Исследователи обобщили все данные о Русской планете
The main idea of the text is that the surface of Venus, which is characterized by volcanoes and tectonic formations along with unique features like tesserae and coronae, is relatively young, forming only 2.5-3 billion years ago. This is later than the surface evolution of Mars and Mercury. The research, conducted by Russian scientists in collaboration with international colleagues, suggests that Venus has undergone significant geological changes in its recent history.
