File:Changes in tilt of Mars's axis PIA15095.jpg

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Description
English: Changes in Mars's axial tilt affecting its climate and ice cover. Present-day Mars seen top left.
Ελληνικά: Οι αλλαγές στην κλίση του άξονα περιστροφής του Άρη (Mετάπτωση των ισημεριών) επηρεάζουν ανάλογα και το κλίμα του, καθώς και το ποσοστό της επιφάνειάς του που καλύπτεται από πάγο. Ο Άρης όπως είναι σήμερα φαίνεται πάνω αριστερά.

Original caption

Modern-day Mars experiences cyclical changes in climate and, consequently, ice distribution. Unlike Earth, the obliquity (or tilt) of Mars changes substantially on timescales of hundreds of thousands to millions of years. At present day obliquity of about 25-degree tilt on Mars' rotational axis, ice is present in relatively modest quantities at the north and south poles (top left). This schematic shows that ice builds up near the equator at high obliquities (top right) and the poles grow larger at very low obliquities (bottom) (References: Laskar et al., 2002; Head <="" i="">., 2003).
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Source http://photojournal.jpl.nasa.gov/catalog/PIA15095 file
Author NASA/JPL-Caltech
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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.)
Warnings:
This image or video was catalogued by Jet Propulsion Laboratory of the United States National Aeronautics and Space Administration (NASA) under Photo ID: PIA15095.

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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21 November 2011

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current02:30, 14 April 2012Thumbnail for version as of 02:30, 14 April 20121,048 × 684 (27 KB)wikimediacommons>Badseed{{Information |Description={{en|Changes in Mars's axial tilt affecting its climate and ice cover. Present-day Mars seen top left.}} {{el|Οι αλλαγές στην κλίση του άξονα περιστροφής του Άρη ([[w:el:μετάπτ...

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