Samples of rhodonite (MnSiO_3-pyroxenoid from Franklin, New Jersey) have been shockloaded to pressures up to 496 kilobars. Optical spectral studies of four recovered samples show a decreasing Mn^(3+) content upon recovery from successively higher shock pressures; after shock-loading to 496 kbar, the Mn^(3+) has essentially disappeared. No corresponding change in the optical spectrum results from heating rhodonite to 1250°C for 3.5 hours in a reducing atmosphere. Rhodonite heated to 1360° under the same conditions melts incongruently to manganese-rich glass and silica with disappearance of the 540 nm Mn^(3+) absorption band. The color change in the shocked rhodonite arises from irreversible reduction of Mn3+ during high shock pressures and ...
The Gaussian resolution procedure of Faye (1975) leading to the conclusion that the spectral change...
The physical and chemical properties of materials are profoundly affected by highpressure and temper...
Shock metamorphism of minerals in meteorites could help to understand the shock history of its paren...
Samples of rhodonite (MnSiO_3-pyroxenoid from Franklin, New Jersey) have been shockloaded to pressur...
Samples of rhodonite (MnSiOa-pyroxenoid from Franklin, New Jersey) have been shock-loaded to pressur...
New infrared absorption spectra, thermo-gravimetric analyses and optical-and scanning electron micro...
[1] Optical emission of MgSiO3 glass, enstatite, olivine, and quartz under shock wave compression wa...
Thermoluminescence, electron paramagnetic resonance and optical absorption properties of rhodonite, ...
The physical and chemical properties of materials are profoundly affected by high pressure and tempe...
Literature data show that, among EH chondrites, the Abee impact-melt breccia exhibits unusual minera...
Electron spin resonance (ESR) studies have been carried out on three single grains of terrestrial ol...
International audienceTransient high pressures and temperatures generated during meteor or asteroid ...
Riverside nontronite, a candidate for the major mineral in the Martian fines, becomes both redder an...
Ovoid grains consisting of glass of stoichiometric (Mg, Fe)SiO3 composition that is intimately assoc...
MnSiO₃ - Mohs Hardness: 5½ - 6½. Rhodonite is a popular mineral among collectors. When it forms in ...
The Gaussian resolution procedure of Faye (1975) leading to the conclusion that the spectral change...
The physical and chemical properties of materials are profoundly affected by highpressure and temper...
Shock metamorphism of minerals in meteorites could help to understand the shock history of its paren...
Samples of rhodonite (MnSiO_3-pyroxenoid from Franklin, New Jersey) have been shockloaded to pressur...
Samples of rhodonite (MnSiOa-pyroxenoid from Franklin, New Jersey) have been shock-loaded to pressur...
New infrared absorption spectra, thermo-gravimetric analyses and optical-and scanning electron micro...
[1] Optical emission of MgSiO3 glass, enstatite, olivine, and quartz under shock wave compression wa...
Thermoluminescence, electron paramagnetic resonance and optical absorption properties of rhodonite, ...
The physical and chemical properties of materials are profoundly affected by high pressure and tempe...
Literature data show that, among EH chondrites, the Abee impact-melt breccia exhibits unusual minera...
Electron spin resonance (ESR) studies have been carried out on three single grains of terrestrial ol...
International audienceTransient high pressures and temperatures generated during meteor or asteroid ...
Riverside nontronite, a candidate for the major mineral in the Martian fines, becomes both redder an...
Ovoid grains consisting of glass of stoichiometric (Mg, Fe)SiO3 composition that is intimately assoc...
MnSiO₃ - Mohs Hardness: 5½ - 6½. Rhodonite is a popular mineral among collectors. When it forms in ...
The Gaussian resolution procedure of Faye (1975) leading to the conclusion that the spectral change...
The physical and chemical properties of materials are profoundly affected by highpressure and temper...
Shock metamorphism of minerals in meteorites could help to understand the shock history of its paren...