The earth has a bulk density of 5.5 grams per cubic centimeter. This
density reflects the composition of material at the location in
the solar system where the Earth was assembled via accretion. Logically
one would therefore expect the moon to the have the same density.
However,the moon has a density of 3.3 grams per cubic centimeter. Is this a problem? Yes! This implies
a special formation history for the Moon which is difficult to understand
from first principles.
The Origin of the Moon:
Until recently, this was not understood. The moon has long been an anomaly because its mass compared to the earth is 1/80 and there is very large for a planetary satellite
Possibilities for Lunar Origin:
The above 3 scenarios for lunar formation are all physically implausible so why is the moon there?
Let's imagine the following sequence:
Here is the Sequence if there was an impact
![]() | Step 1: The Mars planetisimal is poised to strike the molten protoplanet earth which has been differentiated. |
![]() | Step 2: The impact into the molten earth sends large molten lumps of debris out of the earth - mostly from the middle layers of the differeniated earth. |
![]() | Step 3: The debris ring of molten ejecta coalesces, by accretion, into a single object. The density of that object would be similar to the density of the middle layers of the earth (e.g. about 3.5 grams/cc). In computer numerical models, this coalescence occurs fast, on a timescale of about 100 million years. |
The problem with this scenario is that the probability of a direct collision is small. However, the same result can occur if there is not a direct collision but instead there is a close passage by the Mars sizes object.
Here is the Sequence if it was a close passage:
![]() | This shows the encounter path. |
![]() | Step 1: A tidal force is exerted on the molten earth which causes an obvious deformation. |
![]() | Step 2: The deformation actually separates from the earth initially as a whole molten blob whose composition again reflects the middle layers of the Earth |
![]() | Step 3: However, this molten blob is gravitationally perturbed by the combined forces of the Earth and the still near Mars size object so it distengrates into a debris ring. |
![]() | After a 100 million years or so, the debris ring has coalesced into the moon, and the Earth has cooled so that water vapor in its atmosphere (combined with bombardment by comets) has produced the oceans. |
Since the moon formed from the condensation of a debris ring in relatively near-earth orbit, the moon was initially quite close to the earth. At this time (4.6 billion years ago) the earth was rotating quite rapidly (about once every 5 hours). The nearby moon exerted large tidal forces on the spinning earth causing it to slow down. This process continues to day. To conserve total system angular momentum, the response of the moon is then to move farther away from the earth.