Data from grain-size separates, stepwise-heated fractions, and bulk analyses of 20 samples of fines and breccias from five lunar sites are used to define three-isotope and ordinate intercept correlations in an attempt to resolve the lunar heavy rare gas system in a statistically valid approach. Tables of concentrations and isotope compositions are given.
Krypton and xenon in lunar fines
Lunar Science Conference ; 1973 ; Houston, TX
1973-01-01
Miscellaneous
No indication
English
NTRS | 1970
|Total emittance of lunar fines.
NTRS | 1972
|Glassy particles in lunar fines
NTRS | 1970
|