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Laboratory simulation of Pluto's atmospheric chemistry

Authors :
Lora Jovanovic
Thomas Gautier
Nicolas Jaisle
Ludovic Vettier
Nathalie Carrasco
PLANETO - LATMOS
Laboratoire Atmosphères, Milieux, Observations Spatiales (LATMOS)
Sorbonne Université (SU)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Sorbonne Université (SU)-Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)
Institut Universitaire de France (IUF)
Ministère de l'Education nationale, de l’Enseignement supérieur et de la Recherche (M.E.N.E.S.R.)
Cardon, Catherine
Source :
EPSC-DPS Joint Meeting 2019, EPSC-DPS Joint Meeting 2019, Sep 2019, Geneva, Switzerland. pp.EPSC-DPS2019-957-1, HAL
Publication Year :
2019
Publisher :
HAL CCSD, 2019.

Abstract

International audience; The detection of thin haze layers in Pluto's atmosphere highlighted the complex photochemistry occurring in it. In order to understand the processes leading to the formation of Pluto's aerosols, we produced in laboratory a plasma mimicking Pluto's atmospheric chemistry and we analyzed this plasma by in situ mass spectrometry.

Details

Language :
English
Database :
OpenAIRE
Journal :
EPSC-DPS Joint Meeting 2019, EPSC-DPS Joint Meeting 2019, Sep 2019, Geneva, Switzerland. pp.EPSC-DPS2019-957-1, HAL
Accession number :
edsair.dedup.wf.001..4a4edf8cc27d606c57a1e3844ece618f