TY - JOUR
T1 - The terrestrial alteration of saharan shergottites dar al ganid 476 and 489
T2 - A case study of weathering in a hot desert environment
AU - Crozaz, Ghislaine
AU - Wadhwa, Meenakshi
N1 - Funding Information:
This study received financial support from National Science Foundation Grants EAR96-14212 and EAR99-80394 to G.C. and EAR97-25659 to M.W.
PY - 2001
Y1 - 2001
N2 - Rare earth element (REE) and other selected trace and minor element concentrations were determined in various phases of Dar al Gani 476 and 489, two basaltic shergottites recently found in the Libyan Sahara. Whereas merrillite and feldspathic glass compositions do not seem to have been altered since the fall of these meteorites, olivine and pyroxenes commonly show light REE enrichments, sometimes accompanied by Ce anomalies, that are attributed to terrestrial alteration. Sr and Ba enrichments are also observed. The calcium carbonate that resides in most cracks is essentially devoid of REE but a fine-grained amorphous silicate material that fills some veins and pockets has striking light REE enrichments and elevated P, Sr, and Ba. It is argued that this material, likely to be impact melt, as well as the notoriously light REE-poor olivine and pyroxenes, were preferentially affected by a crustal light REE-rich contaminant. Caution is urged when using whole rock, or even mineral separate, compositional, and isotopic data for hot desert meteorites.
AB - Rare earth element (REE) and other selected trace and minor element concentrations were determined in various phases of Dar al Gani 476 and 489, two basaltic shergottites recently found in the Libyan Sahara. Whereas merrillite and feldspathic glass compositions do not seem to have been altered since the fall of these meteorites, olivine and pyroxenes commonly show light REE enrichments, sometimes accompanied by Ce anomalies, that are attributed to terrestrial alteration. Sr and Ba enrichments are also observed. The calcium carbonate that resides in most cracks is essentially devoid of REE but a fine-grained amorphous silicate material that fills some veins and pockets has striking light REE enrichments and elevated P, Sr, and Ba. It is argued that this material, likely to be impact melt, as well as the notoriously light REE-poor olivine and pyroxenes, were preferentially affected by a crustal light REE-rich contaminant. Caution is urged when using whole rock, or even mineral separate, compositional, and isotopic data for hot desert meteorites.
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U2 - 10.1016/S0016-7037(00)00586-X
DO - 10.1016/S0016-7037(00)00586-X
M3 - Article
AN - SCOPUS:0035064942
SN - 0016-7037
VL - 65
SP - 971
EP - 977
JO - Geochimica et Cosmochimica Acta
JF - Geochimica et Cosmochimica Acta
IS - 6
ER -