Transient HCl in the atmosphere of Mars

Author:

Korablev Oleg1ORCID,Olsen Kevin S.2ORCID,Trokhimovskiy Alexander1ORCID,Lefèvre Franck3ORCID,Montmessin Franck3ORCID,Fedorova Anna A.1ORCID,Toplis Michael J.4,Alday Juan2ORCID,Belyaev Denis A.1ORCID,Patrakeev Andrey1ORCID,Ignatiev Nikolay I.1ORCID,Shakun Alexey V.1ORCID,Grigoriev Alexey V.1ORCID,Baggio Lucio3ORCID,Abdenour Irbah3ORCID,Lacombe Gaetan3ORCID,Ivanov Yury S.5,Aoki Shohei67ORCID,Thomas Ian R.7ORCID,Daerden Frank7ORCID,Ristic Bojan7ORCID,Erwin Justin T.7ORCID,Patel Manish8ORCID,Bellucci Giancarlo9ORCID,Lopez-Moreno Jose-Juan10ORCID,Vandaele Ann C.7ORCID

Affiliation:

1. Space Research Institute (IKI), Moscow, Russia.

2. Department of Physics, University of Oxford, Oxford, UK.

3. Laboratoire Atmosphères, Milieux, Observations Spatiales (LATMOS/CNRS), Paris, France.

4. L’Institut de Recherche en Astrophysique et Planétologie (IRAP/CNRS), Toulouse, France.

5. Main Astronomical Observatory (MAO NASU), Kyiv, Ukraine.

6. LPAP, STAR Institute, Université de Liège, Liège, Belgium.

7. Royal Belgian Institute of Space Aeronomy (BIRA-IASB), Brussels, Belgium.

8. Open University, Milton-Keynes, UK.

9. Istituto di Astrofisica e Planetologia Spaziali (IAPS-INAF), Rome, Italy.

10. Instituto de Astrofìsica de Andalucía (IAA/CSIC), Granada, Spain.

Abstract

The discovery of chlorine in the martian atmosphere points to its surface origin.

Funder

Natural Sciences and Engineering Research Council of Canada

European Space Agency

Agence Nationale de la Recherche

Centre National d’Etudes Spatiales

Russian Science Foundation

United Kingdom Space Agency

State Space Corporation ROSCOSMOS

Ministry of Science, Innovation and Universities of Spain

Spanish Science Ministry Centro de Excelencia Severo Ochoa Program

Italian Space Agency

Ministry of Science and Education of Russia

Belgian Science Policy Office

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

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