Add to ORKGGenesis, a NASA sample return mission, collected solar wind (SW) in space for 2.5 years for precise elemental and isotopic analyses. SW matter originates from the photosphere and outer convective zone of the Sun and serves as a proxy of solar nebula composition. One major objective of Genesis was to determine solar abundances and isotopic composition of volatile elements. The solar composition of noble gases is difficult to determine as they are depleted in primitive meteorites and also not detectable in the photospheric spectrum due to their high excitation energies
AbstractThe fluence and isotopic composition of solar wind xenon have been determined from silicon c...
The Genesis mission captured Solar Wind (SW) and delivered it to Earth for laboratory analyses. Due ...
The Genesis mission captured Solar Wind (SW) and delivered it to Earth for laboratory analyses. Due ...
Genesis, a NASA sample return mission, collected solar wind (SW) in space for 2.5 years for precise...
Knowledge of the composition of the solar nebula is necessary in understanding how the solar system ...
We present the elemental and isotopic composition of noble gases in the bulk solar wind collected by...
The Genesis Discovery mission returned solar matter in the form of the solar wind with the goal of o...
The Genesis Discovery Mission returned samples of solar matter by exposing ultrapure materials to t...
The Sun's composition is a proxy for that of the solar nebula, which serves as a reference baseline...
The Sun's composition is a proxy for that of the solar nebula, which serves as a reference baseline...
NASA's Genesis mission was flown to capture samples of the solar wind and return them to the Earth f...
Solar abundances are important to planetary science since the prevalent model assumes that the compo...
Solar abundances are important to planetary science since the prevalent model assumes that the compo...
One of the major goals of the Genesis Mission was to refine our knowledge of the isotopic compositio...
We discuss data of light noble gases from the solar wind implanted into a metallic glass target flow...
AbstractThe fluence and isotopic composition of solar wind xenon have been determined from silicon c...
The Genesis mission captured Solar Wind (SW) and delivered it to Earth for laboratory analyses. Due ...
The Genesis mission captured Solar Wind (SW) and delivered it to Earth for laboratory analyses. Due ...
Genesis, a NASA sample return mission, collected solar wind (SW) in space for 2.5 years for precise...
Knowledge of the composition of the solar nebula is necessary in understanding how the solar system ...
We present the elemental and isotopic composition of noble gases in the bulk solar wind collected by...
The Genesis Discovery mission returned solar matter in the form of the solar wind with the goal of o...
The Genesis Discovery Mission returned samples of solar matter by exposing ultrapure materials to t...
The Sun's composition is a proxy for that of the solar nebula, which serves as a reference baseline...
The Sun's composition is a proxy for that of the solar nebula, which serves as a reference baseline...
NASA's Genesis mission was flown to capture samples of the solar wind and return them to the Earth f...
Solar abundances are important to planetary science since the prevalent model assumes that the compo...
Solar abundances are important to planetary science since the prevalent model assumes that the compo...
One of the major goals of the Genesis Mission was to refine our knowledge of the isotopic compositio...
We discuss data of light noble gases from the solar wind implanted into a metallic glass target flow...
AbstractThe fluence and isotopic composition of solar wind xenon have been determined from silicon c...
The Genesis mission captured Solar Wind (SW) and delivered it to Earth for laboratory analyses. Due ...
The Genesis mission captured Solar Wind (SW) and delivered it to Earth for laboratory analyses. Due ...