K-Ar and noble gas surface exposure age measurements were carried out on the Windjana sandstone, Kimberley region, Gale Crater, Mars, by using the Sample Analysis at Mars instrument on the Curiosity rover. The sandstone is unusually rich in sanidine, as determined by CheMin X-ray diffraction, contributing to the high KO concentration of 3.09 ± 0.20 wt % measured by Alpha-Particle X-ray Spectrometer analysis. A sandstone aliquot heated to ~915°C yielded a K-Ar age of 627 ± 50 Ma. Reheating this aliquot yielded no additional Ar. A second aliquot heated in the same way yielded a much higher K-Ar age of 1710 ± 110 Ma. These data suggest incomplete Ar extraction from a rock with a K-Ar age older than 1710 Ma. Incomplete extraction at ~900°C is n...
We review the in situ geochronology experiments conducted by the Mars Science Laboratory mission's C...
MSL Curiosity investigated the Windjana sandstone outcrop, in the Kimberley area of Gale Crater, and...
Here we present the isotopic concentrations of He, Ne, Ar, Kr, and Xe for the three Martian meteori...
K-Ar and noble gas surface exposure age measurements were carried out on the Windjana sandstone, Kim...
K-Ar and noble gas surface exposure age measurements were carried out on the Windjana sandstone, Kim...
By combining the Sample Analysis at Mars (SAM) instrument’s capabilities with those of the alpha par...
Following K-Ar dating of a mudstone and a sandstone, a third sample has been dated by the Curiosity ...
Following K-Ar dating of a mudstone and a sandstone, a third sample has been dated by the Curiosity ...
Radiometric age dating of Martian rocks and surfaces at known locations for which crater densities c...
We determined radiogenic and cosmogenic noble gases in a mudstone on the floor of Gale Crater. A K-A...
We determined radiogenic and cosmogenic noble gases in a mudstone on the floor of Gale Crater. A K-A...
We determined radiogenic and cosmogenic noble gases in a mudstone on the floor of Gale Crater. A K-A...
The development of an in-situ geochronology capability for Mars and other planetary surfaces has the...
International audienceThe Martian breccias NWA 7034, NWA 7533, and paired meteorites record events r...
The absolute chronology of Mars is poorly known and as a consequence a key science aim is to perform...
We review the in situ geochronology experiments conducted by the Mars Science Laboratory mission's C...
MSL Curiosity investigated the Windjana sandstone outcrop, in the Kimberley area of Gale Crater, and...
Here we present the isotopic concentrations of He, Ne, Ar, Kr, and Xe for the three Martian meteori...
K-Ar and noble gas surface exposure age measurements were carried out on the Windjana sandstone, Kim...
K-Ar and noble gas surface exposure age measurements were carried out on the Windjana sandstone, Kim...
By combining the Sample Analysis at Mars (SAM) instrument’s capabilities with those of the alpha par...
Following K-Ar dating of a mudstone and a sandstone, a third sample has been dated by the Curiosity ...
Following K-Ar dating of a mudstone and a sandstone, a third sample has been dated by the Curiosity ...
Radiometric age dating of Martian rocks and surfaces at known locations for which crater densities c...
We determined radiogenic and cosmogenic noble gases in a mudstone on the floor of Gale Crater. A K-A...
We determined radiogenic and cosmogenic noble gases in a mudstone on the floor of Gale Crater. A K-A...
We determined radiogenic and cosmogenic noble gases in a mudstone on the floor of Gale Crater. A K-A...
The development of an in-situ geochronology capability for Mars and other planetary surfaces has the...
International audienceThe Martian breccias NWA 7034, NWA 7533, and paired meteorites record events r...
The absolute chronology of Mars is poorly known and as a consequence a key science aim is to perform...
We review the in situ geochronology experiments conducted by the Mars Science Laboratory mission's C...
MSL Curiosity investigated the Windjana sandstone outcrop, in the Kimberley area of Gale Crater, and...
Here we present the isotopic concentrations of He, Ne, Ar, Kr, and Xe for the three Martian meteori...