ETH Zurich researchers have pinned down where Earth came from. The answer raises a harder question.
In a paper published March 27 in Nature Astronomy, Paolo Sossi and Dan Bower analyzed 10 nucleosynthetic isotope systems across planetary bodies and meteorites. Their conclusion: Earth formed almost entirely from material native to the inner Solar System. Less than 2 percent of its mass came from beyond Jupiter's orbit. Previous estimates had put that figure between 6 and 40 percent.
The method matters. Earlier work relied on one or two isotope systems. Sossi and Bower used 10, which tightens the error bars enough to rule out significant outer Solar System contribution. They also applied Bayesian hierarchical statistical methods — tools more common in other fields but rarely used in geochemistry. The Earth assembled from inner Solar System material whose composition stayed remarkably constant throughout accretion.
The researchers compared existing isotope ratio data from a range of meteorites, including samples from Mars and the asteroid Vesta, against Earth. Non-carbonaceous meteorites, which form exclusively in the inner Solar System, match Earth's composition closely. Carbonaceous meteorites, which originate in the outer Solar System and carry more water and carbon, do not. This is the compositional fingerprint the researchers were looking for, and they found it.
The finding complicates a leading explanation for Earth's water. The comet-delivery hypothesis held that icy bodies from beyond Jupiter delivered water during a late heavy bombardment. If less than 2 percent of Earth's material came from the outer Solar System, that story breaks down. The water had to be there already.
This is the part the researchers cannot yet explain. Water and volatile elements must have been present in the inner Solar System during Earth's accretion — in a region hot enough that ice should not have been stable. How volatiles survived in that environment long enough to become incorporated into the planet is an open problem. Sossi and Bower plan to investigate why there was sufficient water in the hot inner Solar System to form Earth's oceans. They do not have an answer yet.
Jupiter, the researchers note, acted as a material barrier. Its gravity tore a gap in the protoplanetary disk orbiting the young Sun, preventing outer Solar System reservoirs from mixing into the inner disk where Earth formed. The composition of Vesta and Mars matches what the isotope data predicts. Venus and Mercury likely do too, though no rock samples from either planet exist to confirm it.
The result narrows where scientists need to look for explanations of Earth's habitability. Volatiles were present during accretion. The mechanism that delivered them is not the one researchers had assumed. That gap is now the live question.
"Our calculations make it clear: the building material of the Earth originates from a single material reservoir," Sossi said. His colleague Bower added: "We were truly astonished to find that the Earth is composed entirely of material from the inner Solar System distinct from any combination of existing meteorites."
The paper is Sossi PA, Bower DJ. Homogeneous accretion of the Earth in the inner Solar System. Nature Astronomy (2026).