Effect of non-adiabatic thermal profiles on the inferred compositions of Uranus and Neptune-Reference-Cited by-同舟云学术

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Effect of non-adiabatic thermal profiles on the inferred compositions of Uranus and Neptune

Published:2019-05-29 Issue:2 Volume:487 Page:2653-2664
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Podolak Morris¹^ORCID,Helled Ravit²,Schubert Gerald³

Affiliation:

1. Department of Geoscience, Tel-Aviv University, Tel Aviv, Israel 69978

2. Centre for Theoretical Physics and Cosmology, University of Zurich, Zurich, CH-8057 Switzerland

3. Department of Earth, Planetary and Space Sciences, University of California, Los Angeles, CA 90095-1567 USA

Funder

Swiss National Science Foundation

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/advance-article-pdf/doi/10.1093/mnras/stz1467/28739225/stz1467.pdf

Reference52 articles.

1. Saturn's very axisymmetric magnetic field: No detectable secular variation or tilt

2. New Models of Jupiter in the Context of Juno and Galileo

3. The Interior Structure, Composition, and Evolution of Giant Planets

4. Thermal conductivity of dissociating water—an ab initio study

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1. Uranus and Neptune as methane planets: Producing icy giants from refractory planetesimals;Icarus;2024-10

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3. GASTLI;Astronomy & Astrophysics;2024-08

4. Atmospheric Helium Abundances in the Giant Planets;Space Science Reviews;2024-07-29

5. Extensive Pollution of Uranus and Neptune’s Atmospheres by Upsweep of Icy Material during the Nice Model Migration;The Astronomical Journal;2024-07-09

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