Valley network
Valley networks are branching networks of valleys on Mars that superficially resemble terrestrial river drainage basins . [1] They are found mainly incised into the terrain of the martian southern highlands , and are typically - though not always - of Noachian age (approximately four billion years old). The individual valleys are typically less than 5 kilometers wide, though they may extend for up to hundreds or even thousands of kilometers across the martian surface.
Page Revisions
| Year | Metadata | Sections | Top Words | First Paragraph |
| 2018 |
124573 characters 10 sections 20 paragraphs 8 images 745 internal links 4 external links |
networks 0.414 valleys 0.260 valley 0.259 noachian 0.212 co2 0.149 greenhouse 0.127 recharge 0.110 hesperian 0.106 precipitation 0.105 aquifers 0.096 ramirez 0.094 groundwater 0.092 channel 0.090 formation 0.087 scales 0.087 |
Valley networks are branching networks of valleys on Mars that superficially resemble terrestrial river drainage basins . [1] They are found mainly incised into the terrain of the martian southern highlands , and are typically - though not always - of Noachian age (approximately four billion years old). The individual valleys are typically less than 5 kilometers wide, though they may extend for up to hundreds or even thousands of kilometers across the martian surface. |
|
| 2017 |
146975 characters 10 sections 20 paragraphs 11 images 846 internal links 4 external links |
networks 0.414 valleys 0.260 valley 0.259 noachian 0.212 co2 0.149 greenhouse 0.127 recharge 0.110 hesperian 0.106 precipitation 0.105 aquifers 0.096 ramirez 0.094 groundwater 0.092 channel 0.090 formation 0.087 scales 0.087 |
Valley networks are branching networks of valleys on Mars that superficially resemble terrestrial river drainage basins . [1] They are found mainly incised into the terrain of the martian southern highlands , and are typically - though not always - of Noachian age (approximately four billion years old). The individual valleys are typically less than 5 kilometers wide, though they may extend for up to hundreds or even thousands of kilometers across the martian surface. |
|
| 2016 |
83424 characters 10 sections 19 paragraphs 11 images 291 internal links 4 external links |
networks 0.428 valleys 0.269 valley 0.255 noachian 0.219 recharge 0.114 hesperian 0.110 precipitation 0.109 aquifers 0.100 groundwater 0.096 channel 0.093 scales 0.090 paleoclimate 0.088 highlands 0.087 mechanisms 0.084 typically 0.083 |
Valley networks are branching networks of valleys on Mars that superficially resemble terrestrial river drainage basins . [1] They are found mainly incised into the terrain of the martian southern highlands , and are typically - though not always - of Noachian age (approximately four billion years old). The individual valleys are typically less than 5 kilometers wide, though they may extend for up to hundreds or even thousands of kilometers across the martian surface. |
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| 2015 |
82946 characters 10 sections 19 paragraphs 11 images 291 internal links 4 external links |
networks 0.428 valleys 0.269 valley 0.255 noachian 0.219 recharge 0.114 hesperian 0.110 precipitation 0.109 aquifers 0.100 groundwater 0.096 channel 0.093 scales 0.090 paleoclimate 0.088 highlands 0.087 mechanisms 0.084 typically 0.083 |
Valley networks are branching networks of valleys on Mars that superficially resemble terrestrial river drainage basins . [1] They are found mainly incised into the terrain of the martian southern highlands , and are typically - though not always - of Noachian age (approximately four billion years old). The individual valleys are typically less than 5 kilometers wide, though they may extend for up to hundreds or even thousands of kilometers across the martian surface. |
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| 2014 |
59931 characters 10 sections 19 paragraphs 8 images 185 internal links 4 external links |
networks 0.428 valleys 0.269 valley 0.255 noachian 0.219 recharge 0.114 hesperian 0.110 precipitation 0.109 aquifers 0.100 groundwater 0.096 channel 0.093 scales 0.090 paleoclimate 0.088 highlands 0.087 mechanisms 0.084 typically 0.083 |
Valley networks are branching networks of valleys on Mars that superficially resemble terrestrial river drainage basins . [1] They are found mainly incised into the terrain of the martian southern highlands , and are typically - though not always - of Noachian age (approximately four billion years old). The individual valleys are typically less than 5 kilometers wide, though they may extend for up to hundreds or even thousands of kilometers across the martian surface. |
|
| 2013 |
59921 characters 10 sections 19 paragraphs 8 images 185 internal links 4 external links |
networks 0.428 valleys 0.269 valley 0.255 noachian 0.219 recharge 0.114 hesperian 0.110 precipitation 0.109 aquifers 0.100 groundwater 0.096 channel 0.093 scales 0.090 paleoclimate 0.088 highlands 0.087 mechanisms 0.084 typically 0.083 |
Valley networks are branching networks of valleys on Mars that superficially resemble terrestrial river drainage basins . [1] They are found mainly incised into the terrain of the martian southern highlands , and are typically - though not always - of Noachian age (approximately four billion years old). The individual valleys are typically less than 5 kilometers wide, though they may extend for up to hundreds or even thousands of kilometers across the martian surface. |
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| 2012 |
59859 characters 10 sections 19 paragraphs 8 images 184 internal links 4 external links |
networks 0.428 valleys 0.269 valley 0.255 noachian 0.219 recharge 0.114 hesperian 0.110 precipitation 0.109 aquifers 0.100 groundwater 0.096 channel 0.093 scales 0.090 paleoclimate 0.088 highlands 0.087 mechanisms 0.084 typically 0.083 |
Valley networks are branching networks of valleys on Mars that superficially resemble terrestrial river drainage basins . [1] They are found mainly incised into the terrain of the martian southern highlands , and are typically - though not always - of Noachian age (approximately four billion years old). The individual valleys are typically less than 5 kilometers wide, though they may extend for up to hundreds or even thousands of kilometers across the martian surface. |
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| 2011 |
57857 characters 9 sections 19 paragraphs 7 images 183 internal links 0 external links |
networks 0.428 valleys 0.269 valley 0.255 noachian 0.219 recharge 0.114 hesperian 0.110 precipitation 0.109 aquifers 0.100 groundwater 0.096 channel 0.093 scales 0.090 paleoclimate 0.088 highlands 0.087 mechanisms 0.084 typically 0.083 |
Valley networks are branching networks of valleys on Mars that superficially resemble terrestrial river drainage basins [1] . They are found mainly incised into the terrain of the martian southern highlands , and are typically - though not always - of Noachian age (approximately four billion years old). The individual valleys are typically less than 5 kilometers wide, though they may extend for up to hundreds or even thousands of kilometers across the martian surface. |