The Arispe iron meteorite contains thin stingers of retained austenite (taenite) between plates of ferrite (kamacite). These stringers contain microstructures of various Fe-Ni phases called plessite. Plessite has been observed in the Arispe iron meteorite as fine and coarsened pearlitic (lamellar), spheroiditic, and microwidmanstatten a structure. Each of these structures consists of kamacite and a high-Ni unidentified taenite phase, identification of the high-Ni taenite phase can aid in the determination of the Fe-Ni phase diagram. Through TEM observations and EDS analyses of the pearlitic plessite, this high-Ni phase was determined to be tetrataenite, an ordered face-centered cubic phase with ~50% Ni. Furthermore, it was concluded that th...
Several mineral and metallic phases in a sample from the Agpalilik mass of the Cape York iron meteor...
The nakhlite group of martian meteorites found in the Antarctic contain varying abundances of both m...
A Study of Iron Meteorite Microstructure by EBSD and High-Speed AFM S. Moore *a, P.G. Martin a, L. P...
The microstructure of the outer taenite rim and cloudy zone of meteoritic metal was investigated usi...
Plessite is a mixture of body-centered cubic (bcc) kamacite (alpha), face-centered cubic (fcc) taeni...
The IABs represent one of only two groups of iron meteorites that did not form by fractional crystal...
The IABs represent one of only two groups of iron meteorites that did not form by fractional crystal...
Tetrataenite (Fe_Ni_γ" phase) is a unique metallic mineral in meteorites. A magnetic granulometry an...
This thesis reports on the results of investigating Fe-containing minerals in meteorites, with focus...
Tetrataenite is a new meteoritic mineral with ideal formula FeNi, which forms by ordering of Fe and ...
The phase composition of the El Hammami meteorite was investigated by X-ray, magnetostatic, Mössbaue...
Meteorites are perhaps one of the most tangible aspects of outer space. With their irregular, ablate...
The work described in this thesis features the study of planetary materials, including nakhlite mart...
Almahata Sitta (AS) is a polymict breccia mainly composed of variable ureilite lithologies with smal...
Tishomingo is a chemically and structurally unique iron with 32.5 wt.% Ni that contains 20% residual...
Several mineral and metallic phases in a sample from the Agpalilik mass of the Cape York iron meteor...
The nakhlite group of martian meteorites found in the Antarctic contain varying abundances of both m...
A Study of Iron Meteorite Microstructure by EBSD and High-Speed AFM S. Moore *a, P.G. Martin a, L. P...
The microstructure of the outer taenite rim and cloudy zone of meteoritic metal was investigated usi...
Plessite is a mixture of body-centered cubic (bcc) kamacite (alpha), face-centered cubic (fcc) taeni...
The IABs represent one of only two groups of iron meteorites that did not form by fractional crystal...
The IABs represent one of only two groups of iron meteorites that did not form by fractional crystal...
Tetrataenite (Fe_Ni_γ" phase) is a unique metallic mineral in meteorites. A magnetic granulometry an...
This thesis reports on the results of investigating Fe-containing minerals in meteorites, with focus...
Tetrataenite is a new meteoritic mineral with ideal formula FeNi, which forms by ordering of Fe and ...
The phase composition of the El Hammami meteorite was investigated by X-ray, magnetostatic, Mössbaue...
Meteorites are perhaps one of the most tangible aspects of outer space. With their irregular, ablate...
The work described in this thesis features the study of planetary materials, including nakhlite mart...
Almahata Sitta (AS) is a polymict breccia mainly composed of variable ureilite lithologies with smal...
Tishomingo is a chemically and structurally unique iron with 32.5 wt.% Ni that contains 20% residual...
Several mineral and metallic phases in a sample from the Agpalilik mass of the Cape York iron meteor...
The nakhlite group of martian meteorites found in the Antarctic contain varying abundances of both m...
A Study of Iron Meteorite Microstructure by EBSD and High-Speed AFM S. Moore *a, P.G. Martin a, L. P...