2023
DOI: 10.1029/2022je007545
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Sources of Clay‐Rich Sediment in Eberswalde Crater, Mars With Implications for Biopreservation Potential

Abstract: Introduction and Background Mars HabitabilityToday, the mean atmospheric pressure at the surface of Mars is ∼0.6 atm, and the mean surface temperature during the day has been shown to be ∼200 K (e.g., Schofield et al., 1997). Within this cold and thin atmosphere, liquid water is not thermodynamically stable, and most water on present-day Mars is locked in the cryosphere. However, abundant geologic evidence in the form of massive drainage networks (e.g., Barnhart et al., 2009;Hynek & Phillips, 2003), and numero… Show more

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Cited by 1 publication
(2 citation statements)
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“…Io's mean density and moment of inertia indicate the presence of a core with possible compositions that range from pure Fe to an Fe-FeS eutectic mixture [which is ~25% sulfur by mass (30)]. These constraints, combined with experiments on equilibrium sulfur partitioning between metal and silicates, indicate that 80 to 97% of Io's initial sulfur inventory is in the core (20). Our measurement of 94 to 99% sulfur loss is therefore consistent with the fraction of noncore sulfur lost if Io has been losing mass at ~0.5 to 5 times its current rate over its entire 4.57-Gyr lifetime.…”
Section: Io's Mass-loss Historymentioning
confidence: 99%
See 1 more Smart Citation
“…Io's mean density and moment of inertia indicate the presence of a core with possible compositions that range from pure Fe to an Fe-FeS eutectic mixture [which is ~25% sulfur by mass (30)]. These constraints, combined with experiments on equilibrium sulfur partitioning between metal and silicates, indicate that 80 to 97% of Io's initial sulfur inventory is in the core (20). Our measurement of 94 to 99% sulfur loss is therefore consistent with the fraction of noncore sulfur lost if Io has been losing mass at ~0.5 to 5 times its current rate over its entire 4.57-Gyr lifetime.…”
Section: Io's Mass-loss Historymentioning
confidence: 99%
“…Io's atmosphere is thought to be well-mixed up to a boundary known as the homopause [altitude ~30 km (19)]. Between the homopause and another boundary known as the exobase (altitude ~600 km), molecular diffusion produces a gravitationally stratified atmosphere (20). In the exosphere (above the exobase), the atmosphere is collision-less.…”
Section: The 34 S/ 32 S Ratiomentioning
confidence: 99%