Explore the words cloud of the Photonis project. It provides you a very rough idea of what is the project "Photonis" about.
The following table provides information about the project.
Coordinator |
UNIVERSITE DE LORRAINE
Organization address contact info |
Coordinator Country | France [FR] |
Project website | http://photonis.univ-lorraine.fr |
Total cost | 2˙810˙229 € |
EC max contribution | 2˙810˙229 € (100%) |
Programme |
1. H2020-EU.1.1. (EXCELLENT SCIENCE - European Research Council (ERC)) |
Code Call | ERC-2015-AdG |
Funding Scheme | ERC-ADG |
Starting year | 2017 |
Duration (year-month-day) | from 2017-01-01 to 2021-12-31 |
Take a look of project's partnership.
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1 | UNIVERSITE DE LORRAINE | FR (NANCY CEDEX) | coordinator | 2˙810˙229.00 |
Light elements such as hydrogen and nitrogen present large isotope variations among solar system objects and reservoirs (including planetary atmospheres) that remain unexplained at present. Works based on theoretical approaches are model-dependent and do not reach a consensus. Laboratory experiments are required in order to develop the underlying physical mechanisms. The aim of the project is to investigate the origins of and processes responsible for isotope variations of the light elements and noble gases in the Solar System through an experimental approach involving ionization of gaseous species. We will also investigate mechanisms and processes of isotope fractionation of atmophile elements in planetary atmospheres that have been irradiated by solar UV photons, with particular reference to Mars and the early Earth. Three pathways will be considered: (i) plasma ionisation of gas mixtures (H2-CO-N2-noble gases) in a custom-built reactor; (ii) photo-ionisation and photo-dissociation of the relevant gas species and mixtures using synchrotron light; and (iii) UV irradiation of ices containing the species of interest. The results of this study will shed light on the early Solar System evolution and on processes of planetary formation.
year | authors and title | journal | last update |
---|---|---|---|
2018 |
David V. Bekaert, Michael W. Broadley, Frédéric Delarue, Guillaume Avice, Francois Robert, Bernard Marty Archean kerogen as a new tracer of atmospheric evolution: Implications for dating the widespread nature of early life published pages: eaar2091, ISSN: 2375-2548, DOI: 10.1126/sciadv.aar2091 |
Science Advances 4/2 | 2019-06-14 |
2017 |
David V. Bekaert, Guillaume Avice, Bernard Marty, Bryana Henderson, Murthy S. Gudipati Stepwise heating of lunar anorthosites 60025, 60215, 65315 possibly reveals an indigenous noble gas component on the Moon published pages: 114-131, ISSN: 0016-7037, DOI: 10.1016/j.gca.2017.08.041 |
Geochimica et Cosmochimica Acta 218 | 2019-06-13 |
2018 |
David V. Bekaert, Sylvie Derenne, Laurent Tissandier, Yves Marrocchi, Sebastien Charnoz, Christelle Anquetil, Bernard Marty High-temperature Ionization-induced Synthesis of Biologically Relevant Molecules in the Protosolar Nebula published pages: 142, ISSN: 1538-4357, DOI: 10.3847/1538-4357/aabe7a |
The Astrophysical Journal 859/2 | 2019-06-13 |
2018 |
David V. Bekaert, Guillaume Avice, Bernard Marty Origin and significance of cosmogenic signatures in vesicles of lunar basalt 15016 published pages: 1238-1251, ISSN: 1086-9379, DOI: 10.1111/maps.13069 |
Meteoritics & Planetary Science 53/6 | 2019-06-13 |
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The information about "PHOTONIS" are provided by the European Opendata Portal: CORDIS opendata.