Spacecraft observations revealed that rocks on carbonaceous asteroids, which constitute
the most numerous class by composition, can develop millimeter-to-meter-scale fractures …

Spacecraft missions have observed regolith blankets of unconsolidated subcentimetre
particles on stony asteroids,–. Telescopic data have suggested the presence of regolith …

Aims. We want to find the distribution of initial conditions that best reproduces disc
observations at the population level. Methods. We first ran a parameter study using a 1D …

The asteroid (16) Psyche is the largest of the M-type asteroids, which have been
hypothesized to be the cores of disrupted planetesimals and the parent bodies of the iron …

Context. We are in an era of large catalogs and, thus, statistical analysis tools for large data
sets, such as machine learning, play a fundamental role. One example of such a survey is …

Planet formation simulations are capable of directly integrating the evolution of hundreds to
thousands of planetary embryos and planetesimals as they accrete pairwise to become …

Failure modes of lunar boulders depend both on rheology and the erosion agents acting in
the lunar surface environment. Here, we address the failure modes of lunar boulders and …

Abstract Main‐belt asteroid (16) Psyche is the largest M‐type asteroid, a class of object
classically thought to be the metal cores of differentiated planetesimals and the parent …

Deriving thermophysical properties such as thermal inertia from thermal infrared
observations provides useful insights into the structure of the surface material on planetary …

The thermal conductivity of granular planetary regolith is strongly dependent on the porosity,
or packing density, of the regolith particles. However, existing models for regolith thermal …