Melas Chasma
Melas Chasma is a canyon on Mars , the widest segment of the Valles Marineris canyon system, [1] located east of Ius Chasma at 9.8°S, 283.6°E in Coprates quadrangle . It cuts through layered deposits that are thought to be sediments from an old lake that resulted from runoff of the valley networks to the west. [2] Other theories include windblown sediment deposits and volcanic ash. [1] Support for abundant, past water in Melas Chasma is the discovery by MRO of hydrated sulfates. In addition, sulfate and iron oxides were found by the same satellite. [3] Although not chosen as one of the finalists, it was one of eight potential landing sites for the Mars 2020 rover, a mission with a focus on astrobiology.
Page Revisions
| Year | Metadata | Sections | Top Words | First Paragraph |
| 2018 |
91325 characters 3 sections 9 paragraphs 10 images 672 internal links 9 external links |
melas 0.666 chasma 0.460 canyon 0.184 dem 0.157 channels 0.109 eleven 0.097 fluctuating 0.087 lake 0.081 ash 0.080 whipped 0.078 marineris 0.075 digital 0.074 fluid 0.067 networks 0.067 click 0.066 |
Melas Chasma is a canyon on Mars , the widest segment of the Valles Marineris canyon system, [1] located east of Ius Chasma at 9.8°S, 283.6°E in Coprates quadrangle . It cuts through layered deposits that are thought to be sediments from an old lake that resulted from runoff of the valley networks to the west. [2] Other theories include windblown sediment deposits and volcanic ash. [1] Support for abundant, past water in Melas Chasma is the discovery by MRO of hydrated sulfates. In addition, sulfate and iron oxides were found by the same satellite. [3] Although not chosen as one of the finalists, it was one of eight potential landing sites for the Mars 2020 rover, a mission with a focus on astrobiology. |
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| 2017 |
49502 characters 3 sections 9 paragraphs 10 images 190 internal links 7 external links |
melas 0.666 chasma 0.460 canyon 0.184 dem 0.157 channels 0.109 eleven 0.097 fluctuating 0.087 lake 0.081 ash 0.080 whipped 0.078 marineris 0.075 digital 0.074 fluid 0.067 networks 0.067 click 0.066 |
Melas Chasma is a canyon on Mars , the widest segment of the Valles Marineris canyon system, [1] located east of Ius Chasma at 9.8°S, 283.6°E in Coprates quadrangle . It cuts through layered deposits that are thought to be sediments from an old lake that resulted from runoff of the valley networks to the west. [2] Other theories include windblown sediment deposits and volcanic ash. [1] Support for abundant, past water in Melas Chasma is the discovery by MRO of hydrated sulfates. In addition, sulfate and iron oxides were found by the same satellite. [3] Although not chosen as one of the finalists, it was one of eight potential landing sites for the Mars 2020 rover, a mission with a focus on astrobiology. |
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| 2016 |
46183 characters 3 sections 8 paragraphs 10 images 186 internal links 6 external links |
melas 0.668 chasma 0.415 canyon 0.221 eleven 0.117 fluctuating 0.105 lake 0.098 ash 0.096 whipped 0.094 marineris 0.091 fluid 0.081 click 0.079 windblown 0.078 datasets 0.076 layered 0.076 283 0.074 |
Melas Chasma is a canyon on Mars , the widest segment of the Valles Marineris canyon system, [1] located east of Ius Chasma at 9.8°S, 283.6°E in Coprates quadrangle . It cuts through layered deposits that are thought to be sediments from an old lake that resulted from runoff of the valley networks to the west. [2] Other theories include windblown sediment deposits and volcanic ash. [1] Support for abundant, past water in Melas Chasma is the discovery by MRO of hydrated sulfates. In addition, sulfate and iron oxides were found by the same satellite. [3] It is one of eight potential landing sites for the Mars 2020 rover, a mission with a focus on astrobiology. |
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| 2015 |
46184 characters 3 sections 8 paragraphs 10 images 186 internal links 6 external links |
melas 0.669 chasma 0.415 canyon 0.221 eleven 0.117 fluctuating 0.105 lake 0.098 ash 0.096 whipped 0.094 marineris 0.091 fluid 0.081 click 0.079 windblown 0.078 datasets 0.076 layered 0.076 283 0.074 |
Melas Chasma is a canyon on Mars , the widest segment of the Valles Marineris canyon system, [1] located east of Ius Chasma at 9.8°S, 283.6°E in Coprates quadrangle . It cuts through layered deposits that are thought to be sediments from an old lake that resulted from runoff of the valley networks to the west. [2] Other theories include windblown sediment deposits and volcanic ash. [1] Support for abundant, past water in Melas Chasma is the discovery by MRO of hydrated sulfates. In addition, sulfate and iron oxides were found by the same satellite. [3] It is one of eight potential landing sites for the Mars 2020 rover, a mission with a focus on astrobiology. |
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| 2014 |
38643 characters 2 sections 8 paragraphs 10 images 165 internal links 5 external links |
melas 0.672 chasma 0.417 canyon 0.222 eleven 0.117 fluctuating 0.105 lake 0.098 ash 0.096 whipped 0.095 marineris 0.091 fluid 0.082 click 0.079 windblown 0.079 datasets 0.076 layered 0.076 283 0.074 |
Melas Chasma is a canyon on Mars , the widest segment of the Valles Marineris canyon system, [1] located east of Ius Chasma at 9.8°S, 283.6°E in Coprates quadrangle . It cuts through layered deposits that are thought to be sediments from an old lake that resulted from runoff of the valley networks to the west. [2] Other theories include windblown sediment deposits and volcanic ash. [1] Support for abundant, past water in Melas Chasma is the discovery by MRO of hydrated sulfates. In addition, sulfate and iron oxides were found by the same satellite. [3] |
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| 2013 |
37883 characters 2 sections 7 paragraphs 10 images 164 internal links 5 external links |
melas 0.638 chasma 0.385 canyon 0.264 ash 0.114 whipped 0.113 marineris 0.108 fluid 0.097 click 0.094 windblown 0.093 layered 0.090 283 0.088 deposits 0.088 eolian 0.084 layers 0.084 shadowed 0.083 |
Melas Chasma is a canyon on Mars , the widest segment of the Valles Marineris canyon system, [1] located east of Ius Chasma at 9.8°S, 283.6°E. It cuts through layered deposits that are thought to be sediments from an old lake that resulted from runoff of the valley networks to the west. [2] Other theories include windblown sediment deposits and volcanic ash. [1] Support for abundant, past water in Melas Chasma is the discovery by MRO of hydrated sulfates. In addition, sulfate and iron oxides were found by the same satellite. [3] |
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| 2012 |
16555 characters 2 sections 8 paragraphs 6 images 21 internal links 5 external links |
melas 0.638 chasma 0.385 canyon 0.264 ash 0.114 whipped 0.113 marineris 0.108 fluid 0.097 click 0.094 windblown 0.093 layered 0.090 283 0.088 deposits 0.088 eolian 0.084 layers 0.084 shadowed 0.083 |
Melas Chasma is a canyon on Mars , the widest segment of the Valles Marineris canyon system, [1] located east of Ius Chasma at 9.8°S, 283.6°E. It cuts through layered deposits that are thought to be sediments from an old lake that resulted from runoff of the valley networks to the west. [2] Other theories include windblown sediment deposits and volcanic ash. [1] Support for abundant, past water in Melas Chasma is the discovery by MRO of hydrated sulfates. In addition, sulfate and iron oxides were found by the same satellite. [3] |
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| 2011 |
14677 characters 2 sections 7 paragraphs 5 images 15 internal links 4 external links |
melas 0.611 chasma 0.362 canyon 0.289 ash 0.125 whipped 0.123 marineris 0.118 fluid 0.106 click 0.103 windblown 0.102 layered 0.099 283 0.097 deposits 0.096 eolian 0.092 layers 0.092 widest 0.089 |
Melas Chasma is a canyon on Mars , the widest segment of the Valles Marineris canyon system, [1] located east of Ius Chasma at 9.8°S, 283.6°E. It cuts through layered deposits that are thought to be sediments from an old lake that resulted from runoff of the valley networks to the west. [2] Other theories include windblown sediment deposits and volcanic ash. [1] Support for abundant, past water in Melas Chasma is the discovery by MRO of hydrated sulfates. In addition, sulfate and iron oxides were found by the same satellite. [3] |
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| 2010 |
10614 characters 1 sections 6 paragraphs 5 images 12 internal links 2 external links |
melas 0.611 chasma 0.362 canyon 0.289 ash 0.125 whipped 0.123 marineris 0.118 fluid 0.106 click 0.103 windblown 0.102 layered 0.099 283 0.097 deposits 0.096 eolian 0.092 layers 0.092 widest 0.089 |
Melas Chasma is a canyon on Mars , the widest segment of the Valles Marineris canyon system, [1] located east of Ius Chasma at 9.8°S, 283.6°E. It cuts through layered deposits that are thought to be sediments from an old lake that resulted from runoff of the valley networks to the west. [2] Other theories include windblown sediment deposits and volcanic ash. [1] Support for abundant, past water in Melas Chasma is the discovery by MRO of hydrated sulfates. In addition, sulfate and iron oxides were found by the same satellite. [3] |
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| 2009 |
9780 characters 1 sections 5 paragraphs 5 images 11 internal links 2 external links |
melas 0.604 chasma 0.347 canyon 0.267 ash 0.144 whipped 0.142 marineris 0.136 fluid 0.122 click 0.119 windblown 0.118 layered 0.114 283 0.111 deposits 0.111 eolian 0.106 layers 0.106 widest 0.102 |
Melas Chasma is a canyon on Mars , the widest segment of the Valles Marineris canyon system, [1] located east of Ius Chasma at 9.8°S, 283.6°E. It cuts through layered deposits that are thought to be sediments from an old lake that resulted from runoff of the valley networks to the west. [2] Other theories include windblown sediment deposits and volcanic ash. [1] |
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| 2008 |
6919 characters 1 sections 2 paragraphs 2 images 9 internal links 2 external links |
melas 0.412 canyon 0.364 chasma 0.284 ash 0.197 whipped 0.194 marineris 0.186 fluid 0.167 windblown 0.161 283 0.152 eolian 0.145 widest 0.140 plains 0.139 slide 0.135 lake 0.134 ius 0.133 |
Melas Chasma is a canyon on Mars , the widest segment of the Valles Marineris canyon system, [1] located east of Ius Chasma at 9.8°S, 283.6°E. It cuts through layered deposits that are thought to be sediments from an old lake that resulted from runoff of the valley networks to the west. [2] Other theories include windblown sediment deposits and volcanic ash. [1] |
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| 2007 |
6893 characters 1 sections 2 paragraphs 2 images 9 internal links 2 external links |
melas 0.412 canyon 0.364 chasma 0.284 ash 0.197 whipped 0.194 marineris 0.186 fluid 0.167 windblown 0.161 283 0.152 eolian 0.145 widest 0.140 plains 0.139 slide 0.135 lake 0.134 ius 0.133 |
Melas Chasma is a canyon on Mars , the widest segment of the Valles Marineris canyon system, [1] located east of Ius Chasma at 9.8°S, 283.6°E. It cuts through layered deposits that are thought to be sediments from an old lake that resulted from runoff of the valley networks to the west. [2] Other theories include windblown sediment deposits and volcanic ash. [1] |