Results 61 to 70 of about 240,920 (191)
Ab initio free energy calculations are employed to derive the entropy of liquid and superionic water over a wide range of conditions in the interiors of Uranus and Neptune.
Burkhard Militzer
doaj +1 more source
Planetary Surface Instruments Workshop : held at Houston, Texas, May 12-13, 1995
This report on planetary surface investigations and planetary landers covers: the precise chemical analysis of solids; isotopes and evolved gas analyses; planetary interiors; planetary atmospheres from within as measured by landers; mineralogical ...
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Session B-1: Model building in Planetary Science and the NGSS [PDF]
In this session I will guide teachers through the steps my students take in Planetary Science to develop a conceptual model of how planetary interiors work.
Hawker, Eric
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The Linear Mixing Approximation in Silica–Water Mixtures at Planetary Conditions
The linear mixing approximation (LMA) is often used in planetary models for calculating the equations of state (EOS) of mixtures. A commonly assumed planetary composition is a mixture of rock and water. Here we assess the accuracy of the LMA for pressure–
Valiantsin Darafeyeu +3 more
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Improving Constraints on Planetary Interiors With PPs Receiver Functions. [PDF]
Kim D +17 more
europepmc +1 more source
Variations in the Radius Distribution of Single- and Compact Multiple-transiting Planets
Previous work has established the enhanced occurrence of compact systems of multiple small exoplanets around metal-poor stars. Understanding the origin of this effect in the planet formation process is a topic of ongoing research.
Benjamin T. Liberles +3 more
doaj +1 more source
Initial and present volatile inventories and distributions in the Earth, other planets, meteorites, and comets; observational evidence on the time history of volatile transfer among reservoirs; and volatiles in planetary bodies, their mechanisms of ...
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Using Array Seismology to Study Planetary Interiors [PDF]
: Stratification is a dominant feature of all planetary interiors. Fine-scale structure associated with layering, as well as heterogeneities hold important clues on a planet's compositional, thermal, and dynamical state, as well as its evolution.
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Accelerating the Discovery of Steady‐States of Planetary Interior Dynamics With Machine Learning
Simulating mantle convection often requires reaching a computationally expensive steady‐state, crucial for deriving scaling laws for thermal and dynamical flow properties and benchmarking numerical solutions.
Siddhant Agarwal +4 more
doaj +1 more source
Constraining the interiors of exoplanets by measuring the Love number k2,f
This talk summarizes how the Love-numbers can be used to constrain the planetary interiors, how we can measure the exoplanetary Love-numbers and what precision can be ...
Hellard, Hugo, Csizmadia, Szilard
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