Heterogeneous distribution of moderately volatile elements in the Moon determined from Apollo 15 and 17 pyroclastic glass beads

Description

Quantitative moderately volatile element abundance data obtained by laser ablation inductively coupled plasma mass spectrometry on the Apollo 15 low-Ti and Apollo 17 high-Ti pyroclastic glass beads. The methods, results and interpretation of these data are presented in a manuscript of the same name "Heterogeneous distribution of moderately volatile elements in the Moon determined from Apollo 15 and 17 pyroclastic glass beads" by McIntosh, E.C. and Day, J.M.D. Within the excel file are seven sub-tabs: Table 1: Average moderately volatile element abundance (ug/g) data for 74220 and 15426. Table S1: Compiled corrected data for lunar sample 74220 (in ug/g). Table S2: Compiled corrected data for lunar sample 15426 (in ug/g). Table S3: NIST 610 Standard Data for Sessions (in ug/g). Table S4: BHVO-2g Standard Data for Sessions (in ug/g). Table S5: BCR-2G Standard Data for Sessions (in ug/g). Table S6: BIR-1G Standard Data for Sessions (in ug/g).

Steps to reproduce

Data reproduction should be done on appropriate thin-sections, using the same standard reference materials, using LA-ICP-MS.

Institutions

• University of California San Diego

  CA, La Jolla

Categories

Funders

• National Aeronautics and Space Administration

  District of Columbia, United States

  Grant ID: 80NSSC19K0932
• National Aeronautics and Space Administration

  District of Columbia, United States

  Grant ID: 80NSSC22K0098

Licence