Wei Zhu (祝伟)
Thursday group meeting
2020-07-09
Papers presenting dilute core models: Wahl et al. (2017); Debras & Chabrier (2019)
A recent review on Jupiter: Stevenson (2020)
\( V(r, \theta) = \frac{GM}{r} \left[ 1- \sum_{n=1} J_{2n} \left(\frac{a}{r}\right)^{2n} P_{2n} (\cos{\theta}) \right] \)
\(J_{2n}\): gravitational moments (zonal harmonic coefficients);
\(P_{2n}\): Legendre polynomial;
\(\theta\): angle to the rotational axis.
2016-2021
Image credit: James Tuttle Keane
Galileo satellite
Galileo entry probe
Image credit: NASA
Image credit: Stevenson (2020)
Immiscible liquid: oil on up of water
Image credit: Marley & Fortney, Encyclopedia of the Solar System
Image credit: Marley & Fortney, Encyclopedia of the Solar System
"Helium rain"
(Stevenson & Salpeter, 1977a, b)
Image credit: Hubbard & Militzer (2016)
$$ \nabla P = \rho \nabla (V_g+V_{cf}) $$
molecular layer
metallic layer
different entropy
"standard" model
A dilute core is preferred, in addition to an enhanced entropy offset or a reduced molecular layer metallicity (less likely).
Image credit: Stevenson (2020)