Anomalous transient enhancement of planetary ion escape at Mars

Atmospheric ion escape plays a crucial role in the evolution of planetary climate and habitability. While Mars has been the focus of extensive in-situ spacecraft observations, our understanding of ion escape at Mars has been constrained by single-point spacecraft measurements, which fail to distinguish spatial and temporal variability. Observations from NASA's Mars Atmosphere and Volatile EvolutioN (MAVEN) mission and China's Tianwen-1 mission provide complementary observations the Martian space environment and a unique opportunity to study the variability of ion escape. Here, we report that ion escape at Mars exhibits unexpected spatial-temporal variability under steady and weak external solar wind conditions. In the hemisphere where the solar wind electric field is directed toward the planet, a condition that usually hinders ion escape into space, we instead observe the transient appearance of escaping planetary ions with high energies and strong escape fluxes. This finding underscores that planetary ion escape can be unsteady and dynamic, even under stable external conditions.

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Publication Details

Journal
Nature Communications
Published
2025-04-02
DOI
https://doi.org/10.1038/s41467-025-58351-y
Citations
6
Primary Topic
Planetary Science and Exploration
Type
article
Field-Weighted Citation Impact
6.93

Funders

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article

Anomalous transient enhancement of planetary ion escape at Mars

K. G. Hanley, Hongyang Zhou, Muni Zhou, Mats Holmström et al.
6 citations
Nature Communications
Planetary Science and Exploration
6.93
article

Anomalous transient enhancement of planetary ion escape at Mars

K. G. Hanley, Hongyang Zhou, Muni Zhou, Mats Holmström, Shannon Curry, J. S. Halekas, Terry Z. Liu, Moa Persson, Chi Zhang, H. Nilsson, Yoshifumi Futaana, Yuxi Chen, Li‐Jen Chen, Y. Dong, Robin Ramstad, Chuanfei Dong, S. Ruhunusiri, M. Yamauchi, Shaosui Xu, C. Mazelle
article en
6 citations

Abstract

Atmospheric ion escape plays a crucial role in the evolution of planetary climate and habitability. While Mars has been the focus of extensive in-situ spacecraft observations, our understanding of ion escape at Mars has been constrained by single-point spacecraft measurements, which fail to distinguish spatial and temporal variability. Observations from NASA's Mars Atmosphere and Volatile EvolutioN (MAVEN) mission and China's Tianwen-1 mission provide complementary observations the Martian space environment and a unique opportunity to study the variability of ion escape. Here, we report that ion escape at Mars exhibits unexpected spatial-temporal variability under steady and weak external solar wind conditions. In the hemisphere where the solar wind electric field is directed toward the planet, a condition that usually hinders ion escape into space, we instead observe the transient appearance of escaping planetary ions with high energies and strong escape fluxes. This finding underscores that planetary ion escape can be unsteady and dynamic, even under stable external conditions.

Nature CommunicationsVol. 16(1)
Dartmouth College (US), Boston University (US), University of Iowa (US), Centre National de la Recherche Scientifique (FR), Planetary Science Institute (US), Goddard Space Flight Center (US), Swedish Institute of Space Physics (SE), Université Toulouse III - Paul Sabatier (FR), University of California, Los Angeles (US), Université Fédérale de Toulouse Midi-Pyrénées (FR), University of Colorado Boulder (US), University of Michigan (US), Laboratory for Atmospheric and Space Physics (US), Astronomy and Space (AU), University of California, Berkeley (US)
National Aeronautics and Space Administration, Nuclear Safety and Security Commission
Climate action
Openalex Percentile: Top 3%
Planetary Science and Exploration
6.93
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