File:Santa Fe ray system (THEMIS thermal inertia map).png

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Українська: Карта теплової інерції (чим вища, тим світліше) околиць марсіанського кратера Санта-Фе. Сам кратер (розташований у центрі зображення) має діаметр 20,3 км. Навколо нього видно численні темні та світлі промені, які (на відміну від звичайних променів кратерів) могли бути створені надзвуковими струменями пари (Schultz, Quintana, 2017).
English: Map of thermal inertia (the more inertia, the brighter image) of the neighbourhood of Martian crater Santa Fe. The crater (in the centre) is 20.3 km in diameter. It is surrounded by a system of dark and bright rays, which (unlike usual crater rays) could be created by supersonic jets of vapour (Schultz, Quintana, 2017).
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Source THEMIS Thermal Inertia 100m Global Mosaic
Author NASA (infrared images of THEMIS camera onboard 2001 Mars Odyssey)

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Public domain 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.)
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current23:39, 16 January 2018Thumbnail for version as of 23:39, 16 January 20181,420 × 1,420 (1.43 MB)Sneeuwschaap (talk | contribs)User created page with UploadWizard

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