A systematic survey of 161 known and postulated minerals originating on Mars points to 20
different mineral‐forming processes (paragenetic modes), which are a subset of formation …

Mars' crustal magnetic field holds information on the planet's interior evolution and exterior
processes that have modified the crust. Crustal magnetization records an ancient dynamo …

Highly siderophile element abundances and Os isotopes of nakhlite and chassignite
meteorites demonstrate that they represent a comagmatic suite from Mars. Nakhlites …

The formation and differentiation of the crust of Mars in the first tens of millions of years after
its accretion can only be deciphered from incredibly limited records. The martian breccia …

The transition from mafic to felsic upper continental crust (UCC) is crucial to habitability of
Earth, and may be related to the onset of plate tectonics. Thus, defining when this crustal …

Titanium and Fe isotopic compositions of lavas from a calc-alkaline differentiation suite and
corresponding mineral separates from the Rindjani Volcano, Indonesia show that Fe and Ti …

Long-lived hydrothermal systems are prime targets for astrobiological exploration on Mars.
Unlike magmatic or impact settings, radiogenic hydrothermal systems can survive for> 100 …

Life cannot emerge on a planet or moon without the appropriate electrochemical
disequilibria and the minerals that mediate energy-dissipative processes. Here, it is argued …

The terrestrial planets endured a phase of bombardment following their accretion, but the
nature of this late accreted material is debated, preventing a full understanding of the origin …

The constraint of Sn isotope composition of the Earth's mantle is the prerequisite for
understanding planet formation with Sn isotopes and Sn isotope fractionation in terrestrial …