فائل:Titan multi spectral overlay.jpg

اس سے زیادہ ریزولیوشن دستیاب نہیں۔

Titan_multi_spectral_overlay.jpg ‏(576 × 576 پکسل، فائل کا حجم: 20 کلوبائٹ، MIME قسم: image/jpeg)

یہ فائل ویکی ذخائر کی ہے اور دیگر منصوبوں کے زیر استعمال ہوسکتی ہے۔ فائل کے صفحہ تعارف پر موجود تعارف ذیل میں موجود ہے۔

تفصیلTitan multi spectral overlay.jpg	English: Photograph of the Saturn moon Titan in False Color, taken by the Cassini space probe with ultraviolet and infrared camera on 26 Oct. 2004. Original caption released with the image: "This image shows Titan in ultraviolet and infrared wavelengths. It was taken by Cassini's imaging science subsystem on Oct. 26, 2004, and is constructed from four images acquired through different color filters. Red and green colors represent infrared wavelengths and show areas where atmospheric methane absorbs light. These colors reveal a brighter (redder) northern hemisphere. Blue represents ultraviolet wavelengths and shows the high atmosphere and detached hazes. Titan has a gigantic atmosphere, extending hundreds of kilometers above the surface. The sharp variations in brightness on Titan's surface (and clouds near the south pole) are apparent at infrared wavelengths. The image scale of this picture is 6.4 kilometers (4 miles) per pixel. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Cassini-Huygens mission for NASA's Office of Space Science, Washington, D.C. The Cassini orbiter and its two onboard cameras, were designed, developed and assembled at JPL. The imaging team is based at the Space Science Institute, Boulder, Colo." Deutsch: Saturnmond Titan; der Bereich der Infrarotstrahlung und der der Ultraviolettstrahlung sind durch unterschiedliche Farbfilter sichtbar gemacht. Rötliche und grünliche Farben repräsentieren den Infrarotbereich und indikieren Areale, in denen in der Atmosphäre enthaltenes Methan Licht absorbiert; bläuliche Farbe repräsentiert den Ultraviolettbereich und indikiert die obere Atmosphäre sowie die getrennten Schichten der Dunstschicht. Das Bild verwendet vier bei Cassinis Vorbeiflug am 26. Oktober 2004 durch unterschiedliche Farbfilter gemachte Aufnahmen. Norsk nynorsk: Bilete av Titan teken av Cassini-romsonden med ultrafiolett og infraraudt kamera den 26. oktober 2004.
تاریخ	26 اکتوبر 2004
ماخذ	NASA planetary photojournal, prepared by Alfred McEwen NASA planetary photojournal, PIA06139 http://photojournal.jpl.nasa.gov/jpeg/PIA06139.jpg
مصنف	NASA/JPL/Space Science Institute
اجازت (فائل کا دوبارہ استعمال)	Copyright information from http://www.jpl.nasa.gov/images/policy/index.cfm - Unless otherwise noted, images and video on JPL public web sites (public sites ending with a jpl.nasa.gov address) may be used for any purpose without prior permission [...]

	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."

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