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Summary Of: Regolith

the regolith is composed of the following subdivisions... People also call various types of earthly regolith by such names as... the presence of regolith is one of the important factors for most... This regolith has been formed over the last 4... The regolith is generally about 4... Below this true regolith is a region of blocky and fractured bedrock created by larger impacts which is often... The physical and optical properties of lunar regolith are altered through a process known as... thick dust layer at the top of the regolith would not support the weight of the... the regolith was found to be quite firm by the robotic... is shaping the martian regolith in the present epoch... and carbon dioxide ices remain frozen within the regolith in the equatorial parts of Mars and on its surface at higher latitudes... returned spectacular and surprising images of an asteroidal regolith on an asteroid so small it was thought that gravity was too low to develop... similarity with regolith on other bodies... of ice grains were not considered to be regolith because when they appear on Earth in the form of... Lunar Regolith and Fragmental Breccias...

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Greek | heterogeneous | rock | dust | soil | rock | Earth | Moon | asteroids | planets | Soil | Alluvium | saprolite | cratons | colluvium | Earth | weathering | biological processes | dirt | dust | gravel | sand | mud | life | plants | animals | This famous image taken during Apollo 11 shows the fine and powdery texture of lunar soil. | | Apollo 11 | lunar | bedrock | meteoroids | micrometeoroids | mare | highland | lunar soil | soil | organic | space weathering | crater rays | Apollo | Thomas Gold | Cornell University | President's Science Advisory Committee | lunar module | Surveyor | hammer | core sampling | Martian sand and boulders photographed by NASA's Mars Exploration Rover Spirit. | | Mars Exploration Rover | Mars | dust storms | groundwater sapping | carbon dioxide hydrates | Regolith beneath NASA's Phoenix Mars Lander, where the descent thrusters have apparently cleared away several patches of soil to expose the underlying ice. | | Phoenix | Taken from just 250 m above the surface of Eros as the NEAR Shoemaker spacecraft was landing, this image shows an area that is only 12 m across. | | NEAR Shoemaker | NEAR Shoemaker | Eros | Hayabusa | Dunes on Titan's surface in a radar image taken by the Cassini spacecraft of a region approximately 160 by 325 kilometers (99 by 202 miles). | | Cassini | Pebbles on Titan's surface, imaged from a height of about 85 cm by the Huygens spacecraft. | | Titan | mechanical | etymologically | mineral | quartz | plagioclase | snow | erosion | aeolian | sedimentary | Huygens probe | clay | In-situ resource utilization | Helium-3 | Soil | Sand | 2007 | 02-15 | 2007 | 02-16 | ISBN 0521334446 | 10 April | 2005 | 2005 | 01-15 | 2005 | 03-28 | Categories | Sedimentology | Geomorphology |
This article is licensed under the GNU Free Documentation License. It uses material from the Wikipedia article "Regolith".