Water storage capacity of the martian mantle through time
Water storage capacity of the martian mantle through time
复制标题
火星地幔随时间变化的储水能力
DOI:
10.1016/j.icarus.2022.115113
复制
发表时间:
2022
期刊:
影响因子:
3.2
通讯作者:
Brennan, Matthew C.
中科院分区:
文献类型:
--
作者:
Dong, Junjie;Fischer, Rebecca A.;Stixrude, Lars P.;Lithgow-Bertelloni, Carolina R.;Eriksen, Zachary T.;Brennan, Matthew C.
Water has been stored in the Martian mantle since its formation, primarily in nominally anhydrous minerals. The short-lived early hydrosphere and intermittently flowing water on the Martian surface may have been supplied and replenished by magmatic degassing of water from the mantle. Estimating the water storage capacity of the solid Martian mantle places important constraints on its water inventory and helps elucidate the sources, sinks, and temporal variations of water on Mars. In this study, we applied a bootstrap aggregation method to investigate the effects of iron on water storage capacities in olivine, wadsleyite, and ringwoodite, based on high-pressure experimental data compiled from the literature, and we provided a quantitative estimate of the upper bound of the bulk water storage capacity in the FeO-rich solid Martian mantle. Along a series of areotherms at different mantle potential temperatures (Tp), we estimated a water storage capacity equal to 9.0−2.2+2.8km Global Equivalent Layer (GEL) for the present-day Martian mantle atTp= 1600 K and 4.9−1.5+1.7km GEL for the initial Martian mantle atTp= 1900 K. The water storage capacity of the Martian mantle increases with secular cooling through time, but due to the lack of an efficient water recycling mechanism on Mars, its actual mantle water content may be significantly lower than its water storage capacity today.