Text 1
For decades, planetary scientists have maintained that the bulk of Earth’s water was delivered by carbonaceous chondrites during the late accretion phase of planetary formation. Proponents of this model point to the deuterium-to-hydrogen () ratios of these water-rich meteorites, which are virtually identical to the isotopic signature observed in Earth's modern surface oceans, suggesting a post-formation meteoritic origin.
Text 2
Geochemist Wu and colleagues propose that a substantial fraction of Earth's water instead originated from the primordial solar nebula. The team analyzed deep-mantle rock samples, which yield a significantly lower ratio than that of surface reservoirs. Wu argues this low ratio reflects nebular hydrogen directly absorbed by the early magma ocean, meaning modern ocean values represent a hybrid mixture rather than a purely chondritic source.
Based on the passages, is the statement that geochemist Wu and colleagues would characterize the isotopic match described in Text 1 as insufficient evidence to establish that Earth's water was delivered entirely after the planet's initial formation true or false?
Answer: Answer