Why do Jupiter models want fewer heavy elements than its atmosphere shows? · revision history
Revision 2
Accepted · core change · record
Changes against revision 1:
- Title
- Why do Jupiter models want fewer heavy elements than its atmosphere shows?
- Plain
- The Galileo probe measured an atmosphere enriched in heavy elements, but many interior models that fit Juno's gravity need a less enriched outer layer. Either the models or the assumed relation between pressure, temperature and density of hydrogen-helium (the equation of state) is wrong, or the planet has an unexpected layering.
- Precise · changed · core
- Revision 1: The Galileo probe found atmospheric heavy-element enrichment of roughly three times solar, while many Juno-fitting interior models require a lower $Z$ in the outer envelope, implying an inverted $Z$ gradient. Determine whether this tension arises from hydrogen-helium equation-of-state errors, deep wind effects on gravity, or a real compositional inversion. An answer is an interior model with atmospheric $Z$ that fits J_2n and $k_2$, or a demonstration that the inversion is required.
- Revision 2: The Galileo probe found atmospheric heavy-element enrichment of roughly three times solar, while many Juno-fitting interior models require a lower $Z$ in the outer envelope, implying an inverted $Z$ gradient. Determine whether this tension arises from hydrogen-helium equation-of-state errors, deep wind effects on gravity, or a real compositional inversion. An answer is an interior model with atmospheric $Z$ that fits $J_2n$ and $k_2$, or a demonstration that the inversion is required.
- Settled by
- Interior models using independently validated equations of state and wind-corrected gravity harmonics that either remove or require the inversion.
- Kind
- well-posed
- Answer type
- identification
- References
- (empty)
- Literature status
- open
- Status note
- (empty)
- Posed since
- (empty)
Decisions
- Accept · 2026-10-15 · record