Abstract The Colour and Stereo Surface Imaging System (CaSSIS) is the main imaging
system onboard the European Space Agency's ExoMars Trace Gas Orbiter (TGO) which was …

BepiColombo has a larger and in many ways more capable suite of instruments relevant for
determination of the topographic, physical, chemical and mineralogical properties of …

BepiColombo is an interdisciplinary mission to explore Mercury, the planet closest to the
sun, carried out jointly between the European Space Agency and the Japanese Aerospace …

We present a global survey of candidate pyroclastic deposits on Mercury, derived from
images obtained during MESSENGER flybys 1–3 that provided near-global coverage at …

In preparation for the ESA/JAXA BepiColombo mission to Mercury, thematic working groups
had been established for coordinating the activities within the BepiColombo Science …

Explosive volcanism on the surface of planet Mercury is visible through the pyroclastic
deposits that surround morphologic features often identified as the vent. Those deposits are …

The increased volume, spatial resolution, and areal coverage of high-resolution images of
Mars over the past 15 years have led to an increased quantity and variety of small-scale …

To detect the mineral diversity of a planet's surface, it is essential to study the spectral
variations over a broad wavelength range at relevant simulated laboratory conditions. The …

Surfaces of atmosphereless planetary bodies, including the Moon and Mercury, are covered
with regolith. Regolith-related processes define surface morphology at scales of meters and …

Volcanism on Mercury has been indisputably identified at various locations on the surface,
by means of both effusive and explosive volcanism. Its characterization is crucial to …