Final answer:
Meteorites can come from the cores of asteroids, comets, Mars, and even the Moon, serving as key scientific evidence of the solar system's early composition. (Option E),
Step-by-step explanation:
Meteorites can indeed come from various sources within our solar system. They are debris from space that survive the journey through Earth's atmosphere and make contact with our planet's surface. Most meteorites are primitive stones, which are often dated to the very origin of the solar system, approximately 4.5 billion years ago. They are broadly classified based on their composition as irons, stony-irons, or stones. Specifically, carbonaceous meteorites can contain organic molecules and are seen as important scientific evidence of the early solar system's makeup.
Meteorites have been known to come from the cores of asteroids, some of which can be differentiated or fragmented due to collisions. The information gives us valuable insights into the original composition of these celestial bodies, making them akin to chemical fossils. While many meteorites originate from asteroids, others are also found to come from comets, Mars, and even the Moon. Meteor showers and observed meteorite falls offer opportunities for scientists to collect and study these extraterrestrial materials. (Option E),