East Meridiani Planum’s karst geomorphology and biosignature preservation potential: a multi-criteria landing site analysis

Introduction Future Mars astrobiology missions require landing sites that balance scientific potential for biosignature detection with engineering safety. This study addresses the need for systematic identification of optimal sites targeting ancient aqueous environments distinct from previously explored terrains. Methods A multi-criteria GIS-based analysis was conducted to evaluate five candidate landing sites (Aram Chaos, East Meridiani Planum, Ottumwa Crater, East Margaritifer Terra, and Nili Fossae) using global and regional datasets including MOLA topography, MOCAAS mineralogy, HiRISE imagery, and thermal inertia measurements. Sites were assessed against engineering constraints (latitude ±30°, elevation <−0.5 km, slopes <15°, thermal inertia >100 J m −2 K −1 s 0.5 ) and scientific criteria (diversity, context, habitability, and biosignature preservation potential). Results East Meridiani Planum emerged as the top-ranked candidate. The site features unique evaporite karst geomorphology (ridges, dolines, salt pans), extensive hydrous sulfate and Fe/Mg phyllosilicate deposits, and favorable engineering parameters (elevation: −1.1 km; thermal inertia: 200–450 J m −2 K −1 s 0.5 ; slopes <5°). The proposed 25 km × 20 km landing ellipse at 0.74°N, 4.44°E provides access to the Noachian-age (∼3.7 Ga) Upper Etched Unit, offering a distinct paleoenvironment from the Hesperian hematite plains explored by the Opportunity rover. Discussion This site offers exceptional potential for investigating Mars' hydrological evolution and detecting preserved organic molecules. The dual mineralogy—neutral-pH smectite clays favorable for molecular preservation and acidic sulfate evaporites conducive to morphological biosignature preservation—enables testing of multiple biosignature hypotheses. The combination of high scientific value, minimal aeolian cover, and flat topography makes East Meridiani Planum an optimal target for future astrobiology missions seeking evidence of ancient Martian habitability.

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Journal
Frontiers in Astronomy and Space Sciences
Published
2026-03-12
DOI
https://doi.org/10.3389/fspas.2026.1681194
Primary Topic
Planetary Science and Exploration
Type
article
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article

East Meridiani Planum’s karst geomorphology and biosignature preservation potential: a multi-criteria landing site analysis

Shaoqiu Wang
Frontiers in Astronomy and Space Sciences
Planetary Science and Exploration
article

East Meridiani Planum’s karst geomorphology and biosignature preservation potential: a multi-criteria landing site analysis

Shaoqiu Wang
article en

Abstract

Introduction Future Mars astrobiology missions require landing sites that balance scientific potential for biosignature detection with engineering safety. This study addresses the need for systematic identification of optimal sites targeting ancient aqueous environments distinct from previously explored terrains. Methods A multi-criteria GIS-based analysis was conducted to evaluate five candidate landing sites (Aram Chaos, East Meridiani Planum, Ottumwa Crater, East Margaritifer Terra, and Nili Fossae) using global and regional datasets including MOLA topography, MOCAAS mineralogy, HiRISE imagery, and thermal inertia measurements. Sites were assessed against engineering constraints (latitude ±30°, elevation <−0.5 km, slopes <15°, thermal inertia >100 J m −2 K −1 s 0.5 ) and scientific criteria (diversity, context, habitability, and biosignature preservation potential). Results East Meridiani Planum emerged as the top-ranked candidate. The site features unique evaporite karst geomorphology (ridges, dolines, salt pans), extensive hydrous sulfate and Fe/Mg phyllosilicate deposits, and favorable engineering parameters (elevation: −1.1 km; thermal inertia: 200–450 J m −2 K −1 s 0.5 ; slopes <5°). The proposed 25 km × 20 km landing ellipse at 0.74°N, 4.44°E provides access to the Noachian-age (∼3.7 Ga) Upper Etched Unit, offering a distinct paleoenvironment from the Hesperian hematite plains explored by the Opportunity rover. Discussion This site offers exceptional potential for investigating Mars' hydrological evolution and detecting preserved organic molecules. The dual mineralogy—neutral-pH smectite clays favorable for molecular preservation and acidic sulfate evaporites conducive to morphological biosignature preservation—enables testing of multiple biosignature hypotheses. The combination of high scientific value, minimal aeolian cover, and flat topography makes East Meridiani Planum an optimal target for future astrobiology missions seeking evidence of ancient Martian habitability.

Frontiers in Astronomy and Space SciencesVol. 13
Imperial College London (GB)
Openalex Percentile: Top 28%
Planetary Science and Exploration
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East Meridiani Planum’s karst geomorphology and biosignature preservation potential: a multi-criteria landing site analysis — Shaoqiu Wang · Frontiers in Astronomy and Space Sciences (2026) | TGRS Research Map | TGRS