### Origin of Earth's Water
Two hypotheses address the origin of Earth's surface oceans.
Hypothesis 1
During Earth's accretion from planetesimals in the inner solar nebula, the high temperatures from gravitational collapse and radioactive decay vaporized all local water. Because Earth's early gravitational field was too weak to retain these light volatile gases, this water vapor escaped into space, leaving the planet completely dry. Subsequently, during the Late Heavy Bombardment ( to billion years ago), water was delivered to Earth's surface by carbonaceous chondrite meteorites. These meteorites are rich in water (up to by weight) and possess a deuterium-to-hydrogen () ratio () that is identical to that of Earth's modern oceans.
Hypothesis 2
Earth's water is primordial, originating from hydrated silicate minerals within the local planetesimals that accreted to form the planet. During the rapid accretion process, Earth's gravity was strong enough to retain the steam outgassed from its molten interior. Deep mantle reservoirs, insulated from surface vapor loss, preserved this primordial water. The ratio of this mantle water is lower () than that of modern surface water. Tectonic recycling and the preferential escape of lighter hydrogen isotopes to space over billions of years have gradually increased the surface ratio to its modern value of .
According to the passage, Hypothesis 1 and Hypothesis 2 differ fundamentally in their assumptions regarding which of the following?
- Whether Earth's gravitational field during the accretion phase was strong enough to prevent outgassed water vapor from escaping into spaceAnswer
- BWhether the deuterium-to-hydrogen ratio of modern ocean water is approximately
- CWhether carbonaceous chondrites delivered water during the Late Heavy Bombardment
- DWhether tectonic recycling of surface water can alter the isotopic composition of the mantle over geological time