Search Results - "NETTELMANN, NADINE"

Uranus and Neptune: Origin, Evolution and Internal Structure by Helled, Ravit, Nettelmann, Nadine, Guillot, Tristan

“…There are still many open questions regarding the nature of Uranus and Neptune, the outermost planets in the Solar System. In this review we summarize the…”
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Stardust in the deep interior of low-mass planets by Nettelmann, Nadine

“…The behaviour of minerals under high pressure affects the bulk properties of exoplanets and planets with rocky components, possibly influencing their…”
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The Interior Structure, Composition, and Evolution of Giant Planets by Fortney, Jonathan J., Nettelmann, Nadine

“…We discuss our current understanding of the interior structure and thermal evolution of giant planets. This includes the gas giants, such as Jupiter and…”
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A FRAMEWORK FOR CHARACTERIZING THE ATMOSPHERES OF LOW-MASS LOW-DENSITY TRANSITING PLANETS by tney, Jonathan J, Mordasini, Christoph, NETTELMANN, NADINE, Kempton, Eliza M-R, Greene, Thomas P, ZAHNLE, KEVIN

“…We perform modeling investigations to aid in understanding the atmospheres and composition of small planets of ~2-4 Earth radii, which are now known to be…”
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Machine-learning Inference of the Interior Structure of Low-mass Exoplanets by Baumeister, Philipp, Padovan, Sebastiano, Tosi, Nicola, Montavon, Grégoire, Nettelmann, Nadine, MacKenzie, Jasmine, Godolt, Mareike

“…We explore the application of machine-learning based on mixture density neural networks (MDNs) to the interior characterization of low-mass exoplanets up to 25…”
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The phase diagram of water and the magnetic fields of Uranus and Neptune by Redmer, Ronald, Mattsson, Thomas R., Nettelmann, Nadine, French, Martin

“…The interior of giant planets can give valuable information on formation and evolution processes of planetary systems. However, the interior and evolution of…”
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Ab Initio Equation of State Data for Hydrogen, Helium, and Water and the Internal Structure of Jupiter by Nettelmann, Nadine, Holst, Bastian, Kietzmann, André, French, Martin, Redmer, Ronald, Blaschke, David

“…The equation of state of hydrogen, helium, and water affects interior structure models of giant planets significantly. We present a new equation of state data…”
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H/He demixing and the cooling behavior of Saturn by Püstow, Robert, Nettelmann, Nadine, Lorenzen, Winfried, Redmer, Ronald

“…•The evolution of Saturn is computed using ab initio H/He phase diagram and EOS data.•Our adiabatic models predict a thick (∼0.1 RS, ∼10 ME) He-rich layer…”
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The Effect of Clouds as an Additional Opacity Source on the Inferred Metallicity of Giant Exoplanets by Poser, Anna Julia, Nettelmann, Nadine, Redmer, Ronald

“…Atmospheres regulate the planetary heat loss and therefore influence planetary thermal evolution. Uncertainty in a giant planet’s thermal state contributes to…”
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Equation of state and phase diagram of water at ultrahigh pressures as in planetary interiors by French, Martin, Mattsson, Thomas R., Nettelmann, Nadine, Redmer, Ronald

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Viscosity and Prandtl Number of Warm Dense Water as in Ice Giant Planets by French, Martin, Nettelmann, Nadine

“…The thermophysical properties in water-rich planets are important for understanding their radius, luminosity, and magnetic field. Here we calculate the shear…”
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Predictions on the core mass of Jupiter and of giant planets in general by Nettelmann, Nadine

“…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…”
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Revelations on Jupiter's formation, evolution and interior: Challenges from Juno results by Helled, Ravit, Stevenson, David J., Lunine, Jonathan I., Bolton, Scott J., Nettelmann, Nadine, Atreya, Sushil, Guillot, Tristan, Militzer, Burkhard, Miguel, Yamila, Hubbard, William B.

“…The Juno mission has revolutionized and challenged our understanding of Jupiter. As Juno transitioned into its extended mission, we review the major findings…”
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Saturn layered structure and homogeneous evolution models with different EOSs by Nettelmann, Nadine, Püstow, Robert, Redmer, Ronald

“…•Saturn’s core mass is little influenced by the H–He EOS and ranges from 0 to 20ME.•Our ab initio EOS data based Saturn models predict an O:H ratio of at most…”
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Magnetic induction processes in hot Jupiters, application to KELT-9b by Dietrich, Wieland, Kumar, Sandeep, Poser, Anna Julia, French, Martin, Nettelmann, Nadine, Redmer, Ronald, Wicht, Johannes

“…Abstract The small semimajor axes of hot Jupiters lead to high atmospheric temperatures of up to several thousand Kelvin. Under these conditions, thermally…”
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Atmospheric Helium Abundances in the Giant Planets by Nettelmann, Nadine, Cano Amoros, Marina, Tosi, Nicola, Helled, Ravit, Fortney, Jonathan J.

“…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…”
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Uranus evolution models with simple thermal boundary layers by Nettelmann, N., Wang, K., Fortney, J.J., Hamel, S., Yellamilli, S., Bethkenhagen, M., Redmer, R.

“…•Thermal boundary between H/He-rich and ice-rich shells can explain the low luminosity.•We suggest that atmospheric thermal equilibrium with the incident flux…”
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Isentropic compression of hydrogen: Probing conditions deep in planetary interiors by Becker, Andreas, Nettelmann, Nadine, Holst, Bastian, Redmer, Ronald

“…We perform ab initio calculations for the equation of state of dense liquid hydrogen and deuterium using quantum molecular dynamics simulations based on…”
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Forward and inverse modeling for jovian seismology by Jackiewicz, Jason, Nettelmann, Nadine, Marley, Mark, Fortney, Jonathan

“…► Jupiter is expected to oscillate in a spectrum of acoustic modes. ► These oscillations can help greatly improve and constrain interiors models. ► We use new…”
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The Interior Structure, Composition, and Evolution ofGiant Planets by tney, Jonathan J, Nettelmann, Nadine

“…We discuss our current understanding of the interior structure and thermal evolution of giant planets. This includes the gas giants, such as Jupiter and…”
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