Linked from

The 21 pages that link to Impact cratering, each with the reason it gives.

• Planetary scienceRelated: Crater populations preserve evidence of surface ages and impact histories.

• Planetary geologyRelated: Crater shapes and densities expose impact histories and help estimate surface ages.

• MercuryRelated: Mercury’s densely cratered crust preserves a long record of impacts.

• U–Pb datingRelated: U–Pb dates can constrain when impact-related minerals crystallized or were reset.

• Lunar highlandsRelated: Billions of years of impacts created the highlands’ dense crater record.

• MeteoroidRelated: Meteoroids that reach the surface can create small impact craters.

• Asteroid collisionRelated: Collisions can excavate craters when the impact does not destroy either asteroid.

• Geology of MarsRelated: Crater patterns reveal surface ages and the history of impacts on Mars.

• Geological history of EarthRelated: Impacts shaped early Earth and left evidence in surviving rocks and craters.

• Geology of MercuryRelated: Impacts dominate Mercury’s visible terrain and preserve a record of its geological past.

• Geology of the MoonRelated: Impacts dominate lunar surface formation and excavate material from different depths.

• Geology of VenusRelated: Venus’s crater distribution constrains surface age and possible episodes of widespread resurfacing.