In recent years, there is a growing interest in small satellites for deep space exploration. The
current approach for planetary navigation is based on ground-based radiometric tracking. A …

In this work we discuss various selected mission concepts addressing Venus evolution
through time. More specifically, we address investigations and payload instrument concepts …

Extreme temperature and pressure conditions on the surface of Venus present formidable
technological challenges against performing ground‐based seismology. Efficient coupling …

Barometers floating on high‐altitude balloons in the relatively clement cloud layer on Venus
could detect and characterize acoustic waves generated by seismic activity, avoiding the …

Altitude-controlled balloons hold great promise for performing high-priority scientific
investigations of Venus's atmosphere and geological phenomena, including tectonic and …

The Akatsuki instrument LIR measured an unprecedented wave feature at the top of
Venusian cloud layer. Stationary bow-shape waves of thousands of kilometers large lasting …

Seismology on Venus has long eluded planetary scientists due to extreme temperature and
pressure conditions on its surface, which most electronics cannot withstand for mission …

The measurements of acoustic waves created by a quake are of great interest for planets
with hot and dense atmospheres, like Venus, because surface deployments of …

A numerical simulation of the upper atmosphere of Venus is carried out with an improved
version of the Institut Pierre-Simon Laplace (IPSL) full-physics Venus General Circulation …

Venus is essential to our understanding of the evolution and habitability of Earth-size
planets throughout the galaxy. The selection of the VERITAS, EnVision, and DAVINCI …