Candor Chasma
Candor Chasma is one of the largest canyons in the Valles Marineris canyon system on Mars . The feature is geographically divided into two halves: East and West Candor Chasmas, respectively. It is unclear how the canyon originally formed; one theory is that it was expanded and deepened by tectonic processes similar to a graben , while another suggests that it was formed by subsurface water erosion similar to a karst . [1] MRO discovered sulfates, hydrated sulfates, and iron oxides in Candor Chasma. [2]
Page Revisions
| Year | Metadata | Sections | Top Words | First Paragraph |
| 2018 |
81015 characters 6 sections 7 paragraphs 6 images 654 internal links 14 external links |
candor 0.694 chasma 0.403 mensa 0.226 ceti 0.184 canyon 0.161 labes 0.138 nia 0.123 ophir 0.105 catenae 0.103 connects 0.103 channels 0.096 chaos 0.096 east 0.094 branched 0.082 baetis 0.076 |
Candor Chasma is one of the largest canyons in the Valles Marineris canyon system on Mars . The feature is geographically divided into two halves: East and West Candor Chasmas, respectively. It is unclear how the canyon originally formed; one theory is that it was expanded and deepened by tectonic processes similar to a graben , while another suggests that it was formed by subsurface water erosion similar to a karst . [1] MRO discovered sulfates, hydrated sulfates, and iron oxides in Candor Chasma. [2] |
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| 2017 |
34880 characters 3 sections 6 paragraphs 9 images 163 internal links 5 external links |
candor 0.632 chasma 0.286 canyon 0.206 channels 0.204 branched 0.175 coprates 0.167 deepened 0.162 chasmas 0.146 marineris 0.140 canyons 0.140 sulfates 0.140 geographically 0.137 tectonic 0.130 karst 0.125 halves 0.121 |
Candor Chasma is one of the largest canyons in the Valles Marineris canyon system on Mars . The feature is geographically divided into two halves: East and West Candor Chasmas, respectively. It is unclear how the canyon originally formed; one theory is that it was expanded and deepened by tectonic processes similar to a graben , while another suggests that it was formed by subsurface water erosion similar to a karst . [1] MRO discovered sulfates, hydrated sulfates, and iron oxides in Candor Chasma. [2] |
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| 2016 |
31150 characters 2 sections 4 paragraphs 9 images 159 internal links 4 external links |
candor 0.682 chasma 0.308 canyon 0.222 coprates 0.181 deepened 0.175 chasmas 0.158 marineris 0.151 canyons 0.151 sulfates 0.151 geographically 0.148 tectonic 0.140 karst 0.135 halves 0.131 valles 0.102 branched 0.095 |
Candor Chasma is one of the largest canyons in the Valles Marineris canyon system on Mars . The feature is geographically divided into two halves: East and West Candor Chasmas, respectively. It is unclear how the canyon originally formed; one theory is that it was expanded and deepened by tectonic processes similar to a graben , while another suggests that it was formed by subsurface water erosion similar to a karst . [1] MRO discovered sulfates, hydrated sulfates, and iron oxides in Candor Chasma. [2] |
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| 2015 |
31149 characters 2 sections 4 paragraphs 9 images 159 internal links 4 external links |
candor 0.682 chasma 0.308 canyon 0.222 coprates 0.181 deepened 0.175 chasmas 0.158 marineris 0.151 canyons 0.151 sulfates 0.151 geographically 0.148 tectonic 0.140 karst 0.135 halves 0.131 valles 0.102 branched 0.095 |
Candor Chasma is one of the largest canyons in the Valles Marineris canyon system on Mars . The feature is geographically divided into two halves: East and West Candor Chasmas, respectively. It is unclear how the canyon originally formed; one theory is that it was expanded and deepened by tectonic processes similar to a graben , while another suggests that it was formed by subsurface water erosion similar to a karst . [1] MRO discovered sulfates, hydrated sulfates, and iron oxides in Candor Chasma. [2] |
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| 2013 |
30963 characters 2 sections 4 paragraphs 9 images 159 internal links 3 external links |
candor 0.682 chasma 0.308 canyon 0.222 coprates 0.181 deepened 0.175 chasmas 0.158 marineris 0.151 canyons 0.151 sulfates 0.151 geographically 0.148 tectonic 0.140 karst 0.135 halves 0.131 valles 0.102 branched 0.095 |
Candor Chasma is one of the largest canyons in the Valles Marineris canyon system on Mars . The feature is geographically divided into two halves: East and West Candor Chasmas, respectively. It is unclear how the canyon originally formed; one theory is that it was expanded and deepened by tectonic processes similar to a graben , while another suggests that it was formed by subsurface water erosion similar to a karst . [1] MRO discovered sulfates, hydrated sulfates, and iron oxides in Candor Chasma. [2] |
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| 2012 |
9600 characters 2 sections 5 paragraphs 6 images 15 internal links 3 external links |
candor 0.682 chasma 0.308 canyon 0.222 coprates 0.181 deepened 0.175 chasmas 0.158 marineris 0.151 canyons 0.151 sulfates 0.151 geographically 0.148 tectonic 0.140 karst 0.135 halves 0.131 valles 0.102 branched 0.095 |
Candor Chasma is one of the largest canyons in the Valles Marineris canyon system on Mars . The feature is geographically divided into two halves: East and West Candor Chasmas, respectively. It is unclear how the canyon originally formed; one theory is that it was expanded and deepened by tectonic processes similar to a graben , while another suggests that it was formed by subsurface water erosion similar to a karst . [1] MRO discovered sulfates, hydrated sulfates, and iron oxides in Candor Chasma. [2] |
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| 2011 |
8297 characters 2 sections 4 paragraphs 5 images 11 internal links 3 external links |
candor 0.638 chasma 0.260 canyon 0.249 coprates 0.203 deepened 0.196 chasmas 0.177 marineris 0.170 canyons 0.169 sulfates 0.169 geographically 0.166 karst 0.152 halves 0.147 valles 0.114 branched 0.106 channels 0.099 |
Candor Chasma is one of the largest canyons in the Valles Marineris canyon system on Mars . The feature is geographically divided into two halves: East and West Candor Chasmas, respectively. It is unclear how the canyon originally formed; one theory is that it was expanded and deepened by tectonic processes similar to a graben , while another suggests that it was formed by subsurface water erosion similar to a karst . [1] MRO discovered sulfates, hydrated sulfates, and iron oxides in Candor Chasma. [2] |
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| 2010 |
8295 characters 2 sections 4 paragraphs 5 images 11 internal links 3 external links |
candor 0.638 chasma 0.260 canyon 0.249 coprates 0.203 deepened 0.196 chasmas 0.177 marineris 0.170 canyons 0.169 sulfates 0.169 geographically 0.166 karst 0.152 halves 0.147 valles 0.114 branched 0.106 channels 0.099 |
Candor Chasma is one of the largest canyons in the Valles Marineris canyon system on Mars . The feature is geographically divided into two halves: East and West Candor Chasmas, respectively. It is unclear how the canyon originally formed; one theory is that it was expanded and deepened by tectonic processes similar to a graben , while another suggests that it was formed by subsurface water erosion similar to a karst . [1] MRO discovered sulfates, hydrated sulfates, and iron oxides in Candor Chasma. [2] |
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| 2009 |
6596 characters 2 sections 3 paragraphs 4 images 9 internal links 2 external links |
candor 0.514 canyon 0.335 deepened 0.264 chasmas 0.238 chasma 0.232 marineris 0.228 canyons 0.227 geographically 0.223 karst 0.204 halves 0.197 valles 0.154 coprates 0.136 unclear 0.132 graben 0.130 largest 0.111 |
Candor Chasma is one of the largest canyons in the Valles Marineris canyon system on Mars . The feature is geographically divided into two halves: East and West Candor Chasmas, respectively. It is unclear how the canyon originally formed; one theory is that it was expanded and deepened by tectonic processes similar to a graben , while another suggests that it was formed by subsurface water erosion similar to a karst . [1] |
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| 2008 |
5505 characters 2 sections 1 paragraphs 3 images 9 internal links 2 external links |
deepened 0.452 canyon 0.383 karst 0.350 candor 0.294 unclear 0.226 graben 0.222 chasma 0.199 marineris 0.196 canyons 0.195 expanded 0.188 tectonic 0.181 theory 0.148 subsurface 0.145 erosion 0.142 formed 0.136 |
Candor Chasma is one of the largest canyons in the Valles Marineris canyon system on Mars . It is unclear how the canyon originally formed; one theory is that it was expanded and deepened by tectonic processes similar to a graben , while another suggests that it was formed by subsurface water erosion similar to a karst . [1] |
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| 2007 |
5521 characters 2 sections 1 paragraphs 3 images 9 internal links 2 external links |
deepened 0.452 canyon 0.383 karst 0.350 candor 0.294 unclear 0.226 graben 0.222 chasma 0.199 marineris 0.196 canyons 0.195 expanded 0.188 tectonic 0.181 theory 0.148 subsurface 0.145 erosion 0.142 formed 0.136 |
Candor Chasma is one of the largest canyons in the Valles Marineris canyon system on Mars . It is unclear how the canyon originally formed; one theory is that it was expanded and deepened by tectonic processes similar to a graben , while another suggests that it was formed by subsurface water erosion similar to a karst . [1] |