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Gledhill is an impact crater in the Hellas quadrangle of Mars, located at 53.2°S latitude and 87.1°E longitude. It is 78.5 km in diameter. It was named after British astronomer Joseph Gledhill, and the name was approved in 1973 by the International Astronomical Union (IAU) Working Group for Planetary System Nomenclature (WGPSN).

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  • Gledhill (crater) (en)
  • Cratere Gledhill (it)
  • 格莱德希尔陨击坑 (zh)
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  • Gledhill è un cratere sulla superficie di Marte. (it)
  • 格莱德希尔陨击坑（Gledhill）是火星希腊区的一座撞击坑，中心坐标位于南纬53.2度、东经87.1度处，直径约78.5公里，其名称取自英国天文学家约瑟夫·格莱德希尔（1837年-1906年），1973年被国际天文联合会正式批准接受。 撞击坑通常有一圈边缘，周围覆盖着喷射物，相比之下，火山坑则一般没有边缘或喷射沉积物。随着陨石坑的增大（直径大于10公里），它们常会有一座中央峰，这种中央峰是因撞击后坑底反弹所形成。在本页图像中格莱德希尔陨击坑显示有一座中央峰。 (zh)
  • Gledhill is an impact crater in the Hellas quadrangle of Mars, located at 53.2°S latitude and 87.1°E longitude. It is 78.5 km in diameter. It was named after British astronomer Joseph Gledhill, and the name was approved in 1973 by the International Astronomical Union (IAU) Working Group for Planetary System Nomenclature (WGPSN). (en)
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  • http://commons.wikimedia.org/wiki/Special:FilePath/Wikigledhill.jpg
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  • Gledhill Crater, as seen by CTX camera . (en)
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  • Gledhill Crater (en)
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  • #FA8072 (en)
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  • -53.2 87.1
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  • Gledhill is an impact crater in the Hellas quadrangle of Mars, located at 53.2°S latitude and 87.1°E longitude. It is 78.5 km in diameter. It was named after British astronomer Joseph Gledhill, and the name was approved in 1973 by the International Astronomical Union (IAU) Working Group for Planetary System Nomenclature (WGPSN). 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. The peak is caused by a rebound of the crater floor following the impact. Gledhill Crater shows a central peak in a picture on this page. (en)
  • Gledhill è un cratere sulla superficie di Marte. (it)
  • 格莱德希尔陨击坑（Gledhill）是火星希腊区的一座撞击坑，中心坐标位于南纬53.2度、东经87.1度处，直径约78.5公里，其名称取自英国天文学家约瑟夫·格莱德希尔（1837年-1906年），1973年被国际天文联合会正式批准接受。 撞击坑通常有一圈边缘，周围覆盖着喷射物，相比之下，火山坑则一般没有边缘或喷射沉积物。随着陨石坑的增大（直径大于10公里），它们常会有一座中央峰，这种中央峰是因撞击后坑底反弹所形成。在本页图像中格莱德希尔陨击坑显示有一座中央峰。 (zh)
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  • Mars (en)
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  • POINT(87.099998474121 -53.200000762939)
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