Марсіанські породи: відмінності між версіями

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Сучасні дані по М.п. свідчать про існування на Марсі хімічно диференційованої кори, аналогічної земній корі.
 
[[Шаруватість]] марсіанських порід описана в ряді джерел з геології планети Марс<ref>Grotzinger, J. and R. Milliken (eds.). 2012. Sedimentary Geology of Mars. SEPM.</ref>
 
<gallery widths="190px" heights="180px">
Image:Layers in a crater in Arabia.JPG|Layers in [[Tikonravev Crater]] in Arabia, as seen by [[Mars Global Surveyor]] (MGS). Layers may form from [[volcanoes]], the wind, or by deposition under water. The craters on the left are pedestal craters. Some researchers believe this crater once held a massive lake.
Image:Tikonravev Crater Floor.JPG|[[Tikonravev Crater]] floor, as seen by Mars Global Surveyor. Click on image to see dark slope streaks and layers.
Image:Tikhonravov Basin Streaks.JPG|Tikhonravov Basin streaks, as seen by HiRISE. Scale bar is {{convert|500|m|ft|abbr=on}} long
Image:Layers in Monument Valley.jpg|Layers in Monument Valley, Arizona. These are accepted as being formed, at least in part, by water deposition. Since Mars contains similar layers, water is considered a major cause of layering on Mars.
Image:Henry Crater Mound.JPG|[[Henry Crater]] mound, as seen by HiRISE. The scale bar is {{convert|500|m|ft|abbr=on}} long
Image:Cassini crater floor.JPG|Crater in the middle of [[Cassini (Martian crater)|Cassini]], as seen by HiRISE. Layers may have been deposited under water since it is believed that Cassini once held a giant lake.
<ref>http://www.uahirise.org/ESP_039997_2170</ref>
 
Image:ESP 025558buttes.jpg|Buttes, as seen by HiRISE under [[HiWish program]]. Buttes have layered rocks with a hard resistant cap rock on the top which protects the underlying rocks from erosion.
Image:25558dikes.jpg|Possible dikes and layered structures, as seen by HiRISE under HiWish program.
Image:25558fault.jpg|Possible fault along a butte, as seen by HiRISE under HiWish program.
</gallery>
 
== Дослідження ==