Claire A. Mondro
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View article: Dark‐Toned Halite‐Enriched Veins Above the Marker Band Record a Drying Environment in Gale Crater
Dark‐Toned Halite‐Enriched Veins Above the Marker Band Record a Drying Environment in Gale Crater Open
The Martian surface preserves evidence of a global climate transition from wetter to drier conditions, but the nature of the fluids involved in this evolution remains poorly constrained. In Gale crater, the clay‐sulfate transition and pres…
View article: A Burial History of the Sedimentary Succession Preserved in Aeolis Mons, as Recorded by Fracture Networks at Maria Gordon Notch, Gale Crater, Mars
A Burial History of the Sedimentary Succession Preserved in Aeolis Mons, as Recorded by Fracture Networks at Maria Gordon Notch, Gale Crater, Mars Open
Fractures in sedimentary rocks preserved within Gale crater record the deformational and burial history of the sediment infill. Fracture geometries and morphology can be used to time other geologic events, such as: compaction, diagenesis, …
View article: Dark-Toned Halite-Enriched Veins Above the Marker Band Record a Drying Environment in Gale Crater
Dark-Toned Halite-Enriched Veins Above the Marker Band Record a Drying Environment in Gale Crater Open
View article: Paleo‐Scours Within the Layered Sulfate‐Bearing Unit at Gale Crater, Mars: Evidence for Intense Wind Erosion
Paleo‐Scours Within the Layered Sulfate‐Bearing Unit at Gale Crater, Mars: Evidence for Intense Wind Erosion Open
The surface of modern Mars is largely shaped by wind, but the influence of past wind activity is less well constrained. Sedimentary rocks exposed in the lower foothills of Aeolis Mons, the central mound within Gale crater, record a transit…
View article: Hypotheses for the water and metal fluxes to the rippled Amapari Marker Band, Gale Crater, Mars
Hypotheses for the water and metal fluxes to the rippled Amapari Marker Band, Gale Crater, Mars Open
View article: Prow & co.: inside the fluvial lenses of Gale's layered sulfate unit
Prow & co.: inside the fluvial lenses of Gale's layered sulfate unit Open
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View article: DEPOSITIONAL ENVIRONMENT AND PALEOCLIMATE IMPLICATIONS OF THE AMAPARI MARKER BAND WAVE RIPPLES
DEPOSITIONAL ENVIRONMENT AND PALEOCLIMATE IMPLICATIONS OF THE AMAPARI MARKER BAND WAVE RIPPLES Open
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View article: Depositional Environment of the Amapari Marker Band: Rising Water Levels Formed Kilometer‐Scale Lake in Gale Crater, Mars
Depositional Environment of the Amapari Marker Band: Rising Water Levels Formed Kilometer‐Scale Lake in Gale Crater, Mars Open
The Amapari Marker Band (AMB) is a layer within the Mount Sharp stratigraphy that has been mapped around the Gale crater in orbital images and was recently investigated up close by the Curiosity rover. Symmetric wave ripple marks within th…
View article: Wave ripples formed in ancient, ice-free lakes in Gale crater, Mars
Wave ripples formed in ancient, ice-free lakes in Gale crater, Mars Open
Symmetrical wave ripples identified with NASA’s Curiosity rover in ancient lake deposits at Gale crater provide a key paleoclimate constraint for early Mars: At the time of ripple formation, climate conditions must have supported ice-free …
View article: Depositional processes and environments of the Layered Sulfate-bearing unit, Gale crater, Mars
Depositional processes and environments of the Layered Sulfate-bearing unit, Gale crater, Mars Open
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View article: The Upper Gediz Vallis Ridge at Gale Crater: Sedimentary Rock Clasts Transported by a Late-Stage Debris Flow on Mars?
The Upper Gediz Vallis Ridge at Gale Crater: Sedimentary Rock Clasts Transported by a Late-Stage Debris Flow on Mars? Open
The Mars Science Laboratory (MSL) Curiosity rover continues to ascend Aeolis Mons in Gale crater, Mars, with the goal of characterising formerly habitable palaeoenvironments. Since September 2022, Curiosity has been traversing Gediz Vallis…
View article: THE AMAPARI MARKER BAND, GALE CRATER, MARS: METAL ENRICHMENTS AND POTENTIAL MECHANISMS OF FORMATION
THE AMAPARI MARKER BAND, GALE CRATER, MARS: METAL ENRICHMENTS AND POTENTIAL MECHANISMS OF FORMATION Open
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View article: Astrobiology eXploration at Enceladus (AXE): A New Frontiers Mission Concept Study
Astrobiology eXploration at Enceladus (AXE): A New Frontiers Mission Concept Study Open
The Saturnian moon Enceladus presents a unique opportunity to sample the contents of a subsurface liquid water ocean in situ via the continuous plume formed over its south polar terrain using a multi-flyby mission architecture. Previous an…
View article: Surface grain size of alluvial fans on Mars from thermal inertia, as an indicator of depositional style
Surface grain size of alluvial fans on Mars from thermal inertia, as an indicator of depositional style Open
The depositional history of alluvial fans on Mars provides insight into the climatic conditions during the time of fan formation in the late Hesperian to early Amazonian.However, traditional stratigraphic analysis of the alluvial fan depos…
View article: SupplementaryMaterial_MarsAlluvialFan_Thermal_Inertia_summary
SupplementaryMaterial_MarsAlluvialFan_Thermal_Inertia_summary Open
This table functions as Supplementary Material for the manuscript cited below. Please see the text of the preprint manuscript for more detail on data collection, results, and discussion.Mondro, C.A, J.E. Moersch, C. Hardgrove, (2023, prepr…