Physics
Scientific paper
Nov 1998
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998m%26ps...33.1271p&link_type=abstract
Meteoritics & Planetary Science, vol. 33, no. 6, pp. 1271-1279.
Physics
6
Scientific paper
Detailed investigations of the microimpact phenomena on Australasian microtektites from four samples in the Central Indian Basin reveal an array of features such as very low velocity captured droplets, welded projectiles, angular fragments and dust, craters generated by projectiles defining an oblique trajectory, high velocity `pitless' craters and the conventional hypervelocity craters with a well defined central pit, radial and concentric cracks - found commonly on lunar surface materials. The microimpacts are a consequence of interparticle collisions within the ejecta plume (as suggested by their chemistry ) subsequent to a major impact and therefore reveal processes inherent in an impact generated plume. All the impact phenomena observed here have taken place while the targets and projectiles were in flight and are therefore secondary impacts in lunar terms. However, some of the resultant features are analogous to lunar microcraters attributed to primary impacts by cosmic dust. Therefore, ballistic sedimentation on the moon is likely to contain plume collisional debris as well.
Prasad Shyam M.
Sudhakar Manju
No associations
LandOfFree
Microimpact phenomena on Australasian microtektites: Implications for ejecta plume characteristics and lunar surface processes does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Microimpact phenomena on Australasian microtektites: Implications for ejecta plume characteristics and lunar surface processes, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Microimpact phenomena on Australasian microtektites: Implications for ejecta plume characteristics and lunar surface processes will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-803161