Work

Uranus evolution models with simple thermal boundary layers

Year: 2016

Type: article

Source: Icarus

DOI: 10.1016/j.icarus.2016.04.008

Authors: N. Nettelmann, K. Wang, J.J. Fortney, S. Hamel, S. Yellamilli, M. Bethkenhagen, R. Redmer

Institutions: University of California, Santa Cruz, University of Rostock, Lawrence Livermore National Laboratory, University of California, Berkeley

Language: English

Topic: Astro and Planetary Science

Subfield: Space and Planetary Science

Field: Earth and Planetary Sciences

Domain: Physical Sciences

Open Access status: green

Funders: National Science Foundation, National Aeronautics and Space Administration, Deutsche Forschungsgemeinschaft, Universität Rostock

Awards: A New Era of Modeling Giant Planet Thermal Evolution, WE PROPOSE TO COMPUTE NEW MODELS OF THE THERMAL EVOLUTION OF URANUS AND NEPTUNE. THE COOLING OF THESE PLANETS IS STILL NOT WELL UNDERSTOOD AS NEPTUNE, G5620122118, G7729037743

OpenAlex ID: W2336371268

FWCI: 8.385

Cites: 70

Cited by: 122

Related to: 10