Can Radio Occultations Constrain Uranus or Neptune’s Internal Rotation Periods?
The shapes of fluid planets bear the signatures of rotational flattening and atmospheric flows. Precise knowledge of their shapes and wind profiles may therefore reveal their interior rotation rates. We reexamine this idea for the ice giants, where missions like the Uranus Orbiter and Probe could us...
Bewaard in:
| Hoofdauteurs: | , , , , |
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| Formaat: | Artigo |
| Taal: | Inglês |
| Gepubliceerd in: |
IOP Publishing
2026-01-01
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| Reeks: | The Planetary Science Journal |
| Onderwerpen: | |
| Online toegang: | https://doi.org/10.3847/PSJ/ae6251 |
| Tags: |
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