Exploratour - Evolution of the Solar System

This is an illustration of the Chicxulub impact.
Click on image for full size
NASA/JPL

At this point in planetary history, of every planet and moon with a solid surface was bombarded with the remains of the material which formed them. Even though the solar system was finished forming, there were still probably a lot of smaller planetesimals and debris around, too. The gravity of the large planets would attract nearby planetesimals, which would hit the planets and leave a crater on the planet's surface.


This was the very last stage of the process whereby planetismals swept up material in their paths.

The surfaces of many planets never changed after this point in time. The surface of such a planet bears the record of the fact that it stopped changing by the unchanged appearance of the craters. The planet Mercury, the Moon, Jupiter's moon Callisto, and some portions of Mars bear such an appearance.



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Windows to the Universe, a project of the National Earth Science Teachers Association, is sponsored in part is sponsored in part through grants from federal agencies (NASA and NOAA), and partnerships with affiliated organizations, including the American Geophysical Union, the Howard Hughes Medical Institute, the Earth System Information Partnership, the American Meteorological Society, the National Center for Science Education, and TERC. The American Geophysical Union and the American Geosciences Institute are Windows to the Universe Founding Partners. NESTA welcomes new Institutional Affiliates in support of our ongoing programs, as well as collaborations on new projects. Contact NESTA for more information. NASA ESIP NCSE HHMI AGU AGI AMS NOAA