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Carbonated ultramafic igneous rocks in Jezero crater, Mars

Williford, K.H. ; Alwmark, S. LU and Yingst, R.A. (2026) In Science 391(6787).
Abstract
The Perseverance rover landed in Jezero crater on Mars, which once contained a lake of liquid water. We report the rock properties encountered by Perseverance during a 10-kilometer traverse extending over 400 meters in elevation, from beneath Jezero's western sedimentary fan to the upper crater rim. These rocks consist of coarse-grained olivine, magnesium and iron carbonates, silica, and phyllosilicates, including some of the oldest materials exposed within Jezero. We infer that these rocks formed by olivine accumulation in an igneous system of layered intrusions, followed by exposure to water and carbon dioxide, which caused extensive carbonation of the silicate minerals. aqueous alteration was more pronounced at lower elevations.... (More)
The Perseverance rover landed in Jezero crater on Mars, which once contained a lake of liquid water. We report the rock properties encountered by Perseverance during a 10-kilometer traverse extending over 400 meters in elevation, from beneath Jezero's western sedimentary fan to the upper crater rim. These rocks consist of coarse-grained olivine, magnesium and iron carbonates, silica, and phyllosilicates, including some of the oldest materials exposed within Jezero. We infer that these rocks formed by olivine accumulation in an igneous system of layered intrusions, followed by exposure to water and carbon dioxide, which caused extensive carbonation of the silicate minerals. aqueous alteration was more pronounced at lower elevations. Higher-elevation exposures on the crater rim appear similar to olivine-rich rocks distributed over the wider Nili Fossae region. Copyright © 2026 the authors, some rights reserved; (Less)
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publication status
published
subject
keywords
carbon dioxide, carbonic acid derivative, iron, magnesium, mineral, silicate, silicon dioxide, carbonate rock, crater, igneous rock, Mars, olivine, phyllosilicate, ultramafic rock, article, astronomy, rock, therapy, water
in
Science
volume
391
issue
6787
article number
eadu8264
publisher
American Association for the Advancement of Science (AAAS)
external identifiers
  • scopus:105030758002
  • pmid:41405541
ISSN
0036-8075
DOI
10.1126/science.adu8264
language
English
LU publication?
yes
id
4202d6ea-5a7c-4f1f-8c0b-eadc37663799
date added to LUP
2026-03-26 12:39:59
date last changed
2026-03-27 03:00:02
@article{4202d6ea-5a7c-4f1f-8c0b-eadc37663799,
  abstract     = {{The Perseverance rover landed in Jezero crater on Mars, which once contained a lake of liquid water. We report the rock properties encountered by Perseverance during a 10-kilometer traverse extending over 400 meters in elevation, from beneath Jezero's western sedimentary fan to the upper crater rim. These rocks consist of coarse-grained olivine, magnesium and iron carbonates, silica, and phyllosilicates, including some of the oldest materials exposed within Jezero. We infer that these rocks formed by olivine accumulation in an igneous system of layered intrusions, followed by exposure to water and carbon dioxide, which caused extensive carbonation of the silicate minerals. aqueous alteration was more pronounced at lower elevations. Higher-elevation exposures on the crater rim appear similar to olivine-rich rocks distributed over the wider Nili Fossae region. Copyright © 2026 the authors, some rights reserved;}},
  author       = {{Williford, K.H. and Alwmark, S. and Yingst, R.A.}},
  issn         = {{0036-8075}},
  keywords     = {{carbon dioxide; carbonic acid derivative; iron; magnesium; mineral; silicate; silicon dioxide; carbonate rock; crater; igneous rock; Mars; olivine; phyllosilicate; ultramafic rock; article; astronomy; rock; therapy; water}},
  language     = {{eng}},
  number       = {{6787}},
  publisher    = {{American Association for the Advancement of Science (AAAS)}},
  series       = {{Science}},
  title        = {{Carbonated ultramafic igneous rocks in Jezero crater, Mars}},
  url          = {{http://dx.doi.org/10.1126/science.adu8264}},
  doi          = {{10.1126/science.adu8264}},
  volume       = {{391}},
  year         = {{2026}},
}