Although the majority of carbonaceous chondrites have only experienced low-intensity (<5 GPa) impacts, we show that compacting initially highly porous matrix aggregates results in large temperature excursions even at low shock pressures
Northwest Africa (NWA) 8709 is a rare example of a type 3 ordinary chondrite melt breccia and provid...
The 13th Symposium on Polar Science/Ordinary sessions [OA] Antarctic meteorites, Thu. 17 Nov
Petrographic analysis of eight CM carbonaceous chondrites (EET 96029, LAP 031166, LON 94101, MET 010...
Prior to becoming chondritic meteorites, primordial solids were a poorly consolidated mix of mm-scal...
Micrometeorites have been significantly altered or melted by heating, which has been mainly ascribed...
Primitive solar system solids were accreted as highly porous bimodal mixtures of mm-sized chondrules...
Recent work has explored the effects of low-intensity impacts into porous chondrite precursors. We s...
Collisions and attendant shock compaction must have been important for the accretion and lithificati...
We have developed a method for simulating the mesoscale compaction of early solar system solids in l...
AbstractPetrographic analysis of eight CM carbonaceous chondrites (EET 96029, LAP 031166, LON 94101,...
Petrographic analysis of eight CM carbonaceous chondrites (EET 96029, LAP 031166, LON 94101, MET 010...
The CV3 Allende is one of the most extensively studied meteorites in worldwide collections. It is cu...
Special Issue: 74th Annual Meeting of the Meteoritical Society, August 8-12, 2011, London, U.K.Inter...
The CV3 Allende is one of the most extensively studied meteorites in worldwide collections. It is cu...
Miller Range 07273 is a chondritic melt breccia that contains clasts of equilibrated ordinary chondr...
Northwest Africa (NWA) 8709 is a rare example of a type 3 ordinary chondrite melt breccia and provid...
The 13th Symposium on Polar Science/Ordinary sessions [OA] Antarctic meteorites, Thu. 17 Nov
Petrographic analysis of eight CM carbonaceous chondrites (EET 96029, LAP 031166, LON 94101, MET 010...
Prior to becoming chondritic meteorites, primordial solids were a poorly consolidated mix of mm-scal...
Micrometeorites have been significantly altered or melted by heating, which has been mainly ascribed...
Primitive solar system solids were accreted as highly porous bimodal mixtures of mm-sized chondrules...
Recent work has explored the effects of low-intensity impacts into porous chondrite precursors. We s...
Collisions and attendant shock compaction must have been important for the accretion and lithificati...
We have developed a method for simulating the mesoscale compaction of early solar system solids in l...
AbstractPetrographic analysis of eight CM carbonaceous chondrites (EET 96029, LAP 031166, LON 94101,...
Petrographic analysis of eight CM carbonaceous chondrites (EET 96029, LAP 031166, LON 94101, MET 010...
The CV3 Allende is one of the most extensively studied meteorites in worldwide collections. It is cu...
Special Issue: 74th Annual Meeting of the Meteoritical Society, August 8-12, 2011, London, U.K.Inter...
The CV3 Allende is one of the most extensively studied meteorites in worldwide collections. It is cu...
Miller Range 07273 is a chondritic melt breccia that contains clasts of equilibrated ordinary chondr...
Northwest Africa (NWA) 8709 is a rare example of a type 3 ordinary chondrite melt breccia and provid...
The 13th Symposium on Polar Science/Ordinary sessions [OA] Antarctic meteorites, Thu. 17 Nov
Petrographic analysis of eight CM carbonaceous chondrites (EET 96029, LAP 031166, LON 94101, MET 010...