Internal Heat Flux and Energy Imbalance of Uranus

Abstract With its extreme axial tilt, Uranus' radiant energy budget (REB) and internal heat flux remain among the most intriguing mysteries in our solar system. By combining observations with modeling, we present the global REB over a complete orbital period (1946–2030), revealing significant seasonal variations. Despite these fluctuations, the global average emitted thermal power consistently exceeds absorbed solar power, indicating a net energy loss. Assuming no significant seasonal variation in emitted power, we estimate an internal heat flux of 0.078 ± 0.018 W/m 2 by analyzing the energy budget over one orbital period. The combination of internal heat and radiant energies indicates substantial global and hemispheric imbalances, with excesses or deficits exceeding 85% of emitted power at the hemispheric scale. These findings are crucial for understanding Uranus' interior and atmosphere. A future flagship mission to Uranus would provide critical observations to address more unresolved questions of this enigmatic ice giant.

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Publication Details

Journal
Geophysical Research Letters
Published
2025-07-14
DOI
https://doi.org/10.1029/2025gl115660
Citations
2
Primary Topic
Astro and Planetary Science
Type
article
Field-Weighted Citation Impact
2.31

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article

Internal Heat Flux and Energy Imbalance of Uranus

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article

Internal Heat Flux and Energy Imbalance of Uranus

Gwenaël Milcareck, Agustín Sánchez-Lavega, S. Pérez‐Hoyos, R. Hueso, Xun Jiang, C. A. Nixon, T. Guillot, Liming Li, Ulyana A. Dyudina, P. M. Fry, Michael T. Roman, Xinyue Wang, Cheng Li, Xi Zhang, Robert A. West, Matthew Kenyon
article en
2 citations

Abstract

Abstract With its extreme axial tilt, Uranus' radiant energy budget (REB) and internal heat flux remain among the most intriguing mysteries in our solar system. By combining observations with modeling, we present the global REB over a complete orbital period (1946–2030), revealing significant seasonal variations. Despite these fluctuations, the global average emitted thermal power consistently exceeds absorbed solar power, indicating a net energy loss. Assuming no significant seasonal variation in emitted power, we estimate an internal heat flux of 0.078 ± 0.018 W/m 2 by analyzing the energy budget over one orbital period. The combination of internal heat and radiant energies indicates substantial global and hemispheric imbalances, with excesses or deficits exceeding 85% of emitted power at the hemispheric scale. These findings are crucial for understanding Uranus' interior and atmosphere. A future flagship mission to Uranus would provide critical observations to address more unresolved questions of this enigmatic ice giant.

Geophysical Research LettersVol. 52(14)
Centre National de la Recherche Scientifique (FR), Space Science Institute (US), Planetary Science Institute (US), Goddard Space Flight Center (US), Jet Propulsion Laboratory (US), University of Wisconsin–Madison (US), University of Leicester (GB), University of the Basque Country (ES), Université Paris Sciences et Lettres (FR), University of Michigan (US), Sorbonne Université (FR), Lagrange Laboratory (FR), Ente Vasco de la Energía (ES), Observatoire de la Côte d’Azur (FR), University of Houston (US)
National Science Foundation, National Aeronautics and Space Administration, Indian Council of Agricultural Research, Nuclear Safety and Security Commission
Affordable and clean energy
Openalex Percentile: Top 11%
Astro and Planetary Science
2.31
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