File:Proctor Crater Dune Field.jpg
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描述Proctor Crater Dune Field.jpg |
English: This observation shows the edge of a dark dune field on the floor of Proctor Crater, a 150-kilometre diameter crater in the Southern highlands of Mars.
The dark dunes are composed of basaltic sand that has collected on the bottom of the crater. Dark dune slip faces (the steeper sides of the dunes) are located on the east side of the dunes and are believed to have formed in response to fall and winter westerly winds caused by geostrophic forces (winds balanced by Coriolis and pressure gradient forces). Superimposed on their surface are smaller secondary dunes that are commonly seen on terrestrial dunes of this size. Many smaller and brighter bed forms, most likely small dunes or granule ripples, cover the substrate between the larger dark dunes as well as most of the floor of Proctor Crater. The dark dunes overlie the small bright bed-forms indicating that they formed more recently. In several areas, however, the dark dunes appear to influence the orientation of the small bright dunes, possibly by wind flowing around the larger ones, suggesting that both dark and bright bed-forms are coeval. The dunes in Proctor Crater may be active today, moving in response to Martian winds.Русский: Oгромные песчаные дюны на дне марсианского кратера Проктор. Фотография была получена с помощью камеры HiRISE, установленной на борту спутника Марс Реконесанс Орбитер (Mars Reconnaissance Orbiter, MRO) — роботизированного космического аппарата, летающего по орбите вокруг Марса. Тёмные волнообразные дюны, скорее всего, сформировались позже, чем более светлые камни под ними. Считается, что они медленно смещаются под действием вездесущих ветров.
Дюны возникают вследствие сложного взаимодействия песчаной марсианской поверхности и сильных ветров. Подобные образования были замечены в кратере Проктор космическим аппаратом Маринер-9 более 35 лет назад. |
日期 | |
来源 | HiRISE |
作者 | NASA/JPL/University of Arizona |
Local Mars time: 3:30 PM. Latitude (centered): -47.0 °. Longitude (East): 30.7 °. Range to target site: 281.8 km. Original image scale range: 28.2 cm/pixel (with 1 x 1 binning) so objects ~85 cm across are resolved. Map projected scale: 25 cm/pixel and north is up. Map projection: EQUIRECTANGULAR. Emission angle: 27.7 °. Phase angle: 22.7 °. Solar incidence angle: 47 °, with the Sun about 43 ° above the horizon. Solar longitude: 254.6 °, Northern Autumn.
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当前 | 2010年11月22日 (一) 12:58 | 2,560 × 1,920(4.34 MB) | Originalwana(留言 | 贡献) | {{Information |Description={{en|1=This observation shows the edge of a dark dune field on the floor of Proctor Crater, a 150-kilometre diameter crater in the Southern highlands of Mars. The dark dunes are composed of basaltic sand that has collected |
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水平分辨率 | 72 dpi |
垂直分辨率 | 72 dpi |
使用软件 | Adobe Photoshop CS5 Macintosh |
文件修改日期时间 | 2010年10月26日 (二) 15:19 |
色彩空间 | sRGB |