Aram Chaos
Aram Chaos , centered at 2.6°N, 21.5°W, [1] is a heavily eroded impact crater on the planet Mars . It lies at the eastern end of the large canyon Valles Marineris and close to Ares Vallis . Various geological processes have reduced it to a circular area of chaotic terrain . Aram Chaos takes its name from Aram, one of the classical albedo features observed by Giovanni Schiaparelli , who named it after the Biblical land of Aram . Spectroscopic observation from orbit indicates the presence of the mineral hematite , likely a signature of a once aqueous environment.
Page Revisions
| Year | Metadata | Sections | Top Words | First Paragraph |
| 2018 |
85516 characters 3 sections 11 paragraphs 13 images 668 internal links 6 external links |
aram 0.804 chaos 0.366 hematite 0.199 oxia 0.097 palus 0.076 eastern 0.075 themis 0.072 floods 0.067 collapsed 0.067 valleys 0.064 chaotic 0.063 ares 0.063 blocks 0.062 ramparts 0.062 water 0.060 |
Aram Chaos , centered at 2.6°N, 21.5°W, [1] is a heavily eroded impact crater on the planet Mars . It lies at the eastern end of the large canyon Valles Marineris and close to Ares Vallis . Various geological processes have reduced it to a circular area of chaotic terrain . Aram Chaos takes its name from Aram, one of the classical albedo features observed by Giovanni Schiaparelli , who named it after the Biblical land of Aram . Spectroscopic observation from orbit indicates the presence of the mineral hematite , likely a signature of a once aqueous environment. |
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| 2017 |
44156 characters 3 sections 11 paragraphs 16 images 175 internal links 6 external links |
aram 0.804 chaos 0.365 hematite 0.198 oxia 0.097 palus 0.076 eastern 0.075 themis 0.072 floods 0.067 collapsed 0.067 valleys 0.064 chaotic 0.063 ares 0.063 blocks 0.062 ramparts 0.062 water 0.060 |
Aram Chaos , centered at 2.6°N, 21.5°W, [1] comprises a heavily eroded impact crater on the planet Mars . It lies at the eastern end of the large canyon Valles Marineris and close to Ares Vallis . Various geological processes have reduced it to a circular area of chaotic terrain . Aram Chaos takes its name from Aram, one of the classical albedo features observed by Giovanni Schiaparelli , who named it after the Biblical land of Aram . Spectroscopic observation from orbit indicates the presence of the mineral hematite , likely a signature of a once aqueous environment. |
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| 2016 |
38749 characters 3 sections 7 paragraphs 12 images 172 internal links 5 external links |
aram 0.773 chaos 0.306 hematite 0.249 themis 0.091 floods 0.085 collapsed 0.084 oxia 0.082 chaotic 0.079 ares 0.079 blocks 0.077 ramparts 0.077 water 0.076 biblical 0.071 catastrophically 0.071 spectroscope 0.071 |
Aram Chaos , centered at 2.6°N, 21.5°W, [1] comprises a heavily eroded impact crater on the planet Mars . It lies at the eastern end of the large canyon Valles Marineris and close to Ares Vallis . Various geological processes have reduced it to a circular area of chaotic terrain . Aram Chaos takes its name from Aram, one of the classical albedo features observed by Giovanni Schiaparelli , who named it after the Biblical land of Aram . Spectroscopic observation from orbit indicates the presence of the mineral hematite , likely a signature of a once aqueous environment. |
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| 2015 |
38668 characters 3 sections 6 paragraphs 12 images 172 internal links 5 external links |
aram 0.773 chaos 0.306 hematite 0.249 themis 0.091 floods 0.085 collapsed 0.084 oxia 0.082 chaotic 0.079 ares 0.079 blocks 0.077 ramparts 0.077 water 0.076 biblical 0.071 catastrophically 0.071 spectroscope 0.071 |
Aram Chaos , centered at 2.6°N, 21.5°W, [1] comprises a heavily eroded impact crater on the planet Mars . It lies at the eastern end of the large canyon Valles Marineris and close to Ares Vallis . Various geological processes have reduced it to a circular area of chaotic terrain . Aram Chaos takes its name from Aram, one of the classical albedo features observed by Giovanni Schiaparelli , who named it after the Biblical land of Aram . Spectroscopic observation from orbit indicates the presence of the mineral hematite , likely a signature of a once aqueous environment. |
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| 2014 |
37839 characters 3 sections 5 paragraphs 11 images 172 internal links 6 external links |
aram 0.772 hematite 0.270 chaos 0.248 themis 0.098 floods 0.092 collapsed 0.091 chaotic 0.086 ares 0.085 blocks 0.084 ramparts 0.084 water 0.082 biblical 0.077 catastrophically 0.077 spectroscope 0.077 channels 0.075 |
Aram Chaos , centered at 2.6°N, 21.5°W, [1] comprises a heavily eroded impact crater on the planet Mars . It lies at the eastern end of the large canyon Valles Marineris and close to Ares Vallis . Various geological processes have reduced it to a circular area of chaotic terrain . Aram Chaos takes its name from Aram, one of the classical albedo features observed by Giovanni Schiaparelli , who named it after the Biblical land of Aram . Spectroscopic observation from orbit indicates the presence of the mineral hematite , likely a signature of a once aqueous environment. |
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| 2013 |
36933 characters 3 sections 5 paragraphs 10 images 171 internal links 6 external links |
aram 0.772 hematite 0.270 chaos 0.248 themis 0.098 floods 0.092 collapsed 0.091 chaotic 0.086 ares 0.085 blocks 0.084 ramparts 0.084 water 0.082 biblical 0.077 catastrophically 0.077 spectroscope 0.077 channels 0.075 |
Aram Chaos , centered at 2.6°N, 21.5°W, [1] comprises a heavily eroded impact crater on the planet Mars . It lies at the eastern end of the large canyon Valles Marineris and close to Ares Vallis . Various geological processes have reduced it to a circular area of chaotic terrain . Aram Chaos takes its name from Aram, one of the classical albedo features observed by Giovanni Schiaparelli , who named it after the Biblical land of Aram . Spectroscopic observation from orbit indicates the presence of the mineral hematite , likely a signature of a once aqueous environment. |
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| 2012 |
14875 characters 2 sections 6 paragraphs 6 images 26 internal links 5 external links |
aram 0.772 hematite 0.270 chaos 0.248 themis 0.098 floods 0.092 collapsed 0.091 chaotic 0.086 ares 0.085 blocks 0.084 ramparts 0.084 water 0.082 biblical 0.077 catastrophically 0.077 spectroscope 0.077 channels 0.075 |
Aram Chaos , centered at 2.6°N, 21.5°W, [1] comprises a heavily eroded impact crater on the planet Mars . It lies at the eastern end of the large canyon Valles Marineris and close to Ares Vallis . Various geological processes have reduced it to a circular area of chaotic terrain . Aram Chaos takes its name from Aram, one of the classical albedo features observed by Giovanni Schiaparelli , who named it after the Biblical land of Aram . Spectroscopic observation from orbit indicates the presence of the mineral hematite , likely a signature of a once aqueous environment. |
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| 2011 |
14876 characters 2 sections 6 paragraphs 7 images 26 internal links 5 external links |
aram 0.772 hematite 0.270 chaos 0.248 themis 0.098 floods 0.092 collapsed 0.091 chaotic 0.086 ares 0.085 blocks 0.084 ramparts 0.084 water 0.082 biblical 0.077 catastrophically 0.077 spectroscope 0.077 channels 0.075 |
Aram Chaos , centered at 2.6°N, 21.5°W, [1] comprises a heavily eroded impact crater on the planet Mars . It lies at the eastern end of the large canyon Valles Marineris and close to Ares Vallis . Various geological processes have reduced it to a circular area of chaotic terrain . Aram Chaos takes its name from Aram, one of the classical albedo features observed by Giovanni Schiaparelli , who named it after the Biblical land of Aram . Spectroscopic observation from orbit indicates the presence of the mineral hematite , likely a signature of a once aqueous environment. |
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| 2010 |
14881 characters 2 sections 6 paragraphs 7 images 26 internal links 5 external links |
aram 0.771 hematite 0.270 chaos 0.248 themis 0.098 floods 0.092 collapsed 0.091 chaotic 0.086 ares 0.085 blocks 0.084 ramparts 0.084 water 0.082 biblical 0.076 catastrophically 0.076 spectroscope 0.076 channels 0.075 |
Aram Chaos , centered at 2.6°N, 21.5°W, [1] comprises a heavily eroded impact crater on the planet Mars . It lies at the eastern end of the large canyon Valles Marineris and close to Ares Vallis . Various geological processes have reduced it to a circular area of chaotic terrain . Aram Chaos takes its name from Aram, one of the classical albedo features observed by Giovanni Schiaparelli , who named it after the Biblical land of Aram . Spectroscopic observation from orbit indicates the presence of the mineral hematite , likely a signature of a once aqueous environment. |
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| 2009 |
14691 characters 2 sections 6 paragraphs 7 images 27 internal links 5 external links |
aram 0.786 chaos 0.253 hematite 0.229 themis 0.100 floods 0.093 collapsed 0.092 chaotic 0.087 ares 0.087 blocks 0.085 ramparts 0.085 water 0.083 biblical 0.078 catastrophically 0.078 channels 0.076 mineral 0.074 |
Aram Chaos , centered at 2.6°N, 21.5°W, [1] comprises a heavily eroded impact crater on the planet Mars . It lies at the eastern end of the large canyon Valles Marineris and close to Ares Vallis . Various geological processes have reduced it to a circular area of chaotic terrain . Aram Chaos takes its name from Aram, one of the classical albedo features observed by Giovanni Schiaparelli , which was named in turn [ by whom? ] after the Biblical land of Aram . Spectroscopic observation from orbit indicates the presence of the mineral hematite , likely a signature of a once aqueous environment. |
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| 2008 |
10569 characters 2 sections 3 paragraphs 3 images 13 internal links 5 external links |
aram 0.660 hematite 0.330 chaos 0.182 floods 0.134 chaotic 0.126 ares 0.125 ramparts 0.123 catastrophically 0.112 mineral 0.106 poured 0.105 water 0.103 circulates 0.103 eastern 0.100 eroded 0.096 stayed 0.096 |
Aram Chaos , centered at 2.6°N, 21.5°W, [1] is a heavily eroded impact crater on the planet Mars . It is located at the eastern end of the large canyon Valles Marineris . Various geological processes have reduced it to a circular area of chaotic terrain . Spectroscopic observation from orbit indicates the presence of the mineral hematite , likely a signature of a once aqueous environment. |
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| 2007 |
8843 characters 2 sections 1 paragraphs 3 images 13 internal links 4 external links |
aram 0.337 signature 0.255 spectroscopic 0.255 aqueous 0.255 hematite 0.236 marineris 0.224 chaotic 0.224 canyon 0.219 chaos 0.217 heavily 0.203 mineral 0.190 reduced 0.181 eastern 0.179 centered 0.176 eroded 0.172 |
Aram Chaos , centered at 2.6°N, 21.5°W, [1] is a heavily eroded impact crater on the planet Mars . It is located at the eastern end of the large canyon Valles Marineris . Various geological processes have reduced it to circular area of chaotic terrain . Spectroscopic observation from orbit indicates the presence of the mineral hematite , likely a signature of a once aqueous environment. |
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| 2006 |
8245 characters 2 sections 1 paragraphs 3 images 11 internal links 4 external links |
aram 0.426 marineris 0.284 chaotic 0.284 canyon 0.277 chaos 0.274 heavily 0.257 reduced 0.229 eastern 0.226 centered 0.223 eroded 0.218 circular 0.198 valles 0.191 21 0.170 processes 0.169 terrain 0.167 |
Aram Chaos , centered at 2.6°N, 21.5°W, [1] is a heavily eroded impact crater on the planet Mars . The located at the eastern end of the large canyon Valles Marineris . Various geological processes have reduced it to circular area of chaotic terrain . |