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1
The Theory of Micro-Meteorites: Part I. In an Isothermal Atmosphere.
Proc Natl Acad Sci U S A. 1950 Dec;36(12):687-95. doi: 10.1073/pnas.36.12.687.
3
Cohenite in meteorites: a proposed origin.
Science. 1966 Jul 1;153(3731):60-2. doi: 10.1126/science.153.3731.60.
4
The Theory of Micro-Meteorites: Part II. In Heterothermal Atmospheres.
Proc Natl Acad Sci U S A. 1951 Jan;37(1):19-30. doi: 10.1073/pnas.37.1.19.
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[Study on the Element Composition of Ancient Fossils and Meteorites].
Guang Pu Xue Yu Guang Pu Fen Xi. 2017 Jan;37(1):247-9.
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Interplanetary dust from the explosive dispersal of hydrated asteroids by impacts.
Nature. 2003 May 1;423(6935):60-2. doi: 10.1038/nature01567.
8
A mechanism for producing magnetic remanence in meteorites and lunar samples by cosmic-ray exposure.
Science. 1971 May 28;172(3986):939-41. doi: 10.1126/science.172.3986.939.
10
What CO2 well gases tell us about the origin of noble gases in the mantle and their relationship to the atmosphere.
Philos Trans A Math Phys Eng Sci. 2008 Nov 28;366(1883):4183-203. doi: 10.1098/rsta.2008.0150.

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1
Remote detection of a lunar granitic batholith at Compton-Belkovich.
Nature. 2023 Aug;620(7972):116-121. doi: 10.1038/s41586-023-06183-5. Epub 2023 Jul 5.
2
The Theory of Micro-Meteorites: Part II. In Heterothermal Atmospheres.
Proc Natl Acad Sci U S A. 1951 Jan;37(1):19-30. doi: 10.1073/pnas.37.1.19.

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