The Martian meteorite North West Africa 6162 (NWA 6162) is a shergottite found in Morocco in 2010. The meteorite has large olivine crystals with Mg-depleted rims as low as FO(sub 65) and Mg-rich cores of up to FO(sub 74). It is similar both in appearance and composition to another shergottite, SaU 005. Our objective is to determine if NWA 6162 represents a liquid or if it is a product of olivine accumulation. Olivine accumulation would leave the parent melt Mg-depleted and the complementary olivine cumulates would be Mg-enriched. Therefore, if NWA 6162 is a partial cumulate we would expect that liquidus olivines grown from this bulk composition would be more magnesium than olivines in the natural sample
Martian meteorite RBT 04262 is in the shergottite class. It displays the two lithologies typically f...
Martian basalts can be classified in at least two geochemically different families: enriched and dep...
We performed a series of experiments at 1 atm pressure and temperatures of 1300–1500 °C to determine...
The Tissint meteorite is a geochemically depleted, olivine-phyric shergottite. Olivine megacrysts co...
© 2017 Elsevier Ltd Martian meteorites are the only samples available from the surface of Mars. Amo...
The 13th Symposium on Polar Science/Ordinary sessions [OA] Antarctic meteorites, Thu. 17 Nov
The DaG 476 martian meteorite shows a porphyritic texture with megacrysts of olivine and orthopyroxe...
The partitioning of elements between olivine and liquid is key to understanding igneous processes i...
Olivine-phyric shergottites are relatively young Martian meteorites that resemble primitive mantle-d...
Most Martian meteorites are heavily shocked, exhibiting numerous shock features, for example undulat...
Knowledge of Martian igneous and mantle compositions is crucial for understanding Mars’ mantle evolu...
NWA 856 or Djel Ibone, is a basaltic shergottite discovered as a single stone of 320 g in South Moro...
Martian meteorites are the only samples currently available on Earth to study Mars. Most martian met...
Artificial meteor ablation was performed on a Mg-rich olivine sample using an arc-heated plasma of i...
Y980459, a new Martian meteorite from Antarctica, is composed of coarse porphyritic olivine grains (...
Martian meteorite RBT 04262 is in the shergottite class. It displays the two lithologies typically f...
Martian basalts can be classified in at least two geochemically different families: enriched and dep...
We performed a series of experiments at 1 atm pressure and temperatures of 1300–1500 °C to determine...
The Tissint meteorite is a geochemically depleted, olivine-phyric shergottite. Olivine megacrysts co...
© 2017 Elsevier Ltd Martian meteorites are the only samples available from the surface of Mars. Amo...
The 13th Symposium on Polar Science/Ordinary sessions [OA] Antarctic meteorites, Thu. 17 Nov
The DaG 476 martian meteorite shows a porphyritic texture with megacrysts of olivine and orthopyroxe...
The partitioning of elements between olivine and liquid is key to understanding igneous processes i...
Olivine-phyric shergottites are relatively young Martian meteorites that resemble primitive mantle-d...
Most Martian meteorites are heavily shocked, exhibiting numerous shock features, for example undulat...
Knowledge of Martian igneous and mantle compositions is crucial for understanding Mars’ mantle evolu...
NWA 856 or Djel Ibone, is a basaltic shergottite discovered as a single stone of 320 g in South Moro...
Martian meteorites are the only samples currently available on Earth to study Mars. Most martian met...
Artificial meteor ablation was performed on a Mg-rich olivine sample using an arc-heated plasma of i...
Y980459, a new Martian meteorite from Antarctica, is composed of coarse porphyritic olivine grains (...
Martian meteorite RBT 04262 is in the shergottite class. It displays the two lithologies typically f...
Martian basalts can be classified in at least two geochemically different families: enriched and dep...
We performed a series of experiments at 1 atm pressure and temperatures of 1300–1500 °C to determine...