Petrology of Apollo 11 regolith breccias.

Details Petrology of Apollo 11 regolith breccias. Petrology of Apollo 11 regolith breccias.

Jan 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984jgr....89..109s&link_type=abstract

Journal of Geophysical Research, Vol. 89, Suppl., p. C109 - C132

Physics

1

Moon Samples:Petrology, Moon:Regolith

Scientific paper

Petrographic and mineral chemical data for 16 Apollo 11 regolith breccias show that: (1) the regolith breccias differ from soil 10084 with respect to (a) agglutinate content, (b) glass population, (c) plagioclase compositions, and (d) proportions of high-K mare and low-K mare basalt components; (2) the A-11 breccias and soil have highland components that are similar both in abundance and petrology; and (3) lunar regolith breccias provide a better comparison with howardites than do lunar soils. The data and observations are consistent with formation of the regolith breccias from immature soil. It appears that little or no highland material has been added to the Tranquilitatis regolith since the formation of the breccias.

Affiliated with

Also associated with

No associations

Rating

Petrology of Apollo 11 regolith breccias. 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 Petrology of Apollo 11 regolith breccias., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Petrology of Apollo 11 regolith breccias. will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-937317