Dawes (Martian crater)
Dawes Crater is located in the Sinus Sabaeus quadrangle of Mars , at 9.2 S and 38 E. [1] It is about 191 km (119 mi) in diameter, and was named after William R. Dawes , a British astronomer (1799–1868) [2] who was ahead of his time in believing that Mars only had a thin atmosphere. Dawes presumed that the atmosphere of Mars was thin because surface markings on the planet could easily be seen. [3]
Page Revisions
| Year | Metadata | Sections | Top Words | First Paragraph |
| 2018 |
84099 characters 5 sections 6 paragraphs 5 images 665 internal links 6 external links |
dawes 0.881 furnee 0.182 oenotria 0.121 continent 0.113 strait 0.088 bay 0.087 craters 0.078 sabaea 0.078 mentioned 0.077 proctor 0.075 ocean 0.073 terra 0.072 deepest 0.063 crater 0.061 aryn 0.061 |
Dawes Crater is located in the Sinus Sabaeus quadrangle of Mars , at 9.2 S and 38 E. [1] It is about 191 km (119 mi) in diameter, and was named after William R. Dawes , a British astronomer (1799–1868) [2] who was ahead of his time in believing that Mars only had a thin atmosphere. Dawes presumed that the atmosphere of Mars was thin because surface markings on the planet could easily be seen. [3] |
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| 2017 |
42755 characters 5 sections 6 paragraphs 8 images 174 internal links 6 external links |
dawes 0.881 furnee 0.182 oenotria 0.121 continent 0.113 strait 0.088 bay 0.087 craters 0.078 sabaea 0.078 mentioned 0.077 proctor 0.075 ocean 0.073 terra 0.072 deepest 0.063 crater 0.061 aryn 0.061 |
Dawes Crater is located in the Sinus Sabaeus quadrangle of Mars , at 9.2 S and 38 E. [1] It is about 191 km (119 mi) in diameter, and was named after William R. Dawes , a British astronomer (1799–1868) [2] who was ahead of his time in believing that Mars only had a thin atmosphere. Dawes presumed that the atmosphere of Mars was thin because surface markings on the planet could easily be seen. [3] |
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| 2016 |
39254 characters 3 sections 5 paragraphs 7 images 156 internal links 7 external links |
dawes 0.462 38 0.301 craters 0.269 cracks 0.254 produced 0.148 9 0.146 minerals 0.139 impact 0.137 1799 0.135 00 0.134 1868 0.129 believing 0.118 deposits 0.118 191 0.116 dissolves 0.109 |
Dawes Crater is located in the Sinus Sabaeus quadrangle of Mars , at 9°12′S 38°00′E / 9.2°S 38°E [1] Coordinates : 9°12′S 38°00′E / 9.2°S 38°E [1] . It is about 191 km (119 mi) in diameter, and was named after William R. Dawes , a British astronomer (1799–1868) [2] who was ahead of his time in believing that Mars only had a thin atmosphere. Dawes presumed that the atmosphere of Mars was thin because surface markings on the planet could easily be seen. [3] |
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| 2014 |
42380 characters 3 sections 5 paragraphs 9 images 162 internal links 7 external links |
dawes 0.462 38 0.301 craters 0.269 cracks 0.254 produced 0.148 9 0.146 minerals 0.139 impact 0.137 1799 0.135 00 0.134 1868 0.129 believing 0.118 deposits 0.118 191 0.116 dissolves 0.109 |
Dawes Crater is located in the Sinus Sabaeus quadrangle of Mars , at 9°12′S 38°00′E / 9.2°S 38°E [1] Coordinates : 9°12′S 38°00′E / 9.2°S 38°E [1] . It is about 191 km (119 mi) in diameter, and was named after William R. Dawes , a British astronomer (1799–1868) [2] who was ahead of his time in believing that Mars only had a thin atmosphere. Dawes presumed that the atmosphere of Mars was thin because surface markings on the planet could easily be seen. [3] |
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| 2013 |
33688 characters 1 sections 1 paragraphs 8 images 157 internal links 3 external links |
dawes 0.551 38 0.478 9 0.232 1799 0.214 00 0.213 1868 0.206 believing 0.188 191 0.184 sabaeus 0.170 markings 0.162 119 0.158 presumed 0.138 thin 0.136 ahead 0.113 2 0.107 |
Dawes Crater is located in the Sinus Sabaeus quadrangle of Mars , at 9°12′S 38°00′E / 9.2°S 38°E [1] Coordinates : 9°12′S 38°00′E / 9.2°S 38°E [1] . It is about 191 km (119 mi) in diameter, and was named after William R. Dawes , a British astronomer (1799–1868) [2] who was ahead of his time in believing that Mars only had a thin atmosphere. Dawes presumed that the atmosphere of Mars was thin because surface markings on the planet could easily be seen. [3] |
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| 2011 |
12389 characters 1 sections 2 paragraphs 4 images 13 internal links 3 external links |
dawes 0.551 38 0.478 9 0.232 1799 0.214 00 0.213 1868 0.206 believing 0.188 191 0.184 sabaeus 0.170 markings 0.162 119 0.158 presumed 0.138 thin 0.136 ahead 0.113 2 0.107 |
Dawes Crater is located in the Sinus Sabaeus quadrangle of Mars , at 9°12′S 38°00′E / 9.2°S 38°E [1] Coordinates : 9°12′S 38°00′E / 9.2°S 38°E [1] . It is about 191 km (119 mi) in diameter, and was named after William R. Dawes , a British astronomer (1799–1868) [2] who was ahead of his time in believing that Mars only had a thin atmosphere. Dawes presumed that the atmosphere of Mars was thin because surface markings on the planet could easily be seen. [3] |
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| 2010 |
12387 characters 1 sections 1 paragraphs 4 images 13 internal links 3 external links |
dawes 0.549 38 0.477 9 0.231 1799 0.213 00 0.213 1868 0.205 believing 0.187 191 0.183 sabaeus 0.169 markings 0.161 119 0.157 presumed 0.138 thin 0.135 ahead 0.113 2 0.107 |
Dawes Crater is located in the Sinus Sabaeus quadrangle of Mars , at 9°12′S 38°00′E / 9.2°S 38°E [1] Coordinates : 9°12′S 38°00′E / 9.2°S 38°E [1] . It is about 191 km (119 mi) in diameter, and was named after William R. Dawes , a British astronomer (1799–1868) [2] who was ahead of his time in believing that Mars only had a thin atmosphere. Dawes presumed that the atmosphere of Mars was thin due to the fact that surface markings on the planet could easily be seen. [3] |
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| 2009 |
9698 characters 1 sections 2 paragraphs 4 images 8 internal links 1 external links |
dawes 0.566 reverend 0.493 322 0.231 clarity 0.220 1799 0.220 1868 0.211 believing 0.193 191 0.189 sabaeus 0.174 markings 0.166 presumed 0.142 ahead 0.116 observe 0.116 sinus 0.107 british 0.105 |
Dawes Crater is a crater in the Sinus Sabaeus quadrangle of Mars at 9.3° south latitude and 322° west longitude. It is about 191 km in diameter and was named after Reverend William R. Dawes , a British astronomer (1799-1868). [1] Reverend Dawes was ahead of his time in believing that Mars only had a thin atmosphere. He presumed that this was because of the clarity with which one could observe the surface markings on the planet. [2] |