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The Methane Diurnal Variation and Microseepage Flux at Gale Crater, Mars as Constrained by the ExoMars Trace Gas Orbiter and Curiosity Observations

John E. Moores, Penelope L. King, Christina L. Smith et al., 2019. Geophysical Research Letters 46(16), 9430–9438.

Proposes that methane seeping from the ground accumulates within metres of the surface at night, when mixing is suppressed, and is diluted below detection at dawn; derives a constant seepage of 1.5 × 10⁻¹⁰ kg m⁻² per sol and notes that only 2.7 × 10⁴ km² of Mars could be emitting unless a fast destruction exists.

MYS0D7EXRJT3793 · mystery · click to copyMMars methane puzzleArticledoi: 10.1029/2019gl083800Checked against the original0

What it's used for here

The night-time containment model.

Cited by on this site 4 records

Cite it

Moores, J. E., King, P. L., Smith, C. L., Martinez, G. M., & et al. (2019). The Methane Diurnal Variation and Microseepage Flux at Gale Crater, Mars as Constrained by the ExoMars Trace Gas Orbiter and Curiosity Observations. Geophysical Research Letters 46(16), 9430–9438. https://doi.org/10.1029/2019gl083800
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