Hale (Martian crater)
Hale is a 150 km × 125 km (93 mi × 78 mi) crater at 35.7°S, 323.4°E on Mars , just north of Argyre basin . The crater is in the Argyre quadrangle .
Page Revisions
| Year | Metadata | Sections | Top Words | First Paragraph |
| 2018 |
83429 characters 4 sections 9 paragraphs 6 images 657 internal links 8 external links |
hale 0.631 gullies 0.220 wall 0.167 aquifer 0.167 aquifers 0.166 crater 0.130 water 0.128 pits 0.124 perchlorate 0.120 flow 0.109 alcove 0.109 ellery 0.108 moanda 0.108 ejecta 0.101 argyre 0.099 |
Hale is a 150 km × 125 km (93 mi × 78 mi) crater at 35.7°S, 323.4°E on Mars , just north of Argyre basin . The crater is in the Argyre quadrangle . |
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| 2017 |
41779 characters 4 sections 9 paragraphs 9 images 164 internal links 8 external links |
hale 0.631 gullies 0.220 wall 0.167 aquifer 0.167 aquifers 0.166 crater 0.130 water 0.128 pits 0.124 perchlorate 0.120 flow 0.109 alcove 0.109 ellery 0.108 moanda 0.108 ejecta 0.101 argyre 0.099 |
Hale is a 150 km × 125 km (93 mi × 78 mi) crater at 35.7°S, 323.4°E on Mars , just north of Argyre basin . The crater is in the Argyre quadrangle . |
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| 2016 |
36454 characters 3 sections 9 paragraphs 5 images 160 internal links 5 external links |
hale 0.542 gullies 0.248 water 0.185 aquifer 0.162 aquifers 0.160 ice 0.158 mantle 0.135 flow 0.132 wall 0.129 pits 0.120 perchlorate 0.116 alcove 0.105 ellery 0.104 young 0.098 ejecta 0.098 |
Hale is a 150 km × 125 km (93 mi × 78 mi) crater at 35.7°S, 323.4°E on Mars , just north of Argyre basin . The crater is in the Argyre quadrangle . On 28 September 2015 NASA confirmed the seasonal existence of liquid water in Hale crater. [1] The salts in the water ( magnesium perchlorate , magnesium chlorate , sodium perchlorate ,...) lower its freezing and melting point to 203 K (−70 °C or −94 °F), which is near the average summer night temperature. Hale was created by an asteroid roughly 35 km (22 mi) across that impacted at an oblique angle about 3.5–3.8 billion years ago. The rim and ejecta are eroded and show smaller impacts, but subsequent deposits have covered up small craters within it. [2] On the southern rim of Hale, parts of the crater wall have moved downslope towards the crater's centre. The surface shows a network of fluvial channels which may have been caused by running water. [3] |
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| 2015 |
36541 characters 3 sections 9 paragraphs 5 images 161 internal links 5 external links |
hale 0.541 gullies 0.248 water 0.185 aquifer 0.161 aquifers 0.160 ice 0.158 mantle 0.135 flow 0.132 wall 0.129 pits 0.119 perchlorate 0.116 alcove 0.105 ellery 0.104 young 0.097 ejecta 0.097 |
Hale is a 150 km × 125 km (93 mi × 78 mi) crater at 35.7°S, 323.4°E on Mars , just north of Argyre basin . The crater is in the Argyre quadrangle . On 2015 September 28th NASA confirmed the seasonal existence of liquid water in Hale crater. [1] The salts in the water ( magnesium perchlorate , magnesium chlorate , sodium perchlorate ,...) lower its freezing and melting point to 203 K (−70 °C or −94 °F), which is near the average summer night temperature. Hale was created by an asteroid roughly 35 km (22 mi) across that impacted at an oblique angle about 3.5–3.8 billion years ago. The rim and ejecta are eroded and show smaller impacts, but subsequent deposits have covered up small craters within it. [2] On the southern rim of Hale, parts of the crater wall have moved downslope towards the crater's centre. The surface shows a network of fluvial channels which may have been caused by running water. [3] |
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| 2014 |
34087 characters 2 sections 8 paragraphs 5 images 155 internal links 4 external links |
hale 0.456 gullies 0.278 aquifer 0.181 water 0.180 aquifers 0.179 ice 0.178 mantle 0.151 flow 0.148 wall 0.145 pits 0.134 alcove 0.118 ellery 0.117 young 0.109 ejecta 0.109 layer 0.108 |
Hale is a 150 by 125 km (93 by 78 mi) crater at 35.7°S, 323.4°E on Mars , just north of Argyre basin . The crater is in the Argyre quadrangle . It was created by an asteroid roughly 35 km (22 mi) across that impacted at an oblique angle about 3.5 to 3.8 billion years ago. The rim and ejecta are eroded and show smaller impacts, but subsequent deposits have covered up small craters within it. [1] On the southern rim of Hale, parts of the crater wall have moved downslope towards the crater’s centre. The surface shows a network of fluvial channels which may have been caused by running water. [2] |
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| 2013 |
34295 characters 2 sections 8 paragraphs 5 images 156 internal links 4 external links |
hale 0.456 gullies 0.278 aquifer 0.181 water 0.180 aquifers 0.179 ice 0.178 mantle 0.151 flow 0.148 wall 0.145 pits 0.134 alcove 0.118 ellery 0.117 young 0.109 ejecta 0.109 layer 0.108 |
Hale is a 150 by 125 km (93 by 78 mi) crater at 35.7°S, 323.4°E on Mars , just north of Argyre basin . The crater is in the Argyre quadrangle . It was created by an asteroid roughly 35 km (22 mi) across that impacted at an oblique angle about 3.5 to 3.8 billion years ago. The rim and ejecta are eroded and show smaller impacts, but subsequent deposits have covered up small craters within it. [1] On the southern rim of Hale, parts of the crater wall have moved downslope towards the crater’s centre. The surface shows a network of fluvial channels which may have been caused by running water. [2] |
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| 2012 |
12985 characters 2 sections 8 paragraphs 1 images 12 internal links 4 external links |
hale 0.456 gullies 0.278 aquifer 0.181 water 0.180 aquifers 0.179 ice 0.178 mantle 0.151 flow 0.148 wall 0.145 pits 0.134 alcove 0.118 ellery 0.117 young 0.109 ejecta 0.109 layer 0.108 |
Hale is a 150 by 125 km (93 by 78 mi) crater at 35.7°S, 323.4°E on Mars , just north of Argyre basin . The crater is in the Argyre quadrangle . It was created by an asteroid roughly 35 km (22 mi) across that impacted at an oblique angle about 3.5 to 3.8 billion years ago. The rim and ejecta are eroded and show smaller impacts, but subsequent deposits have covered up small craters within it. [1] On the southern rim of Hale, parts of the crater wall have moved downslope towards the crater’s centre. The surface shows a network of fluvial channels which may have been caused by running water. [2] |
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| 2011 |
12198 characters 2 sections 8 paragraphs 1 images 11 internal links 4 external links |
hale 0.412 gullies 0.302 aquifer 0.197 water 0.195 aquifers 0.195 ice 0.171 mantle 0.164 flow 0.160 wall 0.157 alcove 0.128 ellery 0.127 young 0.119 layer 0.117 gully 0.114 leaves 0.101 |
Hale is a 150 by 125 km (93 by 78 mi) crater at 35.7°S, 323.4°E on Mars , just north of Argyre basin . It was created by an asteroid roughly 35 km (22 mi) across that impacted at an oblique angle about 3.5 to 3.8 billion years ago. The rim and ejecta are eroded and show smaller impacts, but subsequent deposits have covered up small craters within it. [1] On the southern rim of Hale, parts of the crater wall have moved downslope towards the crater’s centre. The surface shows a network of fluvial channels which may have been caused by running water. [2] |
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| 2010 |
13012 characters 2 sections 9 paragraphs 1 images 12 internal links 5 external links |
hale 0.383 323 0.352 gullies 0.281 aquifer 0.182 water 0.181 aquifers 0.181 35 0.166 ice 0.159 mantle 0.152 flow 0.149 wall 0.146 alcove 0.119 ellery 0.118 young 0.110 layer 0.109 |
Hale is a 150 by 125 km crater at 35.7°S, 323.4°E on Mars , just north of Argyre basin . It was created by an asteroid roughly 35 km across that impacted at an oblique angle about 3.5 to 3.8 billion years ago. The rim and ejecta are eroded and show smaller impacts, but subsequent deposits have covered up small craters within it. [1] On the southern rim of Hale, parts of the crater wall have moved downslope towards the crater’s centre. The surface shows a network of fluvial channels which may have been caused by running water. [2] |
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| 2009 |
12965 characters 2 sections 9 paragraphs 1 images 12 internal links 5 external links |
hale 0.383 323 0.352 gullies 0.281 aquifer 0.182 water 0.181 aquifers 0.181 35 0.166 ice 0.159 mantle 0.152 flow 0.149 wall 0.146 alcove 0.119 ellery 0.118 young 0.110 layer 0.109 |
Hale is a 150 by 125 km crater at 35.7°S, 323.4°E on Mars , just north of Argyre basin . It was created by an asteroid roughly 35 km across that impacted at an oblique angle about 3.5 to 3.8 billion years ago. The rim and ejecta are eroded and show smaller impacts, but subsequent deposits have covered up small craters within it. [1] On the southern rim of Hale, parts of the crater wall have moved downslope towards the crater’s centre. The surface shows a network of fluvial channels which may have been caused by running water. [2] |
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| 2008 |
8520 characters 2 sections 3 paragraphs 1 images 12 internal links 3 external links |
hale 0.613 ellery 0.314 323 0.235 oblique 0.198 35 0.177 downslope 0.176 fluvial 0.168 125 0.164 impacted 0.151 rim 0.150 argyre 0.144 george 0.139 centre 0.135 running 0.109 moved 0.107 |
Hale is a 150 by 125 km crater at 35.7°S, 323.4°E on Mars , just north of Argyre basin . It was created by an asteroid roughly 35 km across that impacted at an oblique angle about 3.5 to 3.8 billion years ago. The rim and ejecta are eroded and show smaller impacts, but subsequent deposits have covered up small craters within it. [1] On the southern rim of Hale, parts of the crater wall have moved downslope towards the crater’s centre. The surface shows a network of fluvial channels which may have been caused by running water. [2] |
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| 2007 |
8518 characters 2 sections 2 paragraphs 1 images 12 internal links 3 external links |
hale 0.613 ellery 0.314 323 0.235 oblique 0.198 35 0.177 downslope 0.176 fluvial 0.168 125 0.164 impacted 0.151 rim 0.150 argyre 0.144 george 0.139 centre 0.135 running 0.109 moved 0.107 |
Hale is a 150 by 125 km crater at 35.7°S, 323.4°E on Mars , just north of Argyre basin . It was created by an asteroid roughly 35 km across that impacted at an oblique angle about 3.5 to 3.8 billion years ago. The rim and ejecta are eroded and show smaller impacts, but subsequent deposits have covered up small craters within it. [1] On the southern rim of Hale, parts of the crater wall have moved downslope towards the crater’s centre. The surface shows a network of fluvial channels which may have been caused by running water. [2] |