Fossil track studies in several meteorites and in lunar dust show that super-heavy (Z > 110) transuranic elements were indeed present when these objects solidified
The Earth-Moon system likely formed as a result of a collision between two large planetary objects. ...
International audiencePlanetary formation models show that terrestrial planets are formed by the acc...
The notion of a dry Moon has recently been challenged by the discovery of high water contents in lun...
Investigations of recordable lengths (maximum etchable lengths) of fossil tracks in meteorites and i...
Search and identification of superheavy elements (SHE) of Z≥110 in a nature were carried out till no...
Meteorites provide a sample of Solar System bodies and so constrain the types of objects that have c...
The main goal of the present work is the search for and identification of relatively stable nuclei o...
We report data for 14 mainly labile trace elements (Ag, Au, Bi, Cd, Cs, Ga, In, Rb, Sb, Se, Te, Tl, ...
New approaches for investigation of relatively stable nuclei of super heavy element (SHE) (Z > 110) ...
Siderophilic element concentrations are high in sediments from the Cretaceous-Tertiary boundary. An ...
Neutron activation analyses of Ag, Au, Bi, Cd, Co, Cs, Ga, In, Rb, Sb, Se, Te, Tl, U and Zn in whole...
A new combined rhenium-osmium– and platinum-group element data set for basalts from the Moon establi...
Genetic contributions to the final stages of planetary growth, including materials associated with t...
A comprehensive survey is presented of five years work on the question of whether the so-called “org...
Recent high-precision measurements of the isotopic composition of lunar rocks demonstrate that the b...
The Earth-Moon system likely formed as a result of a collision between two large planetary objects. ...
International audiencePlanetary formation models show that terrestrial planets are formed by the acc...
The notion of a dry Moon has recently been challenged by the discovery of high water contents in lun...
Investigations of recordable lengths (maximum etchable lengths) of fossil tracks in meteorites and i...
Search and identification of superheavy elements (SHE) of Z≥110 in a nature were carried out till no...
Meteorites provide a sample of Solar System bodies and so constrain the types of objects that have c...
The main goal of the present work is the search for and identification of relatively stable nuclei o...
We report data for 14 mainly labile trace elements (Ag, Au, Bi, Cd, Cs, Ga, In, Rb, Sb, Se, Te, Tl, ...
New approaches for investigation of relatively stable nuclei of super heavy element (SHE) (Z > 110) ...
Siderophilic element concentrations are high in sediments from the Cretaceous-Tertiary boundary. An ...
Neutron activation analyses of Ag, Au, Bi, Cd, Co, Cs, Ga, In, Rb, Sb, Se, Te, Tl, U and Zn in whole...
A new combined rhenium-osmium– and platinum-group element data set for basalts from the Moon establi...
Genetic contributions to the final stages of planetary growth, including materials associated with t...
A comprehensive survey is presented of five years work on the question of whether the so-called “org...
Recent high-precision measurements of the isotopic composition of lunar rocks demonstrate that the b...
The Earth-Moon system likely formed as a result of a collision between two large planetary objects. ...
International audiencePlanetary formation models show that terrestrial planets are formed by the acc...
The notion of a dry Moon has recently been challenged by the discovery of high water contents in lun...
DOI
Add to ORKG