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- Burton is an impact crater in the Memnonia quadrangle of Mars. It is 123.0 km in diameter and was named after British astronomer Charles E. Burton; the name was approved in 1973. It has a central peak. 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. Cobres crater is northeast of Burton, and Marca crater is to the northwest. Mangala Valles is to the east. In December 2021, three craters immediately south of Burton were named. These are Karratha, Khujirt, and Dampier. Karratha is within Dampier.
* Middle section of Burton crater, as seen by CTX camera (on MRO)
* Central peaks of Burton crater, showing dark slope streaks. Note: this is an enlargement of the previous image.
* Topographic map showing the central peak
* Mosaic of Viking Orbiter 1 images, acquired near the end of the Viking mission in 1980 (en)
- Burton è un cratere sulla superficie di Marte. (it)
- Burton é uma cratera marciana. Tem como característica 123 quilômetros de diâmetro. O seu nome é em homenagem a , um astrónomo britânico. (pt)
- 伯顿陨击坑（Burton）是火星门农尼亚区的一座撞击坑，中心坐标位于南纬13.9度、西经156.3度，直径123公里（76.6英里），其名称取自英国天文学家查尔斯·爱德华·伯顿（1846年-1882年），1973年，被国际天文联合会批准采用。 伯顿陨击坑西北和东北分别坐落了较小的马尔卡陨击坑和科夫雷斯陨击坑，而它的东面则分布着曼加拉谷。伯顿陨击坑内矗立有一座中央峰。撞击坑通常有一圈周围分布着喷射物的边缘，相比之下，火山口通常则没有边缘或喷射沉积物。越大的陨坑（直径大于10公里）通常会有一座中心峰，这种中央峰是因撞击后坑底反弹所形成。 2021年12月，伯顿陨击坑南面的三座陨坑：卡拉萨、呼吉尔特和丹皮尔被予以命名，而卡拉萨则位于丹皮尔陨击坑内。
* 显示有暗坡条纹的伯顿陨击坑中央山峰，注：这是前一幅图像的放大版。
* 显示了中央峰的地形图。
* 1980年，海盗1号轨道器在任务接近尾声时拍摄的拼接图。 (zh)
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- 4801 (xsd:nonNegativeInteger)
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- Viking Orbiter 1 image with Burton at the bottom (en)
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- Burton è un cratere sulla superficie di Marte. (it)
- Burton é uma cratera marciana. Tem como característica 123 quilômetros de diâmetro. O seu nome é em homenagem a , um astrónomo britânico. (pt)
- 伯顿陨击坑（Burton）是火星门农尼亚区的一座撞击坑，中心坐标位于南纬13.9度、西经156.3度，直径123公里（76.6英里），其名称取自英国天文学家查尔斯·爱德华·伯顿（1846年-1882年），1973年，被国际天文联合会批准采用。 伯顿陨击坑西北和东北分别坐落了较小的马尔卡陨击坑和科夫雷斯陨击坑，而它的东面则分布着曼加拉谷。伯顿陨击坑内矗立有一座中央峰。撞击坑通常有一圈周围分布着喷射物的边缘，相比之下，火山口通常则没有边缘或喷射沉积物。越大的陨坑（直径大于10公里）通常会有一座中心峰，这种中央峰是因撞击后坑底反弹所形成。 2021年12月，伯顿陨击坑南面的三座陨坑：卡拉萨、呼吉尔特和丹皮尔被予以命名，而卡拉萨则位于丹皮尔陨击坑内。
* 显示有暗坡条纹的伯顿陨击坑中央山峰，注：这是前一幅图像的放大版。
* 显示了中央峰的地形图。
* 1980年，海盗1号轨道器在任务接近尾声时拍摄的拼接图。 (zh)
- Burton is an impact crater in the Memnonia quadrangle of Mars. It is 123.0 km in diameter and was named after British astronomer Charles E. Burton; the name was approved in 1973. It has a central peak. 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.
* Middle section of Burton crater, as seen by CTX camera (on MRO)
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* (en)
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- Burton (crater) (en)
- Cratere Burton (it)
- Burton (cratera) (pt)
- 伯顿陨击坑 (zh)
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- POINT(-156.30000305176 -13.89999961853)
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