AbstractThe composition of basaltic melts in equilibrium with the mantle can be determined for sever...
International audienceWe have performed piston–cylinder experiments on a primitive martian mantle co...
Rocks on the floor of Gusev crater are basalts of uniform composition and mineralogy. Olivine, the o...
We performed a series of experiments at 1 atm pressure and temperatures of 1300–1500 °C to determine...
The partitioning of elements between olivine and liquid is key to understanding igneous processes i...
Several types of Martian igneous meteorites have been identified: clinopyroxenites (nakhlites), basa...
Martian magmas are known to be FeO-rich and the dominant FeO-bearing mineral at many sites visited b...
Martian magmas are known to be FeO-rich and the dominant FeO-bearing mineral at many sites visited b...
Knowledge of Martian igneous and mantle compositions is crucial for understanding Mars’ mantle evolu...
The martian surface is predominantly covered by FeO-rich basalts and their alteration products. Seve...
Martian basalts can be classified in at least two geochemically different families: enriched and dep...
Experimentally rehomogenized melt inclusions from the nakhlite Miller Range 03346 (MIL 03346) and th...
Shergottites, the largest martian meteorite group, come from at least two geochemically different so...
Olivine-phyric shergottites are relatively young Martian meteorites that resemble primitive mantle-d...
Antarctic meteorite Queen Alexandra Range (QUE) 94201 is a 12 g basaltic achondrite dominated by pla...
AbstractThe composition of basaltic melts in equilibrium with the mantle can be determined for sever...
International audienceWe have performed piston–cylinder experiments on a primitive martian mantle co...
Rocks on the floor of Gusev crater are basalts of uniform composition and mineralogy. Olivine, the o...
We performed a series of experiments at 1 atm pressure and temperatures of 1300–1500 °C to determine...
The partitioning of elements between olivine and liquid is key to understanding igneous processes i...
Several types of Martian igneous meteorites have been identified: clinopyroxenites (nakhlites), basa...
Martian magmas are known to be FeO-rich and the dominant FeO-bearing mineral at many sites visited b...
Martian magmas are known to be FeO-rich and the dominant FeO-bearing mineral at many sites visited b...
Knowledge of Martian igneous and mantle compositions is crucial for understanding Mars’ mantle evolu...
The martian surface is predominantly covered by FeO-rich basalts and their alteration products. Seve...
Martian basalts can be classified in at least two geochemically different families: enriched and dep...
Experimentally rehomogenized melt inclusions from the nakhlite Miller Range 03346 (MIL 03346) and th...
Shergottites, the largest martian meteorite group, come from at least two geochemically different so...
Olivine-phyric shergottites are relatively young Martian meteorites that resemble primitive mantle-d...
Antarctic meteorite Queen Alexandra Range (QUE) 94201 is a 12 g basaltic achondrite dominated by pla...
AbstractThe composition of basaltic melts in equilibrium with the mantle can be determined for sever...
International audienceWe have performed piston–cylinder experiments on a primitive martian mantle co...
Rocks on the floor of Gusev crater are basalts of uniform composition and mineralogy. Olivine, the o...