Overview of the MMT 60-day GEER Experiment on Geologic Samples at Venus Surface Conditions
Laboratory experiments on the behavior of rock and mineral samples under Venus conditions can yield a better understanding of gas-solid chemical weathering. The Glenn Extreme Environments Rig (GEER) vessel can maintain Venus surface temperature, pressure and a nine-gas atmosphere for months. Here, we provide an overview of the GEER Test Project Marty’s Minerals Test (MMT), which ran for 60 days at 460°C, 93 bars under a 9 component Venus-relevant gas mixture. This experiment includes over 90 compositionally unique chips and powders of natural samples, selected to explore the pathways and relative rates of alteration of a broad range of mineral and rock types. Target temperature, pressure, and gas (CO2, N2, SO2, OCS) composition were monitored over the run. Rapid SO2 depletion from the vessel gas phase occurred throughout the test indicating sequestration of SO2 gas-solid reactions. A significant sink for SO2 is the formation of iron oxide and Ni sulfide coatings on some chamber parts that was compensated by multiple SO2 gas injections during the run. Initial results for selected samples include the formation of secondary minerals at sample surfaces (e.g., on Na2CO3, natrite) and complete alteration of other samples (e.g., FeS, troilite) to oxide and sulfides. Some powdered samples consolidated to form hardened layers or chips. These observations show that some mineral phases are chemically and/or physically unstable over the timescale of the run. This test confirms that GEER is a critical asset and reference point to support the study of gas-solid interactions on the surface of Venus.
Authors
- M. S. Gilmore (ORCID: https://orcid.org/0000-0001-8583-1513)
- N. R. Izenberg (ORCID: https://orcid.org/0000-0003-1629-6478)
- Tibor Kremic (ORCID: https://orcid.org/0000-0002-1665-2439)
- M. D. Dyar (ORCID: https://orcid.org/0000-0003-4272-793X)
- A. R. Santos (ORCID: https://orcid.org/0000-0003-2314-6662)
- Dorothy Lukco (ORCID: https://orcid.org/0000-0003-3424-0320)
- M. C. McCanta (ORCID: https://orcid.org/0000-0001-9486-8908)
- Mark Sprouse
- Ian Henry
- J. Helbert (ORCID: https://orcid.org/0000-0001-5346-9505)
- Joseph Rymut
- L. B. Breitenfeld (ORCID: https://orcid.org/0000-0002-6810-8224)
- Jennifer M. Jackson (ORCID: https://orcid.org/0000-0002-8256-6336)
- J. A. Balcerski
- M. Yu. Zolotov (ORCID: https://orcid.org/0000-0003-0670-0684)
- S. T. Port (ORCID: https://orcid.org/0000-0002-3113-4437)
- Daniel Gerges
- Kyle G. Phillips
- Maximillian Scardelletti
- Craig Motil
Institutions
- Wesleyan University (US)
- California Institute of Technology (US)
- Mount Holyoke College (US)
- Glenn Research Center (US)
- European Space Agency (FR)
- The University of Texas at San Antonio (US)
- Arizona State University (US)
- Case Western Reserve University (US)
- University of Tennessee at Knoxville (US)
Publication Details
- Published
- 2025-08-12
- DOI
- https://doi.org/10.22541/essoar.175503805.54287367/v1
- Citations
- 1
- Primary Topic
- Planetary Science and Exploration
- Type
- article
- Field-Weighted Citation Impact
- 1.15
Funders
- National Aeronautics and Space Administration
- Keck Institute for Space Studies
- Nuclear Safety and Security Commission