Australasian Microtektites in the South China Sea: Implications Regarding the Location and Size of the Source Crater

Details Australasian Microtektites in the South China Sea: Implications Regarding the Location and Size of the Source Crater Australasian Microtektites in the South China Sea: Implications Regarding the Location and Size of the Source Crater

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003lpi....34.1092g&link_type=abstract

34th Annual Lunar and Planetary Science Conference, March 17-21, 2003, League City, Texas, abstract no.1092

Other

2

Scientific paper

The highest concentration of Australasian microtektites and the highest
ratio of unmelted ejecta to microtektites has been found in at ODP Hole
1144A in the northern South China Sea. These, and other data, were used
to reevaluate the location and size of the Australasian strewn filed
source crater

Affiliated with

Also associated with

No associations

Rating

Australasian Microtektites in the South China Sea: Implications Regarding the Location and Size of the Source Crater 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 Australasian Microtektites in the South China Sea: Implications Regarding the Location and Size of the Source Crater, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Australasian Microtektites in the South China Sea: Implications Regarding the Location and Size of the Source Crater will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1006381