A rock called an impactite
It is made when there is an amazingly crazy amount of force and heat put on rcks that changes it's arrangement to make a new rock. usually from big meteorite impact craters.
Gordon R. Osinski has written: 'Impact cratering' -- subject(s): Impact craters, Cratering
The Moon and Mercury are two bodies in our solar system that show evidence of heavy cratering. Their surfaces are covered with numerous impact craters created by collisions with meteoroids and other celestial bodies over billions of years. This cratering is a result of their limited atmosphere and lack of geological processes to erase the impact scars.
Yes, but there are not so many craters, per square kilometer,as on the Moon.
i cant tell what your question is really, but im assuming youre asking "how did craters impact earth?". the answer is either meteors, earthquakes, or erosion.
The four processes that shaped the rocky crust of terrestrial planets are volcanism, tectonism (such as plate tectonics), impact cratering, and erosion/weathering. These processes have played key roles in shaping the landscapes and surface features of planets like Earth, Mars, Venus, and Mercury.
Impact cratering from asteroids and comets is the primary geological process that has shaped the surface of the moon. Volcanic activity, although minimal, has also contributed to the formation of lunar features like lava plains and small volcanic domes. Additionally, tectonic forces such as moonquakes and faulting have played a role in shaping the moon's surface.
The resulting scar from asteroid or comet strikes is called an impact crater. These craters are formed when the meteorite collides with the surface of a planet or moon, causing a depression in the ground.
No way to tell as the entire planet is shrouded in clouds. But, having said that, many of its moons (e.g., Titania and Oberon) have impact craters. So it's not a far reach to believe that Uranus itself would have impact craters in its rocky central core.
Cratering rates serve as a useful estimate of surface age. Surface features can be reworked primarily through water erosion, but also by wind erosion and faulting (earthquakes), volcanoes, and crustal movement. Mars and Jupiter being closer to the asteroid belt, the rate of cratering may be slightly higher there. Our moon's surface appears to be quite old, judging by the number of impact craters it has. Earth would have even more, being a bigger target, but earth impacts have been largely eroded and subducted over the course of hundreds of millions of years.
Impact cratering: Collisions with asteroids or comets create craters on the surface. Tectonism: Movement of the planet's lithosphere causes features like mountains and valleys. Erosion: Weathering and transportation of materials by wind, water, or ice alters the landforms. Volcanism: Eruptions of molten rock from the planet's interior build up volcanic features like mountains and lava flows.
Two events that can result in cataclastic metamorphism are faulting, which involves the grinding and crushing of rocks along a fault zone, and impact cratering, where the intense pressure and heat generated by a meteorite impact cause rocks to be deformed and recrystallized.
The four stages of planetary development are accretion, differentiation, impact cratering, and tectonics. During accretion, dust and gas combine to form planetesimals that eventually collide to form a planet. Differentiation occurs as heavy materials sink to the planet's core and lighter materials rise to the surface. Impact cratering involves the formation of craters due to collisions with other celestial bodies. Tectonics refers to the processes that shape the planet's surface, such as plate movements and volcanic activity.