Venusian phosphine: a ‘wow!’ signal in chemistry?
The potential detection of ppb levels phosphine (PH3) in the clouds of Venus through millimeter-wavelength astronomical observations is extremely surprising as PH3 is an unexpected component of an oxidized environment of Venus. A thorough analysis of potential sources suggests that no known proce...
Príomhchruthaitheoirí: | Bains, William, Petkowski, Janusz J, Seager, Sara, Ranjan, Sukrit, Sousa-Silva, Clara, Rimmer, Paul B, Zhan, Zhuchang, Greaves, Jane S, Richards, Anita MS |
---|---|
Rannpháirtithe: | Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences |
Formáid: | Alt |
Teanga: | English |
Foilsithe / Cruthaithe: |
Informa UK Limited
2023
|
Rochtain ar líne: | https://hdl.handle.net/1721.1/148516 |
Míreanna comhchosúla
Míreanna comhchosúla
-
Constraints on the Production of Phosphine by Venusian Volcanoes
de réir: Bains, William, et al.
Foilsithe / Cruthaithe: (2022) -
Phosphine on Venus Cannot Be Explained by Conventional Processes
de réir: Bains, William, et al.
Foilsithe / Cruthaithe: (2021) -
The Venusian Lower Atmosphere Haze as a Depot for Desiccated Microbial Life: A Proposed Life Cycle for Persistence of the Venusian Aerial Biosphere
de réir: Seager, Sara, et al.
Foilsithe / Cruthaithe: (2021) -
Phosphine as a Biosignature Gas in Exoplanet Atmospheres
de réir: Ribeiro De Sousa E Silva, Clara, et al.
Foilsithe / Cruthaithe: (2020) -
Only extraordinary volcanism can explain the presence of parts per billion phosphine on Venus
de réir: Bains, William, et al.
Foilsithe / Cruthaithe: (2023)