eEarth, 2, 43-49, 2007
www.electronic-earth.net/2/43/2007/
doi:10.5194/ee-2-43-2007
© Author(s) 2007. This work is licensed under the
Creative Commons Attribution-NonCommercial-ShareAlike 2.5 License.
 
08 Oct 2007
Noble gas signature of the Late Heavy Bombardment in the Earth's atmosphere
B. Marty1 and A. Meibom2
1Centre de Recherches Pétrographiques et Géochimiques, Nancy Universités, Nancy, France
2Muséum National d'Histoire Naturelle, Paris, France

Abstract. The Lunar cratering record is consistent with the occurrence of a late heavy bombardment (LHB), which marked the end of terrestrial planet accretion 3.8 billion years ago. However, clear evidence of a LHB on Earth has not yet been identified. Based on a volatile budget of the terrestrial mantle, the atmosphere and hydrosphere we propose that the LHB did indeed occur on Earth and that we are breathing its aftermaths. The terrestrial atmosphere and hydrosphere is enriched in noble gases relative to the abundance of volatiles in the mantle. This enrichment is consistent with the mass delivered to Earth during the LHB, as recently proposed from dynamical modelling (Gomez et al., 2005), if this material comprised a few Kuiper-belt (cometary) objets (KBOs) mixed in with a population of largely chondritic (i.e. asteroidal) impactors. The fraction of KBOs necessary to account for the atmospheric composition is, however, much lower (<1%) than the one (~50%) inferred from modelling.

Citation: Marty, B. and Meibom, A.: Noble gas signature of the Late Heavy Bombardment in the Earth's atmosphere, eEarth, 2, 43-49, doi:10.5194/ee-2-43-2007, 2007.
 
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