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Thesis

Unravelling the isotopic imprints of Martian CO2 and H2O using solar occultation observations from the Atmospheric Chemistry Suite onboard ExoMars Trace Gas Orbiter

Abstract:

Numerous lines of geomorphological and mineralogical evidence suggest that liquid water was once abundant on Mars’ surface, which might also be indicative of a more hospitable environment for life to grow. The presence of large amounts of liquid water on the surface require climatic conditions very different from those enabled by the dry and thin atmosphere Mars has today. In fact, it is still not well understood how the past Martian atmosphere was able to produce sufficient greenhouse war...

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Division:
MPLS
Department:
Physics
Sub department:
Atmos Ocean & Planet Physics
Role:
Author

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Role:
Supervisor
Role:
Supervisor
ORCID:
0000-0001-5355-1533


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Funder identifier:
http://dx.doi.org/10.13039/100011690
Grant:
ST/R001502/1


Type of award:
DPhil
Level of award:
Doctoral
Awarding institution:
University of Oxford


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