CK carbonaceous chondrites are a highly thermally altered group of carbonaceous chondrites, experiencing temperatures ranging between approximately 576-867 degrees Centigrade. Additionally, the mineralogy of the CK chondrites record the highest overall oxygen fugacity of all chondrites, above the fayalite-magnetite-quartz (FMQ) buffer. Me-tallic Fe-Ni is extremely rare in CK chondrites, but magnetite and Fe,Ni sulfides are commonly observed. Noble metal-rich inclusions have previously been found in some magnetite and sulfide grains. These arsenides, tellurides, and sulfides, which contain varying amounts of Pt, Ru, Os, Te, As, Ir, and S, are thought to form either by condensation from a solar gas, or by exsolution during metamorphism on the...
Mineral grains and matrix of heated chondrites Yamato (Y)-82162,Belgica (B)-7904,Y-86720,and Asuka (...
The unique CO3-chondrite Y-82094 contains abundant FeNi metals. FeNi metal grains are often surround...
The metal-rich (>20 vol% Fe,Ni-metal) carbonaceous chondrites include CH chondrites, CB chondrites ...
CK carbonaceous chondrites are a highly thermally altered group of carbonaceous chondrites, experien...
The recent discoveries of primitive achondrites, metachondrites, and type 7 chondrites challenge the...
CK carbonaceous chondrites are the only group of carbonaceous chondrites that exhibit thermal metamo...
Recent chondritic meteorite finds in Antarctica have included CB, CH, CK and R chondrites, the latte...
Chondrules are generally believed to have lost most or all of their trapped noble gases during their...
The Aguas Zarcas meteorite fell in Costa Rica on 23 April 2019 at 21:07 local time, with a total mas...
CK chondrites constitute the most oxidized anhydrous carbonaceous chondrite group; most of the Fe oc...
Olivine inclusions and chondrules of Kainsaz were formed in a unique process of dust matter melting....
CK chondrites are a relatively new class of carbonaceous chondrite that have been described in the l...
Equilibrated Rumuruti (R) chondrites record an oxygen fugacity between 0 and 3.5 log units below the...
We report on the mineralogy, petrography, and in situ oxygen isotopic composition of twenty-five ult...
Calcium, Aluminum-rich inclusions (CAIs) are the first forming solids of the Solar system. Their obs...
Mineral grains and matrix of heated chondrites Yamato (Y)-82162,Belgica (B)-7904,Y-86720,and Asuka (...
The unique CO3-chondrite Y-82094 contains abundant FeNi metals. FeNi metal grains are often surround...
The metal-rich (>20 vol% Fe,Ni-metal) carbonaceous chondrites include CH chondrites, CB chondrites ...
CK carbonaceous chondrites are a highly thermally altered group of carbonaceous chondrites, experien...
The recent discoveries of primitive achondrites, metachondrites, and type 7 chondrites challenge the...
CK carbonaceous chondrites are the only group of carbonaceous chondrites that exhibit thermal metamo...
Recent chondritic meteorite finds in Antarctica have included CB, CH, CK and R chondrites, the latte...
Chondrules are generally believed to have lost most or all of their trapped noble gases during their...
The Aguas Zarcas meteorite fell in Costa Rica on 23 April 2019 at 21:07 local time, with a total mas...
CK chondrites constitute the most oxidized anhydrous carbonaceous chondrite group; most of the Fe oc...
Olivine inclusions and chondrules of Kainsaz were formed in a unique process of dust matter melting....
CK chondrites are a relatively new class of carbonaceous chondrite that have been described in the l...
Equilibrated Rumuruti (R) chondrites record an oxygen fugacity between 0 and 3.5 log units below the...
We report on the mineralogy, petrography, and in situ oxygen isotopic composition of twenty-five ult...
Calcium, Aluminum-rich inclusions (CAIs) are the first forming solids of the Solar system. Their obs...
Mineral grains and matrix of heated chondrites Yamato (Y)-82162,Belgica (B)-7904,Y-86720,and Asuka (...
The unique CO3-chondrite Y-82094 contains abundant FeNi metals. FeNi metal grains are often surround...
The metal-rich (>20 vol% Fe,Ni-metal) carbonaceous chondrites include CH chondrites, CB chondrites ...