Results from the InSight atmospheric imaging campaign

• Published in: Icarus (New York, N.Y. 1962) N.Y. 1962), 2024-10, Vol.421, p.116248, Article 116248
• Main Authors: Lemmon, M.T., Campbell, C.L., Wolfe, C.A., Viúdez-Moreiras, D., Lorenz, R.D., Maki, J.N., Moores, J., Spiga, A., Banfield, D.
• Format: Article
• Language: English
• Subjects: Atmospheres, composition; Mars, atmosphere; Meteorology; Sciences of the Universe
• ISSN: 0019-1035; 1090-2643
• DOI: 10.1016/j.icarus.2024.116248

NASA's InSight lander monitored the Martian atmosphere while conducting its primarily geophysical investigation. Atmospheric imaging was used to study dust and ice at the site for over two Mars years in 2018–2022. An optical depth record, including dust and ice, was derived from systematic sky imaging in the mornings (for the first part of the mission) and evenings. Optical depths ranged from 0.5 to 1.9 but were typically under 1. Dust storms were seen at expected times in late northern autumn and early winter, including one shortly after landing, along with one late summer storm in January 2022. The optical depth record closely matched that of Curiosity, 600 km to the south, except for the expected additional water ice content during the aphelion cloud belt (ACB, spring to early summer). In addition to ice hazes, the ACB included discrete clouds, whose motion was tracked to show northeasterly to southeasterly daytime winds. While InSight recorded many meteorological vortices, no dust devils were seen, requiring that dust-devil occurrence was