Iani Chaos
Iani Chaos is a region of chaos terrain at the south end of the outflow channel Ares Vallis , of the Margaritifer Sinus quadrangle (MC-19) region of the planet Mars , centered at approximately ~342°E, 2°S. This is the source region of Ares Vallis. The chaotic terrain is widely believed to have formed via the removal of subsurface water or ice , resulting in flooding at the surface, and the formation of Ares Vallis. Within Iani Chaos, deposited stratigraphically above the chaotic terrain, are smooth, low-slope, intermediate-to-light-toned deposits that are rich in a hydrated mineral that is most likely gypsum as well as hematite . [1]
Page Revisions
| Year | Metadata | Sections | Top Words | First Paragraph |
| 2017 |
37202 characters 4 sections 7 paragraphs 10 images 161 internal links 2 external links |
iani 0.621 chaos 0.565 ares 0.145 margaritifer 0.140 gypsum 0.123 sites 0.104 hematite 0.102 stratigraphically 0.101 chaotic 0.097 examine 0.096 vallis 0.093 sinus 0.088 terrain 0.086 arsinoes 0.084 aureum 0.082 |
Iani Chaos is a region of chaos terrain at the south end of the outflow channel Ares Vallis , of the Margaritifer Sinus quadrangle (MC-19) region of the planet Mars , centered at approximately ~342°E, 2°S. This is the source region of Ares Vallis. The chaotic terrain is widely believed to have formed via the removal of subsurface water or ice , resulting in flooding at the surface, and the formation of Ares Vallis. Within Iani Chaos, deposited stratigraphically above the chaotic terrain, are smooth, low-slope, intermediate-to-light-toned deposits that are rich in a hydrated mineral that is most likely gypsum as well as hematite . [1] |
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| 2016 |
35890 characters 4 sections 5 paragraphs 9 images 158 internal links 2 external links |
iani 0.648 chaos 0.449 ares 0.173 gypsum 0.147 sites 0.124 hematite 0.122 stratigraphically 0.121 chaotic 0.116 examine 0.114 margaritifer 0.112 vallis 0.111 sinus 0.105 terrain 0.103 342 0.095 smooth 0.094 |
Iani Chaos is a region of chaos terrain at the south end of the outflow channel Ares Vallis , of the Margaritifer Sinus quadrangle (MC-19) region of the planet Mars , centered at approximately ~342°E, 2°S. This is the source region of Ares Vallis. The chaotic terrain is widely believed to have formed via the removal of subsurface water or ice , resulting in flooding at the surface, and the formation of Ares Vallis. Within Iani Chaos, deposited stratigraphically above the chaotic terrain, are smooth, low-slope, intermediate-to-light-toned deposits that are rich in a hydrated mineral that is most likely gypsum as well as hematite . [1] |
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| 2015 |
36117 characters 4 sections 5 paragraphs 9 images 159 internal links 2 external links |
iani 0.648 chaos 0.449 ares 0.173 gypsum 0.147 sites 0.124 hematite 0.122 stratigraphically 0.121 chaotic 0.116 examine 0.114 margaritifer 0.112 vallis 0.111 sinus 0.105 terrain 0.103 342 0.095 smooth 0.094 |
Iani Chaos is a region of chaos terrain at the south end of the outflow channel Ares Vallis , of the Margaritifer Sinus quadrangle (MC-19) region of the planet Mars , centered at approximately ~342°E, 2°S. This is the source region of Ares Vallis. The chaotic terrain is widely believed to have formed via the removal of subsurface water or ice , resulting in flooding at the surface, and the formation of Ares Vallis. Within Iani Chaos, deposited stratigraphically above the chaotic terrain, are smooth, low-slope, intermediate-to-light-toned deposits that are rich in a hydrated mineral that is most likely gypsum as well as hematite . [1] |
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| 2014 |
35876 characters 4 sections 5 paragraphs 9 images 159 internal links 2 external links |
iani 0.648 chaos 0.449 ares 0.173 gypsum 0.147 sites 0.124 hematite 0.122 stratigraphically 0.121 chaotic 0.116 examine 0.114 margaritifer 0.112 vallis 0.111 sinus 0.105 terrain 0.103 342 0.095 smooth 0.094 |
Iani Chaos is a region of chaos terrain at the south end of the outflow channel Ares Vallis , of the Margaritifer Sinus quadrangle (MC-19) region of the planet Mars , centered at approximately ~342°E, 2°S. This is the source region of Ares Vallis. The chaotic terrain is widely believed to have formed via the removal of subsurface water or ice , resulting in flooding at the surface, and the formation of Ares Vallis. Within Iani Chaos, deposited stratigraphically above the chaotic terrain, are smooth, low-slope, intermediate-to-light-toned deposits that are rich in a hydrated mineral that is most likely gypsum as well as hematite . [1] |
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| 2013 |
34916 characters 4 sections 5 paragraphs 8 images 157 internal links 2 external links |
iani 0.662 chaos 0.402 ares 0.177 gypsum 0.150 sites 0.127 hematite 0.125 stratigraphically 0.124 chaotic 0.119 examine 0.117 margaritifer 0.114 vallis 0.114 sinus 0.107 342 0.097 smooth 0.096 zone 0.096 |
Iani Chaos is a minor canyon accounting for a portion of the extraterrestrial valley, Ares Vallis , of the Margaritifer Sinus quadrangle (MC-19) region of the planet Mars . This is the source region of Ares Vallis on Mars, where it is centered at approximately ~342°E, 2°S. The chaotic terrain is widely believed to have formed via the removal of subsurface water or ice , resulting in flooding at the surface, and the formation of Ares Vallis. Within Iani Chaos, deposited stratigraphically above the chaotic terrain, are smooth, low-slope, intermediate-to-light-toned deposits that are rich in a hydrated mineral that is most likely gypsum as well as hematite . [1] |
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| 2012 |
29777 characters 3 sections 6 paragraphs 7 images 156 internal links 2 external links |
iani 0.686 chaos 0.416 gypsum 0.155 sites 0.131 hematite 0.129 stratigraphically 0.128 chaotic 0.123 ares 0.122 examine 0.121 342 0.100 smooth 0.100 zone 0.099 themis 0.094 landing 0.092 ponded 0.091 |
Iani Chaos , the source region of Ares Vallis on Mars , is centered at ~342°E, 2°S. The chaotic terrain is widely believed to have formed via the removal of subsurface water or ice , resulting in flooding at the surface, and the formation of Ares Vallis. Within Iani Chaos, deposited stratigraphically above the chaotic terrain, are smooth, low-slope, intermediate-to-light-toned deposits that are rich in a hydrated mineral that is most likely gypsum as well as hematite . [1] |
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| 2011 |
29777 characters 3 sections 6 paragraphs 7 images 156 internal links 2 external links |
iani 0.686 chaos 0.416 gypsum 0.155 sites 0.131 hematite 0.129 stratigraphically 0.128 chaotic 0.123 ares 0.122 examine 0.121 342 0.100 smooth 0.100 zone 0.099 themis 0.094 landing 0.092 ponded 0.091 |
Iani Chaos , the source region of Ares Vallis on Mars , is centered at ~342°E, 2°S. The chaotic terrain is widely believed to have formed via the removal of subsurface water or ice , resulting in flooding at the surface, and the formation of Ares Vallis. Within Iani Chaos, deposited stratigraphically above the chaotic terrain, are smooth, low-slope, intermediate-to-light-toned deposits that are rich in a hydrated mineral that is most likely gypsum as well as hematite . [1] |
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| 2010 |
29777 characters 3 sections 6 paragraphs 7 images 156 internal links 2 external links |
iani 0.686 chaos 0.416 gypsum 0.155 sites 0.131 hematite 0.129 stratigraphically 0.128 chaotic 0.123 ares 0.122 examine 0.121 342 0.100 smooth 0.100 zone 0.099 themis 0.094 landing 0.092 ponded 0.091 |
Iani Chaos , the source region of Ares Vallis on Mars , is centered at ~342°E, 2°S. The chaotic terrain is widely believed to have formed via the removal of subsurface water or ice , resulting in flooding at the surface, and the formation of Ares Vallis. Within Iani Chaos, deposited stratigraphically above the chaotic terrain, are smooth, low-slope, intermediate-to-light-toned deposits that are rich in a hydrated mineral that is most likely gypsum as well as hematite . [1] |
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| 2009 |
29691 characters 3 sections 6 paragraphs 7 images 155 internal links 2 external links |
iani 0.686 chaos 0.416 gypsum 0.155 sites 0.131 hematite 0.129 stratigraphically 0.128 chaotic 0.123 ares 0.122 examine 0.121 342 0.100 smooth 0.100 zone 0.099 themis 0.094 landing 0.092 ponded 0.091 |
Iani Chaos , the source region of Ares Vallis on Mars , is centered at ~342°E, 2°S. The chaotic terrain is widely believed to have formed via the removal of subsurface water or ice , resulting in flooding at the surface, and the formation of Ares Vallis. Within Iani Chaos, deposited stratigraphically above the chaotic terrain, are smooth, low-slope, intermediate-to-light-toned deposits that are rich in a hydrated mineral that is most likely gypsum as well as hematite [1] . |
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| 2008 |
25517 characters 2 sections 1 paragraphs 5 images 153 internal links 1 external links |
iani 0.469 stratigraphically 0.306 chaotic 0.294 ares 0.292 chaos 0.284 342 0.240 flooding 0.192 vallis 0.188 gypsum 0.186 terrain 0.173 removal 0.156 hematite 0.154 intermediate 0.148 toned 0.146 hydrated 0.131 |
Iani Chaos , the source region of Ares Vallis on Mars , is centered at ~342°E, 2°S. The chaotic terrain is widely believed to have formed via the removal of subsurface water or ice , resulting in flooding at the surface, and the formation of Ares Vallis. Within Iani Chaos, deposited stratigraphically above the chaotic terrain, are smooth, low-slope, intermediate-to-light-toned deposits that are rich in a hydrated mineral that is most likely gypsum as well as hematite [1] . |
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| 2007 |
5104 characters 2 sections 2 paragraphs 2 images 11 internal links 1 external links |
iani 0.451 stratigraphically 0.294 chaotic 0.282 ares 0.281 template 0.276 chaos 0.273 342 0.231 flooding 0.184 vallis 0.180 gypsum 0.178 terrain 0.166 removal 0.150 hematite 0.148 intermediate 0.142 toned 0.140 |
Iani Chaos , the source region of Ares Vallis on Mars , is centered at ~342°E, 2°S. The chaotic terrain is widely believed to have formed via the removal of subsurface water or ice , resulting in flooding at the surface, and the formation of Ares Vallis. Within Iani Chaos, deposited stratigraphically above the chaotic terrain, are smooth, low-slope, intermediate-to-light-toned deposits that are rich in a hydrated mineral that is most likely gypsum as well as hematite [1] . |