Puńsk is an impact crater on Mars, located in the Oxia Palus quadrangle at 20.8° N and 41.2° W. It measures 11.6 kilometers in diameter and was named after the village of Puńsk in Poland. 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.(Main article: Rampart crater)
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| - Cratere Púnsk (it)
- Puńsk (crater) (en)
- Puńsk (krater marsjański) (pl)
- Punsk (cratera) (pt)
- 蓬斯克陨击坑 (zh)
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| - Puńsk – krater na powierzchni Marsa o średnicy 11,6 km, położony na 20,8° szerokości i 41,2° długości zachodniej. Decyzją Międzynarodowej Unii Astronomicznej w 1976 roku został nazwany od polskiej miejscowości Puńsk. (pl)
- A cratera Punsk é uma cratera no quadrângulo de Oxia Palus em Marte. Ela está localizada a20.8º latitude norte e 41.2º longitude oeste, medindo 11.6 km de diâmetro. Seu nome vem da cidade de Puńsk, na Polônia, tendo sido aprovado em 1976. (pt)
- 蓬斯克陨击坑（Puńsk）是火星欧克西亚沼区的一座撞击坑，其中心坐标位于北纬20.8度、西经41.2度处，直径11.6公里。该特征取名自波兰纽约州波德拉谢省蓬斯克村，1976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。 普斯克陨击坑属于单层喷射物类型中被称为“的陨坑。单层喷射坑是壁垒型坑中的一种。它们有一层从坑口边缘一直延伸至1到1.5倍陨坑半径处的喷射物堆，平均直径10公里。虽然这类陨坑广泛分布于所有纬度区，但它们最常见于赤道附近。离赤道越远，平均尺寸越大。有人认为，这类陨坑是由于撞击到冰冷的地面而形成。具体来说，这是一种不完全穿透冰层的撞击。远离赤道的冰层厚度可能更大，这也解释了距赤道越远的陨坑尺寸增大的原因。 (zh)
- Puńsk is an impact crater on Mars, located in the Oxia Palus quadrangle at 20.8° N and 41.2° W. It measures 11.6 kilometers in diameter and was named after the village of Puńsk in Poland. 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.(Main article: Rampart crater)
* (en)
- Púnsk è un cratere sulla superficie di Marte.Il Cratere Púnsk è un cratere meteoritico nel quadrilatero Oxia Palus di Marte, che si trova a 20,8° N e 41° W. Ha un diametro di 11,6 km e deve il suo nome a Puńsk, Polonia. I crateri da impatto in genere hanno un bordo con materiale espulso intorno a loro, invece i crateri vulcanici di solito non hanno un orlo o prodotti di depositi piroclastici. Sono crateri più grandi (maggiori di 10 km di diametro) che di solito hanno un picco centrale.Il picco è causato da un rimbalzo del cratere a seguito dell'impatto. (it)
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| - Puńsk crater, as seen by CTX camera on MRO. (en)
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| - Puńsk is an impact crater on Mars, located in the Oxia Palus quadrangle at 20.8° N and 41.2° W. It measures 11.6 kilometers in diameter and was named after the village of Puńsk in Poland. 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. Puńsk crater belongs to the class of craters called "Rampart craters" of the single-ejecta variety. Single-layered ejecta craters are one type of rampart crater. They have one ejecta lobe that extends 1 to 1.5 crater radii from the rim of the crater. They have an average diameter of 10 km. Although present at all latitudes, they are most common near the equator. Their average size increases the more distant from the equator. It has been suggested that these types of craters are produced by impact into icy ground. Specifically, it is an impact that does not go entirely through the icy layer. The increase in size away from the equator is explained by a possible greater thickness in the icy layer away from the equator.(Main article: Rampart crater)
* Puńsk crater, as seen by HiRISE. Scale bar is 500 meters long. Image on right is an enlargement of south (bottom) wall of crater. (en)
- Púnsk è un cratere sulla superficie di Marte.Il Cratere Púnsk è un cratere meteoritico nel quadrilatero Oxia Palus di Marte, che si trova a 20,8° N e 41° W. Ha un diametro di 11,6 km e deve il suo nome a Puńsk, Polonia. I crateri da impatto in genere hanno un bordo con materiale espulso intorno a loro, invece i crateri vulcanici di solito non hanno un orlo o prodotti di depositi piroclastici. Sono crateri più grandi (maggiori di 10 km di diametro) che di solito hanno un picco centrale.Il picco è causato da un rimbalzo del cratere a seguito dell'impatto. Il cratere Punsk, visualizzato dalla Fotocamera CTX (it)
- Puńsk – krater na powierzchni Marsa o średnicy 11,6 km, położony na 20,8° szerokości i 41,2° długości zachodniej. Decyzją Międzynarodowej Unii Astronomicznej w 1976 roku został nazwany od polskiej miejscowości Puńsk. (pl)
- A cratera Punsk é uma cratera no quadrângulo de Oxia Palus em Marte. Ela está localizada a20.8º latitude norte e 41.2º longitude oeste, medindo 11.6 km de diâmetro. Seu nome vem da cidade de Puńsk, na Polônia, tendo sido aprovado em 1976. (pt)
- 蓬斯克陨击坑（Puńsk）是火星欧克西亚沼区的一座撞击坑，其中心坐标位于北纬20.8度、西经41.2度处，直径11.6公里。该特征取名自波兰纽约州波德拉谢省蓬斯克村，1976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。 普斯克陨击坑属于单层喷射物类型中被称为“的陨坑。单层喷射坑是壁垒型坑中的一种。它们有一层从坑口边缘一直延伸至1到1.5倍陨坑半径处的喷射物堆，平均直径10公里。虽然这类陨坑广泛分布于所有纬度区，但它们最常见于赤道附近。离赤道越远，平均尺寸越大。有人认为，这类陨坑是由于撞击到冰冷的地面而形成。具体来说，这是一种不完全穿透冰层的撞击。远离赤道的冰层厚度可能更大，这也解释了距赤道越远的陨坑尺寸增大的原因。 (zh)
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