Monte Carlo interior models for Uranus and Neptune

M. S. Marley, P. Gomez, M. Podolak

Research output: Contribution to journalArticlepeer-review

37 Scopus citations

Abstract

To explore a greater realm of model phase space than has previously been mapped, randomly chosen interior models are generated for Uranus and Neptune. The models are constrained by the observed mass, rotation rate, radius, and gravitational moments of the two planets. New models with a composition gradient in the outer third of the planetary radius are found for both planets. Such composition gradients may play a significant role in controlling the internal heat flow. In agreement with previous models, it is found that the pressure-density relation for the central third of both planets is consistent with either ice or a mixture of materials with a similar equation of state. -from Authors

Original languageEnglish (US)
Pages (from-to)23,349-23,353
JournalJournal of geophysical research
Volume100
Issue numberE11
DOIs
StatePublished - 1995
Externally publishedYes

ASJC Scopus subject areas

  • Geophysics
  • Forestry
  • Oceanography
  • Aquatic Science
  • Ecology
  • Water Science and Technology
  • Soil Science
  • Geochemistry and Petrology
  • Earth-Surface Processes
  • Atmospheric Science
  • Earth and Planetary Sciences (miscellaneous)
  • Space and Planetary Science
  • Palaeontology

Fingerprint

Dive into the research topics of 'Monte Carlo interior models for Uranus and Neptune'. Together they form a unique fingerprint.

Cite this