The Earth's core is significantly hotter than its surface, leading to a heat loss through convection and radiation. The heat flux from the Earth's interior is approximately 0.008 W/m2, which is minimal compared to other heat sources. Historical calculations by physicist William Thomson in 1862 estimated the Earth's age to be between 20 million and 400 million years, based on the cooling of a molten Earth, but did not consider radioactive decay or convection, which are crucial for heat retention and transfer. In contrast, Venus lacks plate tectonics, leading to a different heat escape mechanism, where the mantle heats up until it causes resurfacing events. Discussions also touch on the surface conditions of Venus, questioning whether it is molten and addressing the challenges of obtaining accurate data from its harsh environment. The imagery from past probes, like the Venera missions, highlights the difficulties in capturing clear images of Venus's surface due to extreme temperatures and pressures.