1999/11/10 by M. Ozima, F. A. Podosek · 3 citations
Earth and Planetary Sciences · Environmental Science · Physics and Astronomy · #Abundance (ecology) #Astro and Planetary Science #Astrobiology #Astronomy #Atmosphere (unit) #Atomic physics #Cosmochemistry #Earth (classical element) #Geology and Paleoclimatology Research #Isotope #Isotope Analysis in Ecology #Meteorite #Noble gas #Nuclear physics #Physics #Radiogenic nuclide #Radionuclide #Solar System #Xenon
paper · pdf · doi:10.1029/1999jb900257
openalex publication_date 1999/11/10 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/23
The Earth's atmosphere contains excesses of 129 Xe and 136 Xe from decay of the short‐lived radionuclides 129 I and 244 Pu, respectively. The inferred abundances of these radionuclides are substantially less than those in meteorites, nominally indicating that Earth as a planet did not form until more than 100 Myr later than the solar system as a whole, an interval rather longer than that suggested by other lines of evidence. From the comparison of elemental abundance ratios between atmospheric (assumed to approximate the total terrestrial noble gas inventory) and solar noble gases, we conclude that ∼90% of Earth's primordial Xe is missing from the atmosphere. When account is taken of the radiogenic Xe that is likely missing as well, the 129 I‐ 244 Pu formation interval of Earth may be reduced significantly, down to about 50–70 Myr.