THE CRYSTALLINE LUNAR SPHERULES: THEIR FORMATION AND IMPLICATIONS FOR THE ORIGIN OF METEORITIC CHONDRULES
Symes, STEVEN J. K., Sears, DEREK W. G., Akridge, D. GLEN, , Benoit, PAUL H.(1998). THE CRYSTALLINE LUNAR SPHERULES: THEIR FORMATION AND IMPLICATIONS FOR THE ORIGIN OF METEORITIC CHONDRULES. METEORITICS & PLANETARY SCIENCE, 33(1), 13-29. https://doi.org/10.1111/j.1945-5100.1998.tb01604.x
Datasets
| number | title | Methods | variables analyzed | ||
|---|---|---|---|---|---|
| 3 | RAW DATA FOR THE BULK COMPOSITIONS (WT% OXIDE) DETERMINED BY RASTERED-BEAM ELECTRON MICROPROBE ANALYSIS OF RANDOMLY SELECTED TYPE X AND TYPE Y CRYSTALLINE LUNAR SPHERULES | EMP | K2O, Na2O, CaO, TiO2, P2O5, SiO2, Cr2O3, FeO, Al2O3, MgO, MnO | ||
| 5 | COMPOSITIONS OF PLAGIOCLASE LATHES IN TYPE Y CLS (WT% OXIDE) | EMP | MgO, MnO, CaO, FeO, K2O, TiO2, Na2O, SiO2, Al2O3, P2O5, Cr2O3 | ||
| 6 | COMPOSITIONS OF METASTASIS REGIONS IN TYPE Y CLS (WT% OXIDES) | EMP | MgO, MnO, Na2O, Al2O3, CaO, Cr2O3, K2O, P2O5, TiO2, SiO2, FeO | ||
Methods
| method name | laboratory | method comment | More details are available for the following variables | |
|---|---|---|---|---|
| ELECTRON MICROPROBE | JOHNSON SPACE CENTER | CAMEBAX EMP. RAW DATA FOR BULK COMPOSITIONS DETERMINED BY RASTERED-BEAM EMP ANALYSIS |
