Member Since 2006
Edwin S. Kite
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Late‐Stage Aqueous Activity at Gale Crater, Mars, Recorded by Sediment Fans Eroded From Aeolis Mons
JOURNAL OF GEOPHYSICAL RESEARCH: PLANETS
18 march 2025
Joel Davis, Sanjeev Gupta, Peter M. Grindrod, Stev...

Gale crater, the landing site of NASA's Curiosity rover, and the mountain at its center, Aeolis Mons, hosts an extensive record of sedimentary rock...

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Depositional Environment of the Amapari Marker Band: Rising Water Levels Formed Kilometer‐Scale Lake in Gale Crater, Mars
JOURNAL OF GEOPHYSICAL RESEARCH: PLANETS
11 march 2025
Claire Mondro, John Grotzinger, Christopher Fedo, ...

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 ...

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The hydrogeomorphic evolution of Gediz Vallis system, Gale Crater, Mars.
GEOMORPHIC PROCESSES ACROSS PLANETARY SURFACES I ORAL
earth and planetary surface processes | 13 december 2024
Alexander B. Bryk, William E. Dietrich, Kristen A....
Along the northwest facing side of Mt. Sharp in Gale Crater lies a series of erosional and depositional features that suggest a rich history of changi...
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Distributions of H, C, and N during Earth’s formation
FROM THE SURFACE TO DEEP INTERIOR OF THE EARLY TERRESTRIAL WORLDS II ORAL
study of earth's deep interior | 11 december 2024
Jesse T. Gu, Bo Peng, Xuan Ji, Jisheng Zhang, Hong...
The presence of volatile elements (H, C, and N) at the Earths surface is crucial for its habitability. During Earths formation, these elements are dis...
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The Fade of Eden: regime transitions of hydrological cycles & the edge of habitability
ATMOSPHERES, CLIMATE, AND POTENTIAL HABITABILITY OF ROCKY EXOPLANETS III ORAL
planetary sciences | 10 december 2024
Bowen Fan, Edwin S. Kite
The planetary hydrological cycle is crucial for habitability, encompassing factors such as surface liquid abundance1, runaway greenhouse effects2, and...
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Large-scale dissolution of hydrogen in silicate magma oceans
EXPLORING PLANETARY INTERIORS: UNRAVELING THE DYNAMICS, THERMAL EVOLUTION, AND MINERALOGY FROM MANTLE TO CORE I POSTER
mineral and rock physics | 10 december 2024
Razvan Caracas, Edwin S. Kite
The question of hydrogen dissolution in a silicate planet is longstanding within the Earth and planetary science community [1]. Its presence and amoun...
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Feasibility of keeping Mars warm with engineered nanoparticles
PLANETARY ATMOSPHERES: WINDOWS INTO HABITABILITY AND INHABITANCE POSTER
planetary sciences | 10 december 2024
Edwin S. Kite, Samaneh Ansari, Ramses M. Ramirez, ...
One-third of Mars' surface has shallow-buried H2O, but it is currently too cold for use by life. Proposals to warm Mars using greenhouse gases require...
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Carbonate Mineral Detections in Gale Crater with the CheMin Instrument on the Mars Science Laboratory Curiosity Rover
CARBONATES ON MARS: RECORDS OF THE ANCIENT HYDROSPHERE AND ATMOSPHERE POSTER
planetary sciences | 09 december 2024
Elizabeth B. Rampe, Thomas Bristow, Benjamin M. Tu...
The Mars Science Laboratory Curiosity rover landed in Gale crater in August 2012 to characterize ancient and modern environments on Mars and to evalua...
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