Impact melts are rocks formed by the intense heat and pressure generated during high-velocity collisions between celestial bodies, such as asteroids or comets, and planets or moons. These collisions can produce temperatures exceeding thousands of degrees Celsius, melting the rock and forming a unique type of rock known as impact melts. Impact melts can be identified by their characteristic textures, which often include glassy, vesicular, or brecciated features. They can contain a mix of materials from the target rock and the impacting object, and may also exhibit shock features such as planar deformation features (PDFs) or high-pressure minerals. Studying impact melts can provide valuable insights into the processes and effects of impact events on planetary bodies, such as the Moon, Mars, or Earth. They can help researchers understand the dynamics of impact processes, the formation of impact craters, and the distribution of impact-related materials in the solar system. Additionally, impact melts can provide clues about the composition and structure of the impactors themselves, shedding light on the history and evolution of our solar system.