Brownleeite: A New Manganese Silicide Mineral in an Interplanetary Dust Particle
Document Type
Article
Publication Date
2010
Abstract
Brownleeite, ideally stoichiometric MnSi, is a manganese silicide not previously observed in nature that was discovered within an interplanetary dust particle that likely originated from a comet. Three submicrometer brownleeite grains were found, with one of them poikilitically enclosed by Mn-bearing forsterite. Owing to the small size of the brownleeite grains, it was not possible to determine conventional macroscopic properties of this mineral; however, the chemical composition and crystal structure were well constrained by extensive quantitative energy dispersive X-ray analysis and electron diffraction using transmission electron microscopy (TEM). The crystal system for brownleeite is cubic (a = 4.557 Å) with space group P213, cell volume = 94.63 Å3, Z = 4, density (calculated) = 2.913 g/cm3, and empirical formula: (Mn0.77Fe0.18Cr0.05)Si. These brownleeite grains likely formed as high-temperature condensates either in the early Solar System or in the outflow of an evolved star or supernova explosion.
Department
Physics and Astronomy
Publication Title
American Mineralogist
Recommended Citation
K. Nakamura-Messenger, L.P. Keller, S.J. Clemett, S. Messenger, J.H. Jones, R.L. Palma, R.O. Pepin, W. Klöck, M.E. Zolensky, and H. Tatsuoka, 2010. Brownleeite: a New Manganese Silicide Mineral in an Interplanetary Dust Particle. American Mineralogist 95, 221-228.
DOI
10.2138/am.2010.3263
Link to Publisher Version (DOI)
Publisher's Copyright and Source
Copyright © 2010 American Mineralogist. Article published by American Mineralogist in American Mineralogist, volume 95, issue number 2-3, 2010, pages 221-228. Available online: https://doi.org/10.2138/am.2010.3263