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.

Venus, the Planet: Introduction to the Evolution of Earth’s Sister Planet

Space Science Reviews Springer 219:1 (2023) 10

Authors:

Joseph G O’Rourke, Colin F Wilson, Madison E Borrelli, Paul K Byrne, Caroline Dumoulin, Richard Ghail, Anna JP Gülcher, Seth A Jacobson, Oleg Korablev, Tilman Spohn, MJ Way, Matt Weller, Frances Westall

Abstract:

Misconceptions are understandings of concepts that are not in accordance with scientific concepts. Teachers have the potential to experience misconceptions and misconceptions that occur in teachers can result in students also experiencing misconceptions. Research that examines science misconceptions in elementary school teachers is still rare, so there is a need for research examining science misconceptions in elementary school teachers, especially in elementary school teachers who are certified educators. Therefore, this study aims at determining whether science misconceptions occur in elementary school teachers with teaching certificates or not and how much misconceptions are experienced and the misconceptions occurred. This study employs descriptive quantitative by involving 17 certified elementary school teachers who are classroom teachers teaching several subjects in elementary schools including science subjects. Data collection was done by conducting a four tier misconception diagnosis test and the result was analyzed using by referring to four tier test concept developed by various researchers. The findings indicated that primary school teachers possessing teaching certificates exhibited science misconceptions at a rate of 22%, placing them in the low category of scientific understanding at 66%. Despite the relatively low occurrence of misconceptions, it is advisable for certified primary school teachers to further enhance their grasp of the concepts they impart to prevent any potential hindrance to the learning process

Reanalyzing Jupiter ISO/SWS Data through a More Recent Atmospheric Model

ATMOSPHERE 14:12 (2023) ARTN 1731

Authors:

Jose Ribeiro, Pedro Machado, Santiago Perez-Hoyos, Joao A Dias, Patrick Irwin, Elizabeth A Silber, George Balasis

Abstract:

The study of isotopic ratios in planetary atmospheres gives an insight into the formation history and evolution of these objects. The more we can constrain these ratios, the better we can understand the history and future of our solar system. To help in this endeavour, we used Infrared Space Observatory Short Wavelength Spectrometer (ISO/SWS) Jupiter observations in the 793–1500 cm (Formula presented.) region together with the Nonlinear Optimal Estimator for MultivariatE Spectral analySIS (NEMESIS) radiative transfer suite to retrieve the temperature–pressure profile and the chemical abundances for various chemical species. We also used the 1500–2499 cm (Formula presented.) region to determine the cloud and aerosol structure of the upper troposphere. We obtained a best-fit simulated spectrum with (Formula presented.) for the 793–1500 cm (Formula presented.) region and (Formula presented.) for the 1500–2499 cm (Formula presented.) region. From the retrieved methane abundances, we obtained, within a 1 (Formula presented.) uncertainty, a (Formula presented.) C/ (Formula presented.) C ratio of 84 ± 27 and a D/H ratio of (3.5 ± 0.6) × 10 (Formula presented.), and these ratios are consistent with other published results from the literature.

Venus Express

Chapter in Encyclopedia of Astrobiology Third Edition, (2023) 3171-3183

Authors:

D Titov, H Svedhem, C Wilson

HCO+ Dissociative Recombination: A Significant Driver of Nonthermal Hydrogen Loss at Mars

Journal of Geophysical Research Planets American Geophysical Union (AGU) 128:1 (2023)

Authors:

Bethan S Gregory, Rodney D Elliott, Justin Deighan, Hannes Gröller, Michael S Chaffin