Tungsten and osmium isotopic compositions and W, Hf and HSE abundances of metals separated from Apollo 16 lunar impact melt rocks.

Creator(s):
Touboul, Mathieu
Walker, Richard J; ORCID: 0000-0003-0348-2407; SCOPUS: 56134046800
Puchtel, Igor S; SCOPUS: 6603763674
Abstract:
The dataset presents W and Os isotopic compositions and W, Hf and HSE abundances of metals separated from Apollo 16 lunar impact melt rocks. These data are used to determine the W isotope composition of the lunar mantle, monitoring potential effects of meteoritic contamination and cosmic rays on W isotopes.
How to cite this dataset:
Touboul, M., Walker, R. J., Puchtel, I. S., 2015. Tungsten and osmium isotopic compositions and W, Hf and HSE abundances of metals separated from Apollo 16 lunar impact melt rocks., Version 1.0. Interdisciplinary Earth Data Alliance (IEDA). https://doi.org/10.1594/IEDA/100524. Accessed 2021-05-14.
DOI Creation Date:
2015-02-23
Related
Publication(s):
Touboul M., Puchtel I.S., Walker R.J. (2015) "Tungsten isotopic evivence for disproportional late accretion to the Earth and Moon." Nature 520, 530–533.
Publication DOI:
License:
Creative Commons Attribution-NonCommercial-Share Alike 3.0 United States [CC BY-NC-SA 3.0]
User Contributed Keyword(s):
Tungsten isotopes, siderophile, lunar mantle, impact melt
Data Available On:
2015-08-15
Resource Type:
Dataset
Download File(s)
File Name
File Size
File Checksum
849-1_EarthChemdataset_Apollo16_impactmeltmetals_Touboul.xls
144 KB

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