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Studying the mechanisms of internal heat loss on different planets is an important task for understanding the evolution of the Solar System and the Earth in particular. The object of this study is the volcanism of Venus. This paper describes the geological structure and history of the development of the volcano Samodiva Mons, located in the V-29 quadrangle on Venus. The results of mapping lava flows and graben-fissure systems (underlain by dikes) are presented.