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Updated: Jun 30, 2026

Preparation of Authigenic Pyrite from Methane-bearing Sediments for In Situ Sulfur Isotope Analysis Using SIMS
Published on: August 31, 2017
A native sulfur deposit in Gale crater, Mars
Scott J VanBommel1, Jeff A Berger2, Penelope L King3
1McDonnell Center for the Space Sciences, Department of Earth, Environmental, and Planetary Sciences, Washington University in St. Louis, St. Louis, MO, USA.
Ancient Martian rocks contain native sulfur, indicating a subsurface fluid pathway. This discovery suggests magmatic vapor was the sulfur source, released during canyon erosion on Mars.
Area of Science:
- Planetary Science
- Geochemistry
- Astrobiology
Background:
- Martian rocks exhibit sulfur-bearing species like sulfates and sulfides, reflecting an ancient sulfur cycle.
- Understanding Mars' sulfur cycle provides insights into its geological and potential biological evolution.
Purpose of the Study:
- To investigate a native sulfur deposit in Gediz Vallis, Gale crater using the Curiosity rover.
- To determine the formation mechanism and source of native sulfur on Mars.
Main Methods:
- In-situ analysis of light-toned stones in Gediz Vallis using the Curiosity rover.
- Geological context analysis of the sinuous entrenched canyon formation.
Main Results:
- The investigated stones are composed of native sulfur, forming an in-situ deposit.
- The deposit is located within a sinuous entrenched canyon.
- Evidence suggests a sulfur enrichment pathway involving buoyant subsurface fluids.
Conclusions:
- Native sulfur formation implies a significant sulfur cycle on ancient Mars.
- Magmatic vapor, cooling in the subsurface cryosphere, is proposed as the primary sulfur source.
- Decompression during Gediz Vallis erosion likely released this sulfur, leading to native sulfur deposits.
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