Petrologic investigations of martian rocks have been accomplished by mineralogical,
geochemical, and textural analyses from Mars rovers (with geologic context provided by …

The original hydrogen isotope (D/H) ratios of different planetary bodies may indicate where
each body formed in the Solar System. However, geological and atmospheric processes can …

We investigated the transfer of meteorites from Mars to Earth with a combined mineralogical
and numerical approach. We used quantitative shock pressure barometry and …

The 4.1-billion-year-old meteorite Allan Hills 84001 (ALH 84001) may preserve a magnetic
record of the extinct martian dynamo. However, previous paleomagnetic studies have …

Although Mars does not presently appear to have a global dynamo magnetic field, strong
crustal fields have recently been detected by the Mars Global Surveyor above surfaces …

H isotope measurements of carbonate, phosphate, feldspathic and mafic glasses, and post-
stishovite silica phase in the shergottites Zagami, Shergotty, SaU 005, DaG 476, ALHA …

We present the first systematic Micro-Raman spectroscopic investigation of plagioclase of
di# erent degree of shock metamorphism in Martian meteorites. The equilibrium shock …

The thermal histories of Martian meteorite are important for the interpretation of petrologic,
geochemical, geochronological, and paleomagnetic constraints that they provide on the …

Carbonates are predicted to exist on Mars, as they are a common product of the interaction
of CO 2, water, and Fe–Mg silicates over a wide range of conditions. They have been …

The temporal evolution of past martian surface temperatures is poorly known. We used
thermochronology and published noble gas and petrographic data to constrain the …