Jupiter internal structure: the effect of different equations\n of state Article Swipe
Yamila Miguel
,
T. Guillot
,
Lucile Fayon
·
YOU?
·
· 2016
· Open Access
·
· DOI: https://doi.org/10.1051/0004-6361/201629732/pdf
YOU?
·
· 2016
· Open Access
·
· DOI: https://doi.org/10.1051/0004-6361/201629732/pdf
\n Context. Heavy elements, even though they are a smaller constituent, are\n crucial to understand the formation history of Jupiter. Interior models are used to\n determine the amount of heavy elements in the interior of Jupiter, but this range is still\n subject to degeneracies because of the uncertainties in the equations of state.\n Aims. Before Juno mission data arrive, we present optimized calculations\n for Jupiter that explore the effect of different model parameters on the determination of\n the core and the mass of heavy elements of Jupiter. We compare recently published\n equations of state.\n Methods. The interior model of Jupiter was calculated from the equations\n of hydrostatic equilibrium, mass, and energy conservation, and energy transport. The mass\n of the core and heavy elements was adjusted to match the observed radius and gravitational\n moments of Jupiter.\n Results. We show that the determination of the interior structure of\n Jupiter is tied to the estimation of its gravitational moments and the accuracy of\n equations of state of hydrogen, helium, and heavy elements. Locating the region where\n helium rain occurs and defining its timescale is important to determine the distribution\n of heavy elements and helium in the interior of Jupiter. We show that the differences\n found when modeling the interior of Jupiter with recent EOS are more likely due to\n differences in the internal energy and entropy calculation. The consequent changes in the\n thermal profile lead to different estimates of the mass of the core and heavy elements,\n which explains differences in recently published interior models of Jupiter.\n Conclusions. Our results help clarify the reasons for the differences\n found in interior models of Jupiter and will help interpreting upcoming Juno data.\n
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Metadata
- Type
- article
- Language
- en
- https://www.aanda.org/10.1051/0004-6361/201629732/pdf
- OA Status
- green
- Cited By
- 106
- References
- 55
- Related Works
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- OpenAlex ID
- https://openalex.org/W3099941838
All OpenAlex metadata
Raw OpenAlex JSON
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https://openalex.org/W3099941838Canonical identifier for this work in OpenAlex
- DOI
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https://doi.org/10.1051/0004-6361/201629732/pdfDigital Object Identifier
- Title
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Jupiter internal structure: the effect of different equations\n of stateWork title
- Type
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articleOpenAlex work type
- Language
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enPrimary language
- Publication year
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2016Year of publication
- Publication date
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2016-12-14Full publication date if available
- Authors
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Yamila Miguel, T. Guillot, Lucile FayonList of authors in order
- PDF URL
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https://www.aanda.org/10.1051/0004-6361/201629732/pdfDirect link to full text PDF
- Open access
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YesWhether a free full text is available
- OA status
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greenOpen access status per OpenAlex
- OA URL
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https://www.aanda.org/10.1051/0004-6361/201629732/pdfDirect OA link when available
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Jupiter (rocket family), Context (archaeology), Equation of state, State (computer science), Physics, Range (aeronautics), Astrobiology, Astronomy, Geology, Mathematics, Thermodynamics, Spacecraft, Aerospace engineering, Engineering, Algorithm, PaleontologyTop concepts (fields/topics) attached by OpenAlex
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106Total citation count in OpenAlex
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2025: 4, 2024: 5, 2023: 13, 2022: 9, 2021: 9Per-year citation counts (last 5 years)
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55Number of works referenced by this work
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10Other works algorithmically related by OpenAlex
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