EGU26-7267, updated on 14 Mar 2026
https://doi.org/10.5194/egusphere-egu26-7267
EGU General Assembly 2026
© Author(s) 2026. This work is distributed under
the Creative Commons Attribution 4.0 License.
Poster | Monday, 04 May, 16:15–18:00 (CEST), Display time Monday, 04 May, 14:00–18:00
 
Hall X4, X4.163
In the wake of DORN: a comprehensive lunar sample analysis for radon outgassing
Íñigo de Loyola Chacartegui Rojo1,2, Benoit Sabot1, Frédéric Girault2,3, Pierre-Yves Meslin4, Jean Duprat5, Te Jiang5,6,7, and Jiannan Li8
Íñigo de Loyola Chacartegui Rojo et al.
  • 1Université Paris-Saclay, CEA, LIST, Laboratoire National Henri Becquerel (LNE-LNHB), F-91120 Palaiseau, France
  • 2Université Paris Cité, Institut de Physique du Globe de Paris, CNRS, F-75005 Paris, France
  • 3Institut universitaire de France (IUF), Paris, France
  • 4Institut de Recherche en Astrophysique et Planétologie, Université de Toulouse/CNRS/CNES, F-31400 Toulouse, France
  • 5Sorbonne Université/MNHN/CNRS UMR 7590, IMPMC, F-75005 Paris, France
  • 6Université Paris-Saclay, CNRS, Institut d'astrophysique Spatiale (IAS), F-91405 Orsay, France
  • 7Université Paris-Saclay, CNRS, Laboratoire de Physique des deux infinis Irène Joliot Curie (IJCLab), F-91405 Orsay, France
  • 8Institute of Geology and Geophysics, China Academy of Sciences, Beijing, China

The successful return of samples by the Chang’E 5 and Chang’E 6 missions of the China National Space Administration (CNSA) marks an important milestone for lunar science, offering unprecedented access to a new set of samples from young mare basalts and far-side regolith. This study builds upon the scientific legacy of the DORN (Detection of Outgassing RadoN) instrument onboard Chang’E 6, which performed the first in-situ radon measurements on the Moon. It aims to connect orbital and in-situ measurements with laboratory analysis of lunar regolith.

We present a study investigating the mechanisms governing radon dynamics in the regolith and at the regolith-exosphere interface, including production (emanation) and transport (adsorption). Conducted at the Laboratoire National Henri Becquerel (LNE-LNHB), our approach uses a custom-developed suite of high-sensitivity techniques, including low-level gamma-ray spectrometry, liquid scintillation counting, and a purpose-built gas bench. This methodology is designed to characterise quantities of extraterrestrial material on the order of 1 gram.

Having validated our protocols using lunar analogues, we are currently applying this framework to a returned Chang’E 5 sample. We will present our methodology and discuss preliminary findings on the radioactive content and radon emanation fraction of this sample.

How to cite: Chacartegui Rojo, Í. D. L., Sabot, B., Girault, F., Meslin, P.-Y., Duprat, J., Jiang, T., and Li, J.: In the wake of DORN: a comprehensive lunar sample analysis for radon outgassing, EGU General Assembly 2026, Vienna, Austria, 3–8 May 2026, EGU26-7267, https://doi.org/10.5194/egusphere-egu26-7267, 2026.