Effects of Albedo on the MIR Emissivity Spectra of Silicates for Lunar Comparison

Journal of Geophysical Research Planets American Geophysical Union (AGU) 128:4 (2023)

Authors:

KA Shirley, TD Glotch, O Donaldson, J Trelewicz, Y Yang, H Zhang

Short Period Seismometer for the Lunar Farside Seismic Suite Mission

Institute of Electrical and Electronics Engineers (IEEE) 00 (2023) 1-9

Authors:

Ian M Standley, William T Pike, Simon Calcutt, James P Hoffman

The Roasting Marshmallows Program with IGRINS on Gemini South I: Composition and Climate of the Ultrahot Jupiter WASP-18 b

The Astronomical Journal American Astronomical Society 165:3 (2023) 91

Authors:

Matteo Brogi, Vanessa Emeka-Okafor, Michael R Line, Siddharth Gandhi, Lorenzo Pino, Eliza M-R Kempton, Emily Rauscher, Vivien Parmentier, Jacob L Bean, Gregory N Mace, Nicolas B Cowan, Evgenya Shkolnik, Joost P Wardenier, Megan Mansfield, Luis Welbanks, Peter Smith, Jonathan J Fortney, Jayne L Birkby, Joseph A Zalesky, Lisa Dang, Jennifer Patience, Jean-Michel Désert

The Habitability of Venus

Space Science Reviews Springer Nature 219:2 (2023) 17

Authors:

F Westall, D Höning, G Avice, D Gentry, T Gerya, C Gillmann, N Izenberg, MJ Way, C Wilson

Quantification of carbonates, oxychlorines, and chlorine generated by heterogeneous electrochemistry induced by Martian dust activity

Geophysical Research Letters American Geophysical Union 50:4 (2023) e2022GL102127

Authors:

Alian Wang, Andrew W Jackson, Neil C Sturchio, Jen Houghton, Chuck YC Yan, Kevin S Olsen, Quincy HK Qu

Abstract:

Heterogeneous electrochemistry induced by Martian dust activity is an important type of atmosphere-surface interaction that affects geochemical processes at the Martian surface and in the Martian atmosphere. We have experimentally demonstrated that heterogeneous electrochemistry stimulated by mid-strength dust events can decompose common chloride salts, which is accompanied by the release of chlorine atoms into the atmosphere and the generation of (per)chlorates (chlorates and perchlorates) and carbonates. In this study, we present quantitative analyses on the above products from 26 heterogeneous electrochemical experiments on chloride salts. Based on these quantifications, our calculation indicates that such atmosphere-surface interaction during a portion of Amazonian period could accumulate the observed abundance of (per)chlorates, carbonates, and HCl by landed and orbital missions, and thus can be considered as a major driving force of the global chlorine-cycle on Mars. This study emphasizes the importance of measuring the electrical properties of dust activity on Mars.