359 citations · 3.9k across the 46 of their papers we have counts for
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Constraining the interior of extrasolar giant planets with the tidal Love number k_2 using the example of HAT-P-13b
U. Kramm, N. Nettelmann, J. J. Fortney +2
Transit and radial velocity observations continuously discover an increasing number of exoplanets. However, when it comes to the composition of the observed planets the data are co…
Analysis of new high-precision transit light curves of WASP-10 b: starspot occultations, small planetary radius, and high metallicity
G. Maciejewski, St. Raetz, N. Nettelmann +4
The WASP-10 planetary system is intriguing because different values of radius have been reported for its transiting exoplanet. The host star exhibits activity in terms of photometr…
Jupiter models with improved ab initio hydrogen EOS (H-REOS.2)
Nadine Nettelmann, Andreas Becker, Bastian Holst +1
The amount and distribution of heavy elements in Jupiter gives indications on the process of its formation and evolution. Core mass and metallicity predictions however depend on th…
Predictions on the core mass of Jupiter and of giant planets in general
Nadine Nettelmann
More than 80 giant planets are known by mass and radius. Their interior structure in terms of core mass, number of layers, and composition however is still poorly known. An overvie…
Self-Consistent Model Atmospheres and the Cooling of the Solar System's Giant Planets
J. J. Fortney, M. Ikoma, N. Nettelmann +2
We compute grids of radiative-convective model atmospheres for Jupiter, Saturn, Uranus, and Neptune over a range of intrinsic fluxes and surface gravities. The atmosphere grids ser…