### Origin of the Moon
Scientists debate how the Moon was formed. Two primary hypotheses have been proposed:
Hypothesis 1
The Moon formed from the debris of a collision between the early Earth and a Mars-sized protoplanet. The impact ejected mostly the silicate-rich outer mantles of both bodies into orbit, where they accreted to form the Moon. Because the iron cores of both bodies merged to remain with Earth, the Moon was left with a very small iron core.
Hypothesis 2
The Moon formed independently in a different region of the solar nebula and was later captured by Earth's gravitational field during a close planetary flyby. This explains why the Moon has a much lower bulk density than Earth, as it formed from materials in a region of the nebula that was naturally depleted of iron.
New Evidence
Analysis of lunar rock samples reveals that the oxygen isotope ratios ( and ) of lunar rocks are identical to those of Earth's mantle. Bodies that form in different regions of the solar nebula generally possess distinct, unique oxygen isotope signatures.
Based on this information, how does the new evidence affect the two hypotheses?
- It supports Hypothesis 1 and weakens Hypothesis 2.Answer
- BIt weakens Hypothesis 1 and supports Hypothesis 2.
- CIt weakens both Hypothesis 1 and Hypothesis 2.
- DIt supports both Hypothesis 1 and Hypothesis 2.