Collisions are one of the key processes shaping planetary systems. Asteroid families are
outcomes of such collision still identifiable across our solar system. The families provide a …

We review the evidence for buried ice in the asteroid belt; specifically the questions around
the so-called Main Belt Comets (MBCs). We summarise the evidence for water throughout …

Context. Until recently, the 3D shape, and therefore density (when combining the volume
estimate with available mass estimates), and surface topography of the vast majority of the …

Context. The classification of the minor bodies of the Solar System based on observables
has been continuously developed and iterated over the past 40 yr. While prior iterations …

In this work we identify spectral similarities between asteroids and meteorites. Using spectral
features such as absorption bands and spectral curvature, we identify spectral matches …

Context. The third data release by the Gaia mission of the European Space Agency (DR3) is
the first release to provide the community with a large sample of observations for more than …

Context. The source regions of ordinary chondrites (~ 80% of all falls) and large S-type near-
Earth objects (NEOs;~ 30%) have recently been identified with three young asteroid families …

Anhydrous pyroxene-rich interplanetary dust particles (IDPs) have been proposed as
surface analogs for about two-thirds of all C-complex asteroids. However, this suggestion …

Context. The population of near-Earth asteroids (NEAs) shows a large variety of objects in
terms of physical and dynamical properties. They are subject to planetary encounters and to …

The relationship between the near-Earth objects (3200) Phaethon and (155140) 2005 UD is
unclear. While both are parents to meteor showers (the Geminids and Daytime Sextantids …