Impact gardening is the process by which impact events stir the outermost crusts of moons and other celestial objects with no atmospheres. In the particular case of the Moon, this is more often known as lunar gardening. Planetary bodies lacking an atmosphere will generally also lack any erosional processes, with the possible exception of volcanism, and as a result impact debris accumulates at the object's surface as a rough "soil," commonly referred to as regolith. Subsequent impacts, especially by micrometeorites, stir and mix this soil. It had long been estimated that the top centimeter of the lunar surface is overturned every 10 million years.[1] However, a 2016 analysis by the LRO satellite of impact ejecta coverage puts the figure closer to 80,000 years.[2]
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References
- ^ Cole, George H. A.; Woolfson, Michael Mark (2002). Planetary Science: The Science of Planets Around Stars. CRC Press. p. 96.
- ^ Speyerer, Emerson J.; Povilaitis, Reinhold Z.; Robinson, Mark S.; Thomas, Peter C.; Wagner, Robert V. (13 October 2016). "Quantifying crater production and regolith overturn on the Moon with temporal imaging". Nature. 538 (7624): 215–218. Bibcode:2016Natur.538..215S. doi:10.1038/nature19829. PMID 27734864. S2CID 4443574.
Further reading
- Hartmann, William K.; Anguita, Jorge; de la Casa, Miguel A.; et al. (2001). "Martian Cratering 7: The role of Impact Gardening". Icarus. 149 (1): 37–51. Bibcode:2001Icar..149...37H. doi:10.1006/icar.2000.6532.
- Housen, Kevin R.; Wilkening, Laurel L.; Chapman, Clark R.; et al. (1979). "Asteroidal Regoliths". Icarus. 39 (3): 317–351. Bibcode:1979Icar...39..317H. doi:10.1016/0019-1035(79)90145-3.
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This page was last edited on 30 July 2023, at 23:58