Unravelling the isotopic imprints of Martian CO2 and H2O using solar occultation observations from the Atmospheric Chemistry Suite onboard ExoMars Trace Gas Orbiter
<p>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 conditi...
| Main Author: | |
|---|---|
| Other Authors: | |
| Format: | Thesis |
| Language: | English |
| Published: |
2021
|
| Subjects: |