Martian Atmospheric Methane
Instruments on Mars have detected seasonal fluctuations in atmospheric methane (), peaking during the Martian summer. Two scientists propose differing explanations for the source and release mechanism of this methane.
Scientist 1
The seasonal methane spikes are caused by the destabilization of subsurface methane clathrates (crystalline water-based solids physically trapping methane gas). These clathrates were formed billions of years ago when Mars possessed abundant surface water. Under current Martian conditions, clathrates are only thermodynamically stable at depths of or more. During the Martian summer, solar heating warms the upper regolith, sending a thermal wave downward that destabilizes the uppermost clathrates, releasing the trapped , which diffuses through the porous soil into the atmosphere.
Scientist 2
The methane is produced abiotically by modern serpentinization—a geochemical reaction between liquid water and olivine-rich rock. This reaction occurs in the deep crust ( depth) where geothermal heat keeps water liquid. The generated gas accumulates in deep geologic traps. During the Martian summer, the peak gravitational tidal forces exerted by Mars's moons deform the crust, reopening micro-fractures and allowing the pressurized methane to rapidly escape to the surface.
Which of the following is an underlying assumption of Scientist 1's explanation but NOT of Scientist 2's explanation?
- The seasonal temperature variation on Mars penetrates the regolith to a depth of at least with sufficient intensity to destabilize clathrates.Cevap
- BMethane clathrates are abiotically replenished by active serpentinization occurring at depths shallower than .
- CThe thermal stability of methane clathrates is completely independent of the ambient temperature of the surrounding regolith.
- DCrustal deformation caused by the tidal forces of Mars's moons is strongest during the Martian winter.