Virsioni a àuta risuluzzioni(3 374 × 3 300 pixel, grannizza dû file: 15,26 MB, tipu MIME: image/png)

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Discrizzioni

Discrizzioni
English: Colour image of Phobos, imaged by the Mars Reconnaisance Orbiter in 2008.
Türkmençe: Phobos, Mars-yň iki hemrasyndan biri. Güneş Sistemasy-ndaky beýleki hemralara garanyňda planetasyna iň ýakyn ýerleşýän hemradyr. Mars ýüzündäki biri üçin günde iki gezek dogup batýar.
Luogo
InfoField
http://www.nasa.gov/mission_pages/MRO/multimedia/pia10368.html
Data
Fonti NASA
Auturi NASA/JPL-Caltech/University of Arizona
Pirmissu
(Riutilizzari stu file)
Public domain
Àutri virsioni
Sta mmàggini o filmatu fu catalugatu dô
Jet Propulsion Lab
National Aeronautics and Space Administration
(NASA) dê Stati Uniti dâ Mèricacô Photo ID: PIA10368.

This tag does not indicate the copyright status of the attached work. A normal copyright tag is still required. See Commons:Licensing.
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Downloaded from the NASA .tif source and converted to png with convert(1)

Original caption

The High Resolution Imaging Science Experiment (HiRISE) camera on NASA's Mars Reconnaissance Orbiter took two images of the larger of Mars' two moons, Phobos, within 10 minutes of each other on March 23, 2008. This is the first, taken from a distance of about 6,800 kilometers (about 4,200 miles). It is presented in color by combining data from the camera's blue-green, red, and near-infrared channels.

The illuminated part of Phobos seen in the images is about 21 kilometers (13 miles) across. The most prominent feature in the images is the large crater Stickney in the lower right. With a diameter of 9 kilometers (5.6 miles), it is the largest feature on Phobos.

The color data accentuate details not apparent in black-and-white images. For example, materials near the rim of Stickney appear bluer than the rest of Phobos. Based on analogy with materials on our own moon, this could mean this surface is fresher, and therefore younger, than other parts of Phobos.

A series of troughs and crater chains is obvious on other parts of the moon. Although many appear radial to Stickney in this image, recent studies from the European Space Agency's Mars Express orbiter indicate that they are not related to Stickney. Instead, they may have formed when material ejected from impacts on Mars later collided with Phobos. The lineated textures on the walls of Stickney and other large craters are landslides formed from materials falling into the crater interiors in the weak Phobos gravity (less than one one-thousandth of the gravity on Earth).

In the full-resolution version of this image, a pixel encompasses 6.8 meters (22 feet), providing a resolution (smallest visible feature) of about 20 meters (about 65 feet). The image is in the HiRISE catalog as PSP_007769_9010.

NASA's Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Mars Reconnaissance Orbiter for NASA's Science Mission Directorate, Washington. Lockheed Martin Space Systems, Denver, is the prime contractor for the project and built the spacecraft. The High Resolution Imaging Science Experiment is operated by the University of Arizona, Tucson, and the instrument was built by Ball Aerospace & Technologies Corp., Boulder, Colo.

Licenza

Public domain Stu file è ntô duminiu pùbblicu pirchì criatu dâ NASA. La pulìtica supra lu copyright dâ NASA afferma ca «lu matiriali dâ NASA nun è prutiggiutu di copyright a menu ca nun sia spicificatu autrimenti». (NASA copyright policy e JPL Image Use Policy).
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Immagine colorata di fobos, immagine scattata nel 2008

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16 005 884 byte

3 300 pixel

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3 374 pixel

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Data/UraMiniaturaDiminsioniUtentiOggettu
currenti13:33, 10 apr 2008Miniatura di la virsioni dû 13:33, 10 apr 20083 374 × 3 300 (15,26 MB)Ævar Arnfjörð Bjarmason{{Information |Description= Phobos from 6,800 Kilometers (Color) |Source= http://www.nasa.gov/mission_pages/MRO/multimedia/pia10368.html |Date= |Author= |Permission= |other_versions= http://www.nasa.gov/images/content/221831main_PIA10368.tif }} Downloade

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