Radau is an impact crater in the Oxia Palus quadrangle of Mars , located 17.1° N and 4.8° W. It measures 114.5 kilometers in diameter and was named for Rodolphe Radau , a French astronomer (1835–1911). [1] Impact craters generally have a rim with ejecta around them, in contrast volcanic craters usually do not have a rim or ejecta deposits. As craters get larger (greater than 10 km in diameter) they usually have a central peak. [2] The peak is caused by a rebound of the crater floor following the impact. [3]
Year | Metadata | Sections | Top Words | First Paragraph |
2018 |
77317 characters 2 sections 4 paragraphs 6 images 657 internal links 4 external links |
radau 0.750 rodolphe 0.239 1835 0.198 114 0.176 1911 0.169 ejecta 0.166 peak 0.151 ctx 0.145 craters 0.128 rim 0.126 oxia 0.118 rebound 0.117 reconnaissance 0.112 crater 0.107 camera 0.105 |
Radau is an impact crater in the Oxia Palus quadrangle of Mars , located 17.1° N and 4.8° W. It measures 114.5 kilometers in diameter and was named for Rodolphe Radau , a French astronomer (1835–1911). [1] Impact craters generally have a rim with ejecta around them, in contrast volcanic craters usually do not have a rim or ejecta deposits. As craters get larger (greater than 10 km in diameter) they usually have a central peak. [2] The peak is caused by a rebound of the crater floor following the impact. [3] |
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2017 |
35931 characters 2 sections 4 paragraphs 9 images 163 internal links 4 external links |
radau 0.750 rodolphe 0.239 1835 0.198 114 0.176 1911 0.169 ejecta 0.166 peak 0.151 ctx 0.145 craters 0.128 rim 0.126 oxia 0.118 rebound 0.117 reconnaissance 0.112 crater 0.107 camera 0.105 |
Radau is an impact crater in the Oxia Palus quadrangle of Mars , located 17.1° N and 4.8° W. It measures 114.5 kilometers in diameter and was named for Rodolphe Radau , a French astronomer (1835–1911). [1] Impact craters generally have a rim with ejecta around them, in contrast volcanic craters usually do not have a rim or ejecta deposits. As craters get larger (greater than 10 km in diameter) they usually have a central peak. [2] The peak is caused by a rebound of the crater floor following the impact. [3] |
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2016 |
35452 characters 3 sections 6 paragraphs 9 images 158 internal links 4 external links |
radau 0.615 craters 0.245 rodolphe 0.196 1835 0.162 deposits 0.153 impact 0.153 114 0.144 dissolves 0.141 ores 0.139 1911 0.139 ejecta 0.136 crater 0.131 melts 0.127 ore 0.126 peak 0.124 |
Radau Crater is an impact crater in the Oxia Palus quadrangle of Mars , located 17.1° N and 4.8° W. It is 114.5 km in diameter and was named for Rodolphe Radau, a French astronomer (1835–1911). [1] Impact craters generally have a rim with ejecta around them, in contrast volcanic craters usually do not have a rim or ejecta deposits. As craters get larger (greater than 10 km in diameter) they usually have a central peak. [2] The peak is caused by a rebound of the crater floor following the impact. [3] |
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2015 |
35449 characters 3 sections 6 paragraphs 9 images 158 internal links 4 external links |
radau 0.615 craters 0.245 rodolphe 0.196 1835 0.162 deposits 0.153 impact 0.153 114 0.144 dissolves 0.141 ores 0.139 1911 0.139 ejecta 0.136 crater 0.131 melts 0.127 ore 0.126 peak 0.124 |
Radau Crater is an impact crater in the Oxia Palus quadrangle of Mars , located 17.1° N and 4.8° W. It is 114.5 km in diameter and was named for Rodolphe Radau, a French astronomer (1835–1911). [1] Impact craters generally have a rim with ejecta around them, in contrast volcanic craters usually do not have a rim or ejecta deposits. As craters get larger (greater than 10 km in diameter) they usually have a central peak. [2] The peak is caused by a rebound of the crater floor following the impact. [3] |
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2014 |
34935 characters 3 sections 5 paragraphs 9 images 158 internal links 4 external links |
radau 0.615 craters 0.245 rodolphe 0.196 1835 0.162 deposits 0.153 impact 0.153 114 0.144 dissolves 0.141 ores 0.139 1911 0.139 ejecta 0.136 crater 0.131 melts 0.127 ore 0.126 peak 0.124 |
Radau Crater is an impact crater in the Oxia Palus quadrangle of Mars , located 17.1° N and 4.8° W. It is 114.5 km in diameter and was named for Rodolphe Radau, a French astronomer (1835–1911). [1] Impact craters generally have a rim with ejecta around them, in contrast volcanic craters usually do not have a rim or ejecta deposits. As craters get larger (greater than 10 km in diameter) they usually have a central peak. [2] The peak is caused by a rebound of the crater floor following the impact. [3] |
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2013 |
27459 characters 1 sections 1 paragraphs 7 images 154 internal links 1 external links |
radau 0.635 rodolphe 0.405 1835 0.336 114 0.298 1911 0.287 oxia 0.200 french 0.165 palus 0.157 astronomer 0.120 17 0.110 crater 0.090 8 0.064 quadrangle 0.055 impact 0.053 diameter 0.051 |
Radau Crater is an impact crater in the Oxia Palus quadrangle of Mars , located 17.1° N and 4.8° W. It is 114.5 km in diameter and was named for Rodolphe Radau, a French astronomer (1835–1911). [1] |
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2011 |
6169 characters 1 sections 2 paragraphs 3 images 10 internal links 1 external links |
radau 0.635 rodolphe 0.405 1835 0.336 114 0.298 1911 0.287 oxia 0.200 french 0.165 palus 0.157 astronomer 0.120 17 0.110 crater 0.090 8 0.064 quadrangle 0.055 impact 0.053 diameter 0.051 |
Radau Crater is an impact crater in the Oxia Palus quadrangle of Mars , located 17.1° N and 4.8° W. It is 114.5 km in diameter and was named for Rodolphe Radau, a French astronomer (1835–1911). [1] |
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2009 |
5869 characters 1 sections 3 paragraphs 3 images 9 internal links 1 external links |
radau 0.766 rodolphe 0.326 1835 0.270 114 0.239 1911 0.230 oxia 0.161 french 0.133 palus 0.126 crater 0.109 peak 0.103 astronomer 0.096 17 0.088 central 0.083 hirise 0.073 8 0.052 |
Radau Crater is an impact crater in the Oxia Palus quadrangle of Mars , located 17.1° N and 4.8° W. It is 114.5 km in diameter and was named for Rodolphe Radau, a French astronomer (1835-1911). [1] |