2021
DOI: 10.2138/am-2021-7632
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An evolutionary system of mineralogy, Part IV: Planetesimal differentiation and impact mineralization (4566 to 4560 Ma)

Abstract: The fourth installment of the evolutionary system of mineralogy considers two stages of planetesimal mineralogy that occurred early in the history of the solar nebula, commencing by 4.566 Ga and lasting for at least 5 million years: (1) primary igneous minerals derived from planetesimal melting and differentiation into core, mantle, and basaltic components; and (2) impact mineralization resulting in shock-induced deformation, brecciation, melting, and highpressure phase transformations. We tabulate 90 igneous … Show more

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Cited by 23 publications
(5 citation statements)
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“…Future investigations could use mineral natural kinds (Hazen et al, 2019; Hazen et al, 2020; Hazen & Morrison, 2020; Hazen & Morrison, 2021; Morrison & Hazen, 2020; Morrison & Hazen, 2021), which better illustrate natural chemical variations observed in mineral specimens, rather than mineral species; however, these data are not yet fully assembled and are therefore not yet available for study. Another solution is to define the term ‘chemical formula’, which differs from the IMA definition of idealized mineralogical formula and reflects the content of the impurities present in species.…”
Section: Future Workmentioning
confidence: 99%
“…Future investigations could use mineral natural kinds (Hazen et al, 2019; Hazen et al, 2020; Hazen & Morrison, 2020; Hazen & Morrison, 2021; Morrison & Hazen, 2020; Morrison & Hazen, 2021), which better illustrate natural chemical variations observed in mineral specimens, rather than mineral species; however, these data are not yet fully assembled and are therefore not yet available for study. Another solution is to define the term ‘chemical formula’, which differs from the IMA definition of idealized mineralogical formula and reflects the content of the impurities present in species.…”
Section: Future Workmentioning
confidence: 99%
“…Structure data for high-pressure minerals at ambient pressure [5,17] cannot be used here because their bond distances represent the present state at ambient pressure but not at the conditions of formation. Many good experimental compression studies are on solid solutions such as bridgmanite-hiroseite, aluminous or ferraluminous bridgmanite, etc.…”
Section: Methodsmentioning
confidence: 99%
“…Part IV—Primary achondrite minerals (>4.560 Ga) : Planetesimal formation produced at least 94 primary igneous phases ( 29 ). These processes increased Earth's mineral inventory to 141 documented phases (all found in meteorites) that formed from m = 34 different chemical elements, with as many as eight elements [e.g.…”
Section: Mineral Evolution and Functional Informationmentioning
confidence: 99%