Understanding the textures of Apollo 11 high-Ti mare basalts: A quantitative petrographic approach

Creator(s):
Xue, Zhuqing
Abstract:
This dataset contains crystal size distribution (CSD) data of ilmenite and plagioclase for a suite of 12 Apollo 11 high-Ti basalts from four groups. The purpose of the dataset is to investigate how cooling rate, bulk composition, and nucleation density can influence textures of different Apollo 11 basalts. This dataset can help uncover the crystallization environment and effusion rates of loose basalt samples which are not from actual outcrops.
How to cite this dataset:
Xue, Z., 2021. Understanding the textures of Apollo 11 high-Ti mare basalts: A quantitative petrographic approach, Version 1.0. Interdisciplinary Earth Data Alliance (IEDA). https://doi.org/10.26022/IEDA/112193. Accessed 2026-09-21.
DOI Creation Date:
2021-12-13
License:
Creative Commons Attribution-ShareAlike 4.0 International [CC-BY-SA-4.0]
User Contributed Keyword(s):
Apollo 11, high-Ti basalts, ilmenite, crystal size distributions, cooling regimes, nucleation densities, the Moon
Data Available On:
2021-12-13
Resource Type:
Collection
Download File(s)
File Name
File Size
File Checksum
2193-1_CSDprofilesofApollo11basalts.docx
1.17 MB
2193-2_ImagesofApollo11basalts.docx
36.11 MB
2193-3_PetrographyandcrystalsizedistributiondataofApollo11basalts.xlsx
19.17 KB
Format Type
tar.gz  sha1
zip  sha1

Related Information
References:
Mission: apollo-11