EPSC Abstracts
Vol. 17, EPSC2024-954, 2024, updated on 03 Jul 2024
https://doi.org/10.5194/epsc2024-954
Europlanet Science Congress 2024
© Author(s) 2024. This work is distributed under
the Creative Commons Attribution 4.0 License.
Poster | Friday, 13 Sep, 14:30–16:00 (CEST), Display time Friday, 13 Sep, 08:30–19:00|

Venus as an Exoplanet: Effect of varying stellar, orbital, planetary andatmospheric properties upon composition, habitability and detectability

John Lee Grenfell1, Joern Helbert1, Gabriele Arnold1, Konstantin Herbst2, Miriam Sinnhuber3, and Heike Rauer1,4
John Lee Grenfell et al.
  • 1German Aerospace Centre (DLR), Berlin, Germany
  • 2CAU Kiel, Germany
  • 3KIT, Karlsruhe, Germany
  • 4Inst. Geol. Sciences, Free University Berlin, Germany

The newly selected Venus missions EnVISION and VERITAS (Venus Emissivity, Radio Science, InSAR, Topography, and Spectroscopy) offer new opportunities for studying Venus but will also contribute to furthering our knowledge of Venus as an exoplanet. Hot rocky planets are favored targets due to generally more frequent transits than cooler Earth-like objects. In this work we simulate Venus as an exoplanet varying stellar, orbital, planetary and atmospheric parameters and study the effect upon atmospheric composition, climate and spectral detectability.

How to cite: Grenfell, J. L., Helbert, J., Arnold, G., Herbst, K., Sinnhuber, M., and Rauer, H.: Venus as an Exoplanet: Effect of varying stellar, orbital, planetary andatmospheric properties upon composition, habitability and detectability, Europlanet Science Congress 2024, Berlin, Germany, 8–13 Sep 2024, EPSC2024-954, https://doi.org/10.5194/epsc2024-954, 2024.