Evidence map›Paper›PMID 40238880›Full record

ArticleScience advances2025

In situ crystallographic mapping constrains sulfate precipitation and timing in Jezero crater, Mars.

Michael W M Jones, David T Flannery, Joel A Hurowitz, Michael M Tice, Christoph E Schrank, Abigail C Allwood, Nicholas J Tosca, David C Catling, Scott J VanBommel, Abigail L Knight and 18 more

Abstract read
In one paragraph

Article in Science advances, 2025. The graph could read no effect estimate from its abstract, so it casts no vote on the map. Cited by 3 papers.

0numbers the graph read from it
0cells of the map it votes in
3citing papers in PubMed
–field-weighted citation impact
1 · What the graph read from it

What it found

Each row is one number read from the abstract, on the scale the paper reported it, with its interval. Left of the dashed line favours the treatment, right favours the comparator. Under each row is the sentence it came from. New to these charts? A ten-minute tutorial.

The abstract states no effect estimate the extractor could read, or names no intervention and outcome on the map, so this paper lights no cell and moves no belief. It is still indexed, cited and linked below.

2 · The registry

The trial behind it

Trials whose registry record cites this paper, or whose number appears in the abstract. A trial that started after this paper was published is citing it as background, not reporting it.

Neither the registry nor the abstract names a trial number. If this is a trial report, that itself is worth knowing.

3 · Its place in the literature

Who cites it

3 citing papers in PubMed.

  1. Article
  2. Article
  3. Article
4 · The record

Corrections and comments

PubMed lists nothing against this paper. Absence here is not a guarantee, only a check that was made.

5 · Who and what money

Authors and funding

28 authors.

Michael W M JonesCentral Analytical Research Facility, Queensland University of Technology, Brisbane, 4000, Australia.ORCID 0000-0002-0720-8715
David T FlanneryPlanetary Surface Exploration Group, Queensland University of Technology, Brisbane, 4000, Australia.ORCID 0000-0001-8982-496X
Joel A HurowitzDepartment of Geosciences, Stony Brook University, Stony Brook, NY 11794, USA.ORCID 0000-0002-5857-8652
Michael M TiceDepartment of Geology and Geophysics, Texas A&M University, College Station, TX 77843, USA.
Christoph E SchrankPlanetary Surface Exploration Group, Queensland University of Technology, Brisbane, 4000, Australia.ORCID 0000-0001-9643-2382
Abigail C AllwoodJet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA.ORCID 0009-0002-9779-7855
Nicholas J ToscaDepartment of Earth Sciences, University of Cambridge, Cambridge, UK.ORCID 0000-0003-4415-4231
David C CatlingDepartment of Earth and Space Sciences, University of Washington, Seattle WA 98195, USA.ORCID 0000-0001-5646-120X
Scott J VanBommelDepartment of Earth, Environmental, and Planetary Sciences, Washington University in St. Louis, St. Louis, MO, 63130, USA.ORCID 0000-0002-6565-0827
Abigail L KnightDepartment of Earth, Environmental, and Planetary Sciences, Washington University in St. Louis, St. Louis, MO, 63130, USA.ORCID 0000-0001-6832-8190
Briana GanlyMineral Resources, Commonwealth Scientific and Industrial Research Organisation, Sydney, NSW, Australia.ORCID 0000-0002-4364-7037
Kirsten L SiebachDepartment of Earth, Environmental and Planetary Sciences, Rice University, Houston, TX 77005, USA.ORCID 0000-0002-6628-6297
Kathleen C BenisonDepartment of Geology and Geography, West Virginia University, Morgantown, WV 26506, USA.ORCID 0000-0001-6104-2333
Adrian P BrozDepartment of Earth, Atmospheric and Planetary Sciences, Purdue University, West Lafayette, IN 47907, USA.ORCID 0000-0003-1843-6702
Maria-Paz ZorzanoCentro de Astrobiología (CAB), CSIC-INTA, 28850 Torrejón de Ardoz, Madrid, Spain.ORCID 0000-0002-4492-9650
Chris M HeirweghJet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA.ORCID 0009-0002-8234-7288
Brendan J OrensteinPlanetary Surface Exploration Group, Queensland University of Technology, Brisbane, 4000, Australia.ORCID 0000-0002-6586-4227
Benton C ClarkSpace Science Institute, Boulder, CO 80301, USA.ORCID 0000-0002-5546-8757
Kimberly P SinclairDepartment of Earth and Space Sciences, University of Washington, Seattle WA 98195, USA.ORCID 0000-0001-6261-4591
Andrew O ShumwayDepartment of Earth and Space Sciences, University of Washington, Seattle WA 98195, USA.ORCID 0009-0003-3570-4980
Lawrence A WadeJet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA.ORCID 0000-0001-8254-8181
Scott DavidoffJet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA.ORCID 0000-0002-4417-7268
Peter NemerePlanetary Surface Exploration Group, Queensland University of Technology, Brisbane, 4000, Australia.ORCID 0000-0003-2158-6824
Austin P WrightSchool of Computational Science and Engineering, Georgia Institute of Technology, Atlanta, GA 30332, USA.ORCID 0000-0002-0197-4638
Adrian E GalvinJet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA.
Nicholas RandazzoDepartment of Earth and Atmospheric Sciences, University of Alberta, Edmonton, Alberta, Canada.ORCID 0000-0002-5551-8224
Jesús Martinez-FriasInstitute of Geosciences, CSIC-UCM, Madrid, Spain.ORCID 0000-0002-2609-4485
Lauren P O'NeilDepartment of Geology and Geophysics, Texas A&M University, College Station, TX 77843, USA.ORCID 0000-0003-1555-8229

Funding

No grant is acknowledged in the PubMed record.

6 · The paper itself

Abstract

Late-stage Ca-sulfate-filled fractures are common on Mars. Notably, the Shenandoah formation in the western edge of Jezero crater preserves a variety of Ca-sulfate minerals in the fine-grained siliciclastic rocks explored by the Perseverance rover. However, the depositional environment and timing of the formation of these sulfates are unknown. To address this outstanding problem, we developed a technique to map the crystal orientations of these sulfates in situ at two stratigraphically similar locations in the Shenandoah formation, allowing us to constrain the burial depth and paleoenvironment at the time of their precipitation. Our crystal orientation mapping results and outcrop-scale fracture analyses reveal two different generations of Ca-sulfates: one likely precipitated in the shallow subsurface and a second one that formed at a burial depth below 80 meters. These results indicate that two studied locations capture two different times and distinct chemical conditions in the sedimentary history of the Shenandoah formation, providing multiple opportunities to evaluate surface and subsurface habitability.

Identifiers

PMID40238880
PMCPMC12002120

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Read under generation 80e0d062 · epoch 390. Bibliography from PubMed, PubMed Central and OpenAlex; grants from NIH RePORTER; trial links from ClinicalTrials.gov; estimates, votes and beliefs from the OpenQuestion graph.