globale lêergebruik

Metadata