Difference between revisions 2117896 and 2117897 on enwikiversity[[Image:Chain of impact craters on Ganymede.jpg|thumb|right|250px|The image shows a chain of craters on Ganymede. Credit: Galileo Project, Brown University, JPL, NASA.]] A '''crater''' may be any large, roughly circular, depression or hole in or beneath the rocky surface of a rocky object. (contracted; show full) Mariner 10 provided the first close-up images of Mercury's surface, which immediately showed its heavily cratered nature At right is an example of catena on Mercury. {{clear}} ==Venus== {{main|Venus}}⏎ [[Image:Mgn p39146.png|thumb|right|250px|Impact craters on the surface of Venus (image reconstructed from radar data) are shown. Credit: NASA.]] The absence of evidence of lava flow accompanying any of the visible caldera remains an enigma. The planet has few impact craters. After the Venera missions were completed, the prime meridian was redefined to pass through the central peak in the crater Ariadne.<ref>{{ cite book |url=http://astrogeology.usgs.gov/Projects/WGCCRE/constants/iau2000_table1.html (contracted; show full)[[Category:Earth sciences/Lectures]] [[Category:Geography/Lectures]] [[Category:Geology/Lectures]] [[Category:Materials sciences/Lectures]] [[Category:Planetary sciences/Lectures]] [[Category:Radiation/Lectures]] [[Category:Radiation astronomy/Lectures]] [[Category:Resources last modified in November 2018]] All content in the above text box is licensed under the Creative Commons Attribution-ShareAlike license Version 4 and was originally sourced from https://en.wikiversity.org/w/index.php?diff=prev&oldid=2117897.
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