The Martian meteorites (MMs) are peculiar igneous rocks distinguished from other achondrite meteorites based on their different petrography, mineralogy, mineral-chemistry, major and trace elements, and isotopic compositions. To date, MMs are classified into three main groups: Shergottites (basalts), Nakhlites (clinopyroxenites), and Chassignite (dunite). In addition, two unique types of meteorites have been found: ALH84001 (orthopyroxenite) and NWA 7034 (and the related pairs) regolith breccias.
“Chirfa” meteorite: the largest specimen from Mars / Shehaj, X.; Ammannito, E.; Pratesi, G.. - ELETTRONICO. - (2024), pp. 964-964. (Intervento presentato al convegno Congresso congiunto SGI-SIMP - Geology for a sustainable management of our Planet, Bari 2-5 settembre 2024).
“Chirfa” meteorite: the largest specimen from Mars
Shehaj, X.
;Pratesi, G.
2024
Abstract
The Martian meteorites (MMs) are peculiar igneous rocks distinguished from other achondrite meteorites based on their different petrography, mineralogy, mineral-chemistry, major and trace elements, and isotopic compositions. To date, MMs are classified into three main groups: Shergottites (basalts), Nakhlites (clinopyroxenites), and Chassignite (dunite). In addition, two unique types of meteorites have been found: ALH84001 (orthopyroxenite) and NWA 7034 (and the related pairs) regolith breccias.
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