Persbo is an impact crater in the Elysium quadrangle of Mars. It measures 19.5 kilometer in diameter and was named after Persbo, Sweden. It is just south of the Cerberus Fossae, and is adjacent to the Athabasca Valles, which issue from one of the fossae.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.
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| - Cratere Persbo (it)
- Persbo (crater) (en)
- Persbo (cratera) (pt)
- 佩尔斯博陨击坑 (zh)
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| - Persbo è un cratere sulla superficie di Marte. (it)
- A cratera Persbo é uma cratera de impacto no quadrângulo de Elysium em Marte localizada a 8.54° N e 203.24° W. Ela possui 19.5 km em diâmetro e recebeu o nome de uma cidade na Suécia. (pt)
- 佩尔斯博陨击坑(Persbo)是火星埃律西昂区的一座撞击坑,位于科柏洛斯堑沟群南面,并与发源与堑沟群之一的阿萨巴斯卡谷相毗邻。它的中心坐标位于北纬8.54度、西经203.24度处,直径19.5公里,其名称取自瑞典中部达拉纳省卢德维卡市定居区佩尔斯博,2006年被国际天文联合会行星系统命名工作组批准接受。 撞击坑通常有一圈覆盖着喷射物的边缘,相比之下,火山坑则一般没有边缘或喷射沉积物。较大的陨石坑(直径大于10公里或6.2英里)里面常会有一座中央峰,这种中央峰是因撞击后坑底反弹所形成。 (zh)
- Persbo is an impact crater in the Elysium quadrangle of Mars. It measures 19.5 kilometer in diameter and was named after Persbo, Sweden. It is just south of the Cerberus Fossae, and is adjacent to the Athabasca Valles, which issue from one of the fossae.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.
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| - Persbo crater, as seen by CTX camera on MRO (en)
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| - Persbo is an impact crater in the Elysium quadrangle of Mars. It measures 19.5 kilometer in diameter and was named after Persbo, Sweden. It is just south of the Cerberus Fossae, and is adjacent to the Athabasca Valles, which issue from one of the fossae.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.
* Viking Orbiter 1 image with Persbo at top center
* Persbo crater wall, as seen by HiRISE. Scale bar is 500 meters long.
* Persbo crater floor, as seen by HiRISE. Scale bar is 500 meters long. Impacts into floor reached a layer of light-toned materials. These materials were then thrown out over a slightly darker surface. Light-toned materials may be hydrated minerals such as sulfate. (en)
- Persbo è un cratere sulla superficie di Marte. (it)
- A cratera Persbo é uma cratera de impacto no quadrângulo de Elysium em Marte localizada a 8.54° N e 203.24° W. Ela possui 19.5 km em diâmetro e recebeu o nome de uma cidade na Suécia. (pt)
- 佩尔斯博陨击坑(Persbo)是火星埃律西昂区的一座撞击坑,位于科柏洛斯堑沟群南面,并与发源与堑沟群之一的阿萨巴斯卡谷相毗邻。它的中心坐标位于北纬8.54度、西经203.24度处,直径19.5公里,其名称取自瑞典中部达拉纳省卢德维卡市定居区佩尔斯博,2006年被国际天文联合会行星系统命名工作组批准接受。 撞击坑通常有一圈覆盖着喷射物的边缘,相比之下,火山坑则一般没有边缘或喷射沉积物。较大的陨石坑(直径大于10公里或6.2英里)里面常会有一座中央峰,这种中央峰是因撞击后坑底反弹所形成。 (zh)
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