Using radar data from NASA’s Magellan mission, planetary scientists have detected volcanic-related flow features in two different regions of Venus: on the western flank of Sif Mons and in western Niobe Planitia. This image shows the Sif Mons area with the active volcanic region highlighted in red. Image credit: Davide Sulcanese, IRSPS – Università d’Annunzio. Venus’ thick atmosphere has made it difficult to directly observe the surface...
