The fuzzy cores of Jupiter and Saturn
Fuente:
arXiv
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| Autores principales: | , |
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| Formato: | Preprint |
| Publicado: |
2024
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| Acceso en línea: | |
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| _version_ | 1866916163911417856 |
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| author | Helled, Ravit Stevenson, David J. |
| author_facet | Helled, Ravit Stevenson, David J. |
| contents | New interior models of Jupiter and Saturn suggest that both planets have "fuzzy cores". These cores should be viewed as central regions that are enriched with heavy elements but are not distinct from the rest of the deep interior. These cores may contain large amounts of hydrogen and helium though small pure-heavy element cores may also exist. New measurements along with advanced planetary modeling have revolutionized the way we think about the interiors of giant planets and provide important constraints for planet formation and evolution theories. These developments are also relevant for the characterization of giant exoplanets. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2403_11657 |
| institution | arXiv |
| publishDate | 2024 |
| record_format | arxiv |
| spellingShingle | The fuzzy cores of Jupiter and Saturn Helled, Ravit Stevenson, David J. Earth and Planetary Astrophysics New interior models of Jupiter and Saturn suggest that both planets have "fuzzy cores". These cores should be viewed as central regions that are enriched with heavy elements but are not distinct from the rest of the deep interior. These cores may contain large amounts of hydrogen and helium though small pure-heavy element cores may also exist. New measurements along with advanced planetary modeling have revolutionized the way we think about the interiors of giant planets and provide important constraints for planet formation and evolution theories. These developments are also relevant for the characterization of giant exoplanets. |
| title | The fuzzy cores of Jupiter and Saturn |
| topic | Earth and Planetary Astrophysics |
| url | https://arxiv.org/abs/2403.11657 |