When we discussed the formation of the moon via the "Giant Impact
Theory" we found that the model requires a collision between the early Earth
and a Mars-sized protoplanet. The collision splashed off the material from
the outer parts of the Earth which gathered together at a distance from the
Earth to make up our moon.
Now, having learned a bit about ring systems and tidal effects in the Jovian
planets, you can explore this model a bit further.
- How far away from the surface of the Earth did the material have to get
so that it could collect together under its own gravity?
-
Why could it have not formed any closer?
-
What do you think happened to the material that was inside this distance
after the initial collision?