Sound propagation on Mars differs from Earth due to carbon dioxide atmosphere
Recent in-situ acoustic recordings and modeling confirm that sound propagation on Mars differs significantly from Earth due to its carbon dioxide atmosphere and low pressure.
The retrieved papers include direct in-situ measurements and modeling of Martian acoustics using data from the Perseverance rover, confirming distinct sound speeds, attenuation, and vibrational relaxation effects linked to the carbon dioxide-dominated atmosphere.
Maurice S, Chide B, Murdoch N, Lorenz RD, Mimoun D, Wiens RC, Stott A, Jacob X, Bertrand T, Montmessin F, Lanza NL, Alvarez-Llamas C, Angel SM, Aung M, Balaram J, Beyssac O, Cousin A, Delory G, Forni O, Fouchet T, Gasnault O, Grip H, Hecht M, Hoffman J, Laserna J, Lasue J, Maki J, McClean J, Meslin PY, Le Mouélic S, Munguira A, Newman CE, Rodríguez Manfredi JA, Moros J, Ollila A, Pilleri P, Schröder S, de la Torre Juárez M, Tzanetos T, Stack KM, Farley K, Williford K. In situ recording of Mars soundscape.. 2022. https://doi.org/10.1038/s41586-022-04679-0
This study uses Perseverance microphone recordings to confirm unique acoustic properties in Mars's carbon dioxide atmosphere, such as frequency-dependent sound speeds and high-frequency attenuation.
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Martin Gillier, Andi Petculescu, Naomi Murdoch, Alexander E. Stott, Solène Gerier, Sylvestre Maurice, David Mimoun. Geographical, Seasonal and Diurnal Variations of Acoustic Attenuation, and Sound Speed in the Near‐Surface Martian Atmosphere. 2024. https://doi.org/10.1029/2023je008257
This paper models sound attenuation and speed in the Martian atmosphere, explicitly accounting for the effects of carbon dioxide concentrations on acoustic properties.
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