359 citations · 3.9k across the 46 of their papers we have counts for
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Jupiter's Interior with an Inverted Helium Gradient
Nadine Nettelmann, Jonathan J. Fortney
Jupiter's gravity field observed by NASA's Juno spacecraft indicates that the density in the 10--100 GPa region is lower than one would expect from a H/He adiabat with 0.5-5x solar…
Evolution of steam worlds: energetic aspects
Artyom Aguichine, Natalie Batalha, Jonathan J. Fortney +3
Sub-Neptunes occupy an intriguing region of planetary mass-radius space, where theoretical models of interior structure predict that they could be water-rich, where water is in ste…
H-HO demixing in Uranus and Neptune: Adiabatic structure models
Marina Cano Amoros, Nadine Nettelmann, Nicola Tosi +2
Demixing properties of planetary major constituents influence the interior structure and evolution of planets. Comparing experimental and computational data on the miscibility of h…
Atmospheric Helium Abundances in the Giant Planets
N. Nettelmann, M. Cano Amoros, N. Tosi +2
Noble gases are accreted to the giant planets as part of the gas component of the planet-forming disk. While heavier noble gases can separate from the evolution of the hydrogen-ric…
On the hypothesis of an inverted Z-gradient inside Jupiter
Saburo Howard, Tristan Guillot, Steve Markham +6
Models of Jupiter s interior struggle to agree with measurements of the atmospheric composition. Interior models favour a subsolar or solar abundance of heavy elements Z while atmo…
Estimating the number of planets that PLATO can detect
F. Matuszewski, N. Nettelmann, J. Cabrera +2
The PLATO mission is scheduled for launch in 2026. This study aims to estimate the number of exoplanets that PLATO can detect as a function of planetary size and period, stellar br…