The issue of whether crustal contamination has affected the lithophile trace element budget of shergottites has been a point of contention for decades. The evaluation has focused on the enriched shergottite compositions as an outcome of crustal contamination of mantle-derived parent magmas or, alternatively, the compositions of these stones reflect an incompatible trace element (ITE) enriched mantle source
Samarium-neodymium isotopic analyses of unleached and acid-leached mineral fractions from the recent...
Compared to terrestrial basalts, the Martian shergottite meteorites have an extraordinary range of S...
Bulk chemical compositions of the shergottite basalts provide important constraints on magma genesis...
The origin of the incompatible trace element (ITE) enriched compositions of shergottites has been a ...
Shergottites are the most abundant type of meteorite we have from Mars and their study is invaluable...
Geochemically-depleted shergottites are basaltic rocks derived from a martian mantle source reservoi...
Shergottites, the largest martian meteorite group, come from at least two geochemically different so...
Geochemical studies of shergottites suggest that their parental magmas reflect mixtures between at l...
We present a study of the petrology and geochemistry of basaltic shergottite Northwest Africa 2975 (...
NWA 856 or Djel Ibone, is a basaltic shergottite discovered as a single stone of 320 g in South Moro...
The Tenth Symposium on Polar Science/Special session: [OA] Antarctic meteorites, Thur. 5 Dec. / 3F M...
The Martian shergottite meteorites are basaltic to lherzolitic igneous rocks that represent a period...
Martian basalts can be classified in at least two geochemically different families: enriched and dep...
The SNC meteorites are samples of the Martian crust, so inferences about their origins and parent ma...
Martian poikilitic shergottite meteorites are cumulate rocks that can be used to understand melt evo...
Samarium-neodymium isotopic analyses of unleached and acid-leached mineral fractions from the recent...
Compared to terrestrial basalts, the Martian shergottite meteorites have an extraordinary range of S...
Bulk chemical compositions of the shergottite basalts provide important constraints on magma genesis...
The origin of the incompatible trace element (ITE) enriched compositions of shergottites has been a ...
Shergottites are the most abundant type of meteorite we have from Mars and their study is invaluable...
Geochemically-depleted shergottites are basaltic rocks derived from a martian mantle source reservoi...
Shergottites, the largest martian meteorite group, come from at least two geochemically different so...
Geochemical studies of shergottites suggest that their parental magmas reflect mixtures between at l...
We present a study of the petrology and geochemistry of basaltic shergottite Northwest Africa 2975 (...
NWA 856 or Djel Ibone, is a basaltic shergottite discovered as a single stone of 320 g in South Moro...
The Tenth Symposium on Polar Science/Special session: [OA] Antarctic meteorites, Thur. 5 Dec. / 3F M...
The Martian shergottite meteorites are basaltic to lherzolitic igneous rocks that represent a period...
Martian basalts can be classified in at least two geochemically different families: enriched and dep...
The SNC meteorites are samples of the Martian crust, so inferences about their origins and parent ma...
Martian poikilitic shergottite meteorites are cumulate rocks that can be used to understand melt evo...
Samarium-neodymium isotopic analyses of unleached and acid-leached mineral fractions from the recent...
Compared to terrestrial basalts, the Martian shergottite meteorites have an extraordinary range of S...
Bulk chemical compositions of the shergottite basalts provide important constraints on magma genesis...