Superheated Surfaces: Venus' Extreme Temperatures Exploration скачать в хорошем качестве

Superheated Surfaces: Venus' Extreme Temperatures Exploration

The Venusian environment poses a significant challenge for exploration. Missions to Venus revealed a composition dominated by CO2, with trace amounts of sulfur dioxide, nitrogen oxides, and even water vapor (less than 1% at the surface). Despite its slow rotation period of 243 Earth days, Venus exhibits supersonic winds that whip around the planet at speeds up to 360 km/h (224 mph) in its upper atmosphere. The driving mechanism behind these powerful winds remains a subject of active scientific research. Current theories propose a combination of solar heating and atmospheric density variations. Visualisations of Venus planet and voice — by iGadgetPro Credit for real RAW-images of Venus: NASA/JPL-Caltech| nasa.gov All NASA's RAW-images were colorized, processed and edited by iGadgetPro #Venus #venus4k #venusplanet #climatescience #planetaryscience #atmosphericdynamics