Premium
MINERALOGY, PETROLOGY AND CHEMISTRY OF THE ISNA (C3) METEORITE
Author(s) -
Methot Robert L.,
Noonan Albert F.,
Jarosewich Eugene,
deGasparis Aurelio A.,
AlFar D.M.
Publication year - 1975
Publication title -
meteoritics
Language(s) - English
Resource type - Journals
eISSN - 1945-5100
pISSN - 0026-1114
DOI - 10.1111/j.1945-5100.1975.tb00017.x
Subject(s) - troilite , nepheline , kamacite , enstatite , augite , meteorite , chondrite , olivine , chondrule , diopside , anorthite , mineralogy , geology , pyroxene , melilite , chemistry , spinel , plagioclase , astrobiology , quartz , paleontology , physics
A total chemical analysis of the Isna, Egypt, meteorite is similar to analyses for chondrites of type C3, Ornans sub‐type; however, comparison with one group of chemical data indicates that Isna is intermediate between the C3(O)'s and C3(V)'s in terms of total Fe. On the basis of atom ratios of Fe, Ca, Al, and Ti to Si, Isna can also be placed into a chemical group which includes types C1 and C2, as well as C3(O). Thin sections show a variety of small, closely‐packed chondrules, fragments, and aggregate‐like masses in a poorly translucent matrix. Olivine + clinoenstatite inclusions rich in metal and troilite, and olivine‐rich inclusions are abundant and show evidence of shock. Ca‐Al‐Ti‐ rich inclusions, of probable high‐temperature origin, contain olivine, spinel , Ca‐ rich nepheline, gehlenite, diopside, augite, enstatite, and anorthite. Kamacite and taenite from various occurrences in the meteorite have rather uniform Ni and Co contents, and Ni/Co for kamacite is close to that for several C3(O)'s.