The origin of Earth’s volatiles has been attributed to a late
addition of meteoritic material after core-mantle differentiation. The nature
and consequences of this 'late veneer' are debated, but may be
traced by isotopes of the highly siderophile, or iron-loving, and volatile
element selenium. Here we present high-precision selenium isotope data for
mantle peridotites, from double spike and hydride generation multi-collector
inductively coupled plasma mass spectrometry. These data indicate that the
selenium isotopic composition of peridotites is unaffected by petrological
processes, such as melt depletion and melt-rock reaction, and thus a narrow range
is preserved that is representative of the silicate Earth. We show that selenium
isotopes record a signature of late accretion after core formation and that this
signature overlaps only with that of the CI-type carbonaceous chondrites. We
conclude that these isotopic constraints indicate the late veneer originated
from the outer Solar System and was of lower mass than previously estimated.
Thus, we suggest a late and highly concentrated delivery of volatiles enabled
Earth to become habitable.