New constraints on the formation of main group pallasites derived from in situ trace element analysis and 2D mapping of olivine and phosphate
M. Chernonozhkin, Seann J. McKibbin, Steven Goderis, Stijn J.M.Van Malderen, Philippe Claeys, Frank Vanhaecke Chemical GeologyAvailable online 20 December 2020 LINK “Pallasites are stony‑iron meteorites consisting mainly of olivine and Fe-Ni metal with a formation…
Ferrovolcanism on metal worlds and the origin of pallasitesOPEN ACCESS
Brandon C. Johnson, Michael M. Sori & Alexander J. Evans Nature Astronomy, 1–4, published: 16 September 2019 LINK PDF (OPEN ACCESS) “As differentiated planetesimals cool, their cores can solidify from the outside in1, as evidenced…
The Fukang pallasite: Characterization and implications for the history of the Main‐group parent body
Daniella N. Della Giustina, Namrah Habib, Kenneth J. Domanik, Dolores H. Hill, Dante S. Lauretta, Yulia S. Goreva, Marvin Killgore, Yang Hexiong, Robert T. Downs Meteoritics & Planetary Science First Published: 16 July 2019 LINK…
Olivine grain growth in partially molten Fe–Ni–S: A proxy for the genesis of pallasite meteorites
Giulio F.D. Solferino, Gregor J. Golabek Earth and Planetary Science Letters Volume 504, 15 December 2018, Pages 38-52 LINK “Highlights • Olivine grain growth in metal matrix is faster when metal is partially molten. •…
