Volcanology of Venus
The surface of Venus is dominated by volcanic features and has more volcanoes than any other planet in the Solar System. It has a surface that is 90% basalt, and about 65% of the planet consists of a mosaic of volcanic lava plains, indicating that volcanism played a major role in shaping its surface. There are more than 1,000 volcanic structures and possible periodic resurfacing of Venus by floods of lava. The planet may have had a major global resurfacing event about 500 million years ago, from what scientists can tell from the density of impact craters on the surface. Venus has an atmosphere rich in carbon dioxide, with a density that is 90 times greater than Earth's atmosphere.
Venus Atmospheric Maneuverable Platform
The aircraft is proposed to be launched as a secondary payload on another spacecraft mission to Venus, probably on Russia's Venera-D in 2026. During daytime, VAMP would be able to make continuous science measurements, while at night the vehicle would descend to 50 km altitude where it would be fully buoyant, remain at a lower-power state, and still perform modest science measurements at the float altitude. The lower cloud layer of Venus, located between 47.5 and 50.5 km altitude, is acidic, but it is considered by some astrobiologists to be a target for exploration due to the favorable conditions for microbial life, including moderate temperatures and pressures (∼60 °C and 1 atm).