TY - JOUR
T1 - Evaporative fractionation of zinc during the first nuclear detonation
AU - Day, James M.D.
AU - Moynier, Frédéric
AU - Meshik, Alex P.
AU - Pradivtseva, Olga V.
AU - Petit, Donald R.
N1 - Publisher Copyright:
© 2017 The Authors, some rights reserved.
PY - 2017/2
Y1 - 2017/2
N2 - Volatile element and compound abundances vary widely in planets and were set during the earliest stages of solar system evolution. Experiments or natural analogs approximating these early conditions are limited. Using silicate glass formed from arkosic sands during the first nuclear detonation at the Trinity test site, New Mexico, we show that the isotopes of zinc were fractionated during evaporation. The green silicate glasses, termed “trinitite,” show +0.5 ± 0.1%/atomic mass unit isotopic fractionation from ~200 m to within 10 m of ground zero of the detonation, corresponding to an fractionation factor between 0.999 and 0.9995. These results confirm that Zn isotopic fractionation occurs through evaporation processes at high temperatures. Evidence for similar fractionations in lunar samples consequently implies a volatile-depleted bulk Moon, with evaporation occurring during a giant impact or in a magma ocean.
AB - Volatile element and compound abundances vary widely in planets and were set during the earliest stages of solar system evolution. Experiments or natural analogs approximating these early conditions are limited. Using silicate glass formed from arkosic sands during the first nuclear detonation at the Trinity test site, New Mexico, we show that the isotopes of zinc were fractionated during evaporation. The green silicate glasses, termed “trinitite,” show +0.5 ± 0.1%/atomic mass unit isotopic fractionation from ~200 m to within 10 m of ground zero of the detonation, corresponding to an fractionation factor between 0.999 and 0.9995. These results confirm that Zn isotopic fractionation occurs through evaporation processes at high temperatures. Evidence for similar fractionations in lunar samples consequently implies a volatile-depleted bulk Moon, with evaporation occurring during a giant impact or in a magma ocean.
UR - http://www.scopus.com/inward/record.url?scp=85020380814&partnerID=8YFLogxK
U2 - 10.1126/sciadv.1602668
DO - 10.1126/sciadv.1602668
M3 - Article
C2 - 28246647
AN - SCOPUS:85020380814
SN - 2375-2548
VL - 3
JO - Science Advances
JF - Science Advances
IS - 2
M1 - e1602668
ER -