Multi-ringed basin

Valhalla Basin on Jupiter's moon Callisto, taken by Voyager 1

A multi-ringed basin (also a multi-ring impact basin) is not a simple bowl-shaped crater, or a peak ring crater, but one containing multiple concentric topographic rings;[1] a multi-ringed basin could be described as a massive impact crater, surrounded by circular chains of mountains[2] resembling rings on a bull's-eye. A multi-ringed basin may have an area of many thousands of square kilometres.[3]

An impact crater of diameter bigger than about 180 miles (290 km) is referred to as a basin.[4]

  1. ^ Head, J. W. (January 2010). "Transition from complex craters to multi-ringed basins on terrestrial planetary bodies: Scale-dependent role of the expanding melt cavity and progressive interaction with the displaced zone". Geophysical Research Letters. 37 (2). Bibcode:2010GeoRL..37.2203H. doi:10.1029/2009GL041790.
  2. ^ "Lunar Landforms Teacher Page". Hawai'i Space Grant Consortium, Hawai'i Institute of Geophysics and Planetology, University of Hawai'i. 1998. Archived from the original on 12 February 2018. Retrieved 18 January 2019.
  3. ^ "Multiringed basin". Encyclopedia Britannica. February 1, 2018. Retrieved January 20, 2019.
  4. ^ "How Multi-Ring Craters Form Revealed by New Research". Ideas, Inventions And Innovations. October 29, 2016. Archived from the original on 1 July 2017.{{cite web}}: CS1 maint: unfit URL (link)[self-published source?]