Extensive Lithological Diversity of Float Rocks at the Mount Washburn Mound in Neretva Vallis, Jezero Crater, Mars
Open Access
- 23 February 2026
- journal article
- research article
- Published by American Geophysical Union (AGU) in Journal of Geophysical Research: Planets
- Vol. 131 (2)
Abstract
During its exploration of Neretva Vallis in Jezero crater, NASA's Mars 2020 Perseverance rover examined Mount Washburn, a set of light‐toned sedimentary mounds that exhibited a diverse array of float rocks. Mastcam‐Z visible/near‐infrared (VISIR) multispectral imaging revealed five spectral types dominated by low‐calcium pyroxene‐bearing rocks, although olivine‐bearing and ferric materials were also identified. SuperCam VISIR point spectroscopy of eight targets noted four spectral groups, including those with low‐Ca pyroxene, hydrated alteration products, and phyllosilicates. SuperCam laser‐induced breakdown spectroscopy data confirmed a wide compositional array among the targets. Overall, these data spanned much of the spectral and compositional range in rocks observed by Perseverance through Sol 1348, with no major outliers, although some rock textures were unique. The rock diversity at Mount Washburn is among the most extensive observed in situ at a single site on Mars, pointing to a multifaceted geological history. Bedrock beneath Mount Washburn exhibited high silica and iron content, closely resembling materials from the nearby Bright Angel sedimentary units and suggesting a possible stratigraphic link. Some geological models of Neretva Vallis are consistent with the idea that Bright Angel‐like materials may have formed the foundation of Mount Washburn, with subsequent deposition of cobbles and boulders as late‐stage fluvial events. These findings suggest that similar rocks—and possibly their source regions—may be encountered during future exploration of the Jezero crater rim and intracrater plains. Such materials would likely sample the olivine/carbonate‐bearing regional units and/or ancient Noachian basement, reflecting the rich geological complexity of the Neretva Vallis watershed.Keywords
Funding Information
- Arizona State University (15‐707/1511125)
- Jet Propulsion Laboratory (1511125)
This publication has 64 references indexed in Scilit:
- Ultramafic float rocks at Jezero crater (Mars): excavation of lower crustal rocks or mantle peridotites by impact cratering?Earth and Planetary Science Letters, 2025
- The mineral diversity of Jezero crater: Evidence for possible lacustrine carbonates on MarsIcarus, 2020
- Refining the age, emplacement and alteration scenarios of the olivine-rich unit in the Nili Fossae region, MarsIcarus, 2020
- The Mars Science Laboratory Curiosity rover Mastcam instruments: Preflight and in‐flight calibration, validation, and data archivingEarth and Space Science, 2017
- Sedimentological evidence for a deltaic origin of the western fan deposit in Jezero crater, Mars and implications for future explorationEarth and Planetary Science Letters, 2017
- Dust deposition on the decks of the Mars Exploration Rovers: 10 years of dust dynamics on the Panoramic Camera calibration targetsEarth and Space Science, 2015
- Assessing the mineralogy of the watershed and fan deposits of the Jezero crater paleolake system, MarsJournal of Geophysical Research: Planets, 2015
- Revised CRISM spectral parameters and summary products based on the currently detected mineral diversity on MarsJournal of Geophysical Research: Planets, 2014
- Near-infrared spectra of ferrous mineral mixtures and methods for their identification in planetary surface spectraIcarus, 2014
- Detection and discrimination of sulfate minerals using reflectance spectroscopyIcarus, 2006