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- Q5611030 subject Q5933994.
- Q5611030 subject Q8909585.
- Q5611030 abstract "During past ages, there was rain and/or snow on Mars; especially in the Noachian and early Hesperian epochs. Some moisture entered the ground and formed aquifers. That is, the water went into the ground, seeped down until it reached a layer that would not allow it to penetrate (such a layer is called impermeable), and then water piled up forming a layer that was saturated with water. In an aquifer water occupies open space (pore space) that lies between rock particles. This layer would spread out, eventually coming to be under most of the Martian surface. The top of this layer is called the water table. Calculations show that the water table on Mars was for a time 600 meters below the surface. Several prominent features on the planet have been produced by the action of groundwater.When water rose to the surface or near surface, various minerals were deposited and sediments became cemented together. Some of the minerals were sulfates that were probably produced when water dissolved sulfur from underground rocks, and then became oxidized when it came into contact with the air.While traveling through the aquifer, the water passed through the igneous rock basalt that contains sulfur.".
- Q5611030 thumbnail Burns_cliff.jpg?width=300.
- Q5611030 wikiPageWikiLink Q103223.
- Q5611030 wikiPageWikiLink Q1036092.
- Q5611030 wikiPageWikiLink Q1093379.
- Q5611030 wikiPageWikiLink Q12370.
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- Q5611030 wikiPageWikiLink Q13085.
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- Q5611030 wikiPageWikiLink Q21027955.
- Q5611030 wikiPageWikiLink Q2466.
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- Q5611030 wikiPageWikiLink Q2619965.
- Q5611030 wikiPageWikiLink Q3038730.
- Q5611030 wikiPageWikiLink Q3054209.
- Q5611030 wikiPageWikiLink Q3054518.
- Q5611030 wikiPageWikiLink Q3299463.
- Q5611030 wikiPageWikiLink Q3461535.
- Q5611030 wikiPageWikiLink Q3501670.
- Q5611030 wikiPageWikiLink Q391388.
- Q5611030 wikiPageWikiLink Q391398.
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- Q5611030 wikiPageWikiLink Q408.
- Q5611030 wikiPageWikiLink Q46.
- Q5611030 wikiPageWikiLink Q47521.
- Q5611030 wikiPageWikiLink Q55818.
- Q5611030 wikiPageWikiLink Q5750336.
- Q5611030 wikiPageWikiLink Q583075.
- Q5611030 wikiPageWikiLink Q5933994.
- Q5611030 wikiPageWikiLink Q621110.
- Q5611030 wikiPageWikiLink Q622221.
- Q5611030 wikiPageWikiLink Q656985.
- Q5611030 wikiPageWikiLink Q7135428.
- Q5611030 wikiPageWikiLink Q7946.
- Q5611030 wikiPageWikiLink Q82480.
- Q5611030 wikiPageWikiLink Q8909585.
- Q5611030 wikiPageWikiLink Q912034.
- Q5611030 comment "During past ages, there was rain and/or snow on Mars; especially in the Noachian and early Hesperian epochs. Some moisture entered the ground and formed aquifers. That is, the water went into the ground, seeped down until it reached a layer that would not allow it to penetrate (such a layer is called impermeable), and then water piled up forming a layer that was saturated with water. In an aquifer water occupies open space (pore space) that lies between rock particles.".
- Q5611030 label "Groundwater on Mars".
- Q5611030 depiction Burns_cliff.jpg.