Eos Chasma
Eos Chasma is a chasma in the southern part of the Valles Marineris canyon system of the Coprates quadrangle and the Margaritifer Sinus quadrangles of the planet Mars .
Page Revisions
| Year | Metadata | Sections | Top Words | First Paragraph |
| 2018 |
75605 characters 3 sections 6 paragraphs 6 images 655 internal links 3 external links |
eos 0.677 chasma 0.566 vicky 0.129 sulfate 0.104 offshoot 0.103 striations 0.096 conclusive 0.096 alh84001 0.089 eolian 0.087 longitudinal 0.081 etched 0.081 ganges 0.081 hamilton 0.081 bars 0.077 obscured 0.075 |
Eos Chasma is a chasma in the southern part of the Valles Marineris canyon system of the Coprates quadrangle and the Margaritifer Sinus quadrangles of the planet Mars . |
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| 2017 |
34212 characters 3 sections 6 paragraphs 9 images 164 internal links 3 external links |
eos 0.677 chasma 0.566 vicky 0.129 sulfate 0.104 offshoot 0.103 striations 0.096 conclusive 0.096 alh84001 0.089 eolian 0.087 longitudinal 0.081 etched 0.081 ganges 0.081 hamilton 0.081 bars 0.077 obscured 0.075 |
Eos Chasma is a chasma in the southern part of the Valles Marineris canyon system of the Coprates quadrangle and the Margaritifer Sinus quadrangles of the planet Mars . |
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| 2013 |
30674 characters 3 sections 4 paragraphs 8 images 161 internal links 2 external links |
eos 0.657 chasma 0.557 vicky 0.140 sulfate 0.113 offshoot 0.113 striations 0.105 conclusive 0.105 alh84001 0.097 eolian 0.095 longitudinal 0.088 etched 0.088 ganges 0.088 hamilton 0.088 bars 0.084 obscured 0.082 |
Eos Chasma is a chasma in the southern part of the Valles Marineris canyon system of the Margaritifer Sinus quadrangle (MC-19) region of the planet Mars . |
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| 2012 |
9205 characters 3 sections 4 paragraphs 4 images 18 internal links 2 external links |
eos 0.661 chasma 0.560 vicky 0.141 sulfate 0.114 offshoot 0.114 striations 0.106 conclusive 0.106 alh84001 0.098 eolian 0.095 longitudinal 0.089 etched 0.089 ganges 0.089 hamilton 0.089 bars 0.085 obscured 0.083 |
Eos Chasma’s western floor is mainly composed of an etched massive material composed of either volcanic or eolian deposits later eroded by the Martian wind. The eastern end of the Eos chasma has a large area of streamlined bars and longitudinal striations. This is interpreted to be stream-carved plateau deposits and material transported and deposited by flowing fluid. Ganges Chasma is an offshoot of Eos Chasma. MRO discovered sulfate, hydrated sulfate, and iron oxides in Eos Chasma. [1] |
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| 2010 |
9139 characters 3 sections 4 paragraphs 4 images 18 internal links 2 external links |
eos 0.661 chasma 0.560 vicky 0.141 sulfate 0.114 offshoot 0.114 striations 0.106 conclusive 0.106 alh84001 0.098 eolian 0.095 longitudinal 0.089 etched 0.089 ganges 0.089 hamilton 0.089 bars 0.085 obscured 0.083 |
Eos Chasma’s western floor is mainly composed of an etched massive material composed of either volcanic or eolian deposits later eroded by the Martian wind. The eastern end of the Eos chasma has a large area of streamlined bars and longitudinal striations. This is interpreted to be stream-carved plateau deposits and material transported and deposited by flowing fluid. Ganges Chasma is an offshoot of Eos Chasma. MRO discovered sulfate, hydrated sulfate, and iron oxides in Eos Chasma. [1] |
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| 2009 |
8172 characters 2 sections 4 paragraphs 4 images 17 internal links 2 external links |
eos 0.645 chasma 0.555 vicky 0.157 offshoot 0.127 striations 0.118 conclusive 0.118 alh84001 0.109 eolian 0.106 longitudinal 0.099 etched 0.099 ganges 0.099 hamilton 0.099 bars 0.095 obscured 0.092 composed 0.090 |
Eos Chasma’s western floor is mainly composed of an etched massive material composed of either volcanic or eolian deposits later eroded by the Martian wind. The eastern end of the Eos chasma has a large area of streamlined bars and longitudinal striations. This is interpreted to be stream-carved plateau deposits and material transported and deposited by flowing fluid. Ganges Chasma is an offshoot of Eos Chasma. |
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| 2007 |
7260 characters 2 sections 3 paragraphs 3 images 17 internal links 2 external links |
chasma 0.592 eos 0.562 vicky 0.192 offshoot 0.154 striations 0.144 alh84001 0.133 eolian 0.130 longitudinal 0.121 etched 0.121 ganges 0.121 hamilton 0.121 bars 0.115 composed 0.109 streamlined 0.091 deposits 0.090 |
Eos Chasma’s western floor is mainly composed of an etched massive material composed of either volcanic or eolian deposits later eroded by the Martian wind. The eastern end of the Eos chasma has a large area of streamlined bars and longitudinal striations. This is interpreted to be stream-carved plateau deposits and material transported and deposited by flowing fluid. Ganges Chasma is an offshoot of Eos Chasma. |
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| 2006 |
6146 characters 2 sections 5 paragraphs 2 images 15 internal links 2 external links |
chasma 0.593 eos 0.563 vicky 0.192 offshoot 0.155 striations 0.144 alh84001 0.133 eolian 0.130 longitudinal 0.121 etched 0.121 ganges 0.121 hamilton 0.121 bars 0.116 composed 0.110 streamlined 0.091 deposits 0.090 |
According to an analysis by Vicky Hamilton of the University of Hawaii , Eos Chasma may be the source of the ALH84001 meteorite, which some believe to be evidence of past life on Mars . |
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| 2005 |
4074 characters 1 sections 4 paragraphs 1 images 12 internal links 1 external links |
chasma 0.589 eos 0.559 vicky 0.191 gangis 0.172 offshoot 0.154 striations 0.143 alh84001 0.132 eolian 0.129 longitudinal 0.120 etched 0.120 hamilton 0.120 bars 0.115 composed 0.109 streamlined 0.090 deposits 0.090 |
According to an analysis by Vicky Hamilton of the University of Hawaii , Eos Chasma may be the source of the ALH84001 meteorite, which some believe to be evidence of past life on Mars . |