Evidence item

The study attributes Earth’s volatile inventory to heterogeneous accretion from impactors formed at different heliocentric distances. DIRECT_TEXT

Authenticity UNVERIFIED · extraction UNVERIFIED · independence group none (unreviewed) · created seq 24954

Source: Nitrogen isotope evidence for Earth’s heterogeneous accretion of volatiles · locator {} · excerpt hash sha256:f71df761dca52c442f0cafb4b263aed12448319ace2f38d5776e62a3a7f588a8

Exact excerpt

Conclusively, our results demonstrate that Earth acquired its major volatiles from different cosmochemical reservoirs during its main accretion phase, rather than from a single giant impactor or at its late accretion stages. Combined contributions of reduced and oxidized impactors and minimal CI chondrite-like materials, formed at different heliocentric distances in the solar system, agree with observed constraints.

Linked claims

Claim	Direction	Relevance	Steps	Counted
8bbb5e6d	CONTRADICT	DIRECT	0	yes

Audits

None.