Insights into Martian water reservoirs from analyses of Martian meteorite QUE94201

By L. Leshin. 2000

149 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Ecology

View Paper: https://www.semanticscholar.org/paper/ae268ce36b1758e5f378648badcc6a2d4b5fbc81

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In Astronomy and Astrophysics

1. A. Morbidelli
2. Jonathan I. Lunine
3. S. Hauck,
4. M. Mellon
5. J. Chambers
6. T. Prettyman
7. Roger J. Phillips
8. W. Feldman

In Ecology

1. A. Morbidelli
2. J. Chambers
3. Roger J. Phillips
4. S. Hauck,
5. V. Krasnopolsky
6. Jonathan I. Lunine
7. W. Feldman
8. H. Yurimoto

Citations in the corpus

• Hydrous melting of the martian mantle produced both depleted and enriched shergottites (2012, unknown): “1527 [14] Leshin (2000) GRL 27.”
• Heterogeneous distribution of H2O in the Martian interior: Implications for the abundance of H2O in depleted and enriched mantle sources (2016, background): “…we did not directly determine the H2O abundances of apatite in this study, previous studies have directly determined H2O abundances in Martian apatite by secondary ion mass spectrometry (SIMS) (Boctor et al. 2003; Greenwood et al. 2008; Leshin 2000; McCubbin et al. 2012; Watson et al. 1994).”
• Hydrogen isotope evidence for loss of water from Mars through time (2008, methodology): “It has been suggested that correlation between D/H and water content of apatite in Martian basaltic shergottite QUE94201 can be used to infer the D/ H of the Martian mantle [Leshin, 2000] (which has been assumed to represent the D/H of accreted water).”
• Mars' upper atmosphere and ionosphere at low, medium, and high solar activities: Implications for evolution of water (2002, background): “9 [Leshin, 2000] were assumed for the initial and final D/H ratios, respectively, and f = 0.”
• Global distribution of near-surface hydrogen on Mars (2004, background): “Measurements of the D/H ratio suggest that between 5 and 50 m of this inventory has been lost to space [Yung et al., 1988; Luhman et al., 1992; Carr, 1990; Jakosky, 1991; Leshin, 2000].”
• The origin of water on Mars (2002, methodology): “Hence, in context of our model we would interpret D/H derived fro magmatic water in QUE94201 as representing either a mordial martian value obtained from accretion of a mixt of asteroidal and cometary water, or one enhanced from primordial value through an early hydrodynamic escap water (Leshin, 200”
• Thermal and crustal evolution of Mars (2002, methodology): “for KLB-1 of Zhang and Herzberg [1994] with the methodology for the calculation of partial melt developed by McKenzie and Bickle [1988] and McKenzie [1984].”
• The Sample Analysis at Mars Investigation and Instrument Suite (2012, background): “The D/H ratio of H2O in the martian atmosphere suggests that a significant fraction of the water that can exchange with the atmosphere has been lost to space (Leshin 2000) but perhaps liquid water still exists in deep subsurface aquifers.”