The change in Jupiter's moment of inertia due to core erosion and planetary contraction

Ravit Helled*

*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

Abstract

We explore the change in Jupiter's normalized axial moment of inertia (NMOI) assuming that Jupiter undergoes core erosion. It is found that Jupiter's contraction combined with an erosion of 20 M from a primordial core of 30M can significantly change Jupiter's NMOI over time. It is shown that Jupiter's NMOI could have changed from 0.235 to 0.264 throughout its evolution. We find that an NMOI value of 0.235 as suggested by dynamical models could, in principle, be consistent with Jupiter's primordial internal structure. Low NMOI values, however, persist only for the first 106years of Jupiter's evolution. Re-evaluation of dynamical stability models as well as more sophisticated evolution models of Jupiter with core erosion seem to be required in order to provide more robust estimates for Jupiter's primordial NMOI.

Original languageEnglish
Article numberL16
JournalAstrophysical Journal Letters
Volume748
Issue number1
DOIs
StatePublished - 20 Mar 2012

Keywords

  • planets and satellites: dynamical evolution and stability
  • planets and satellites: formation
  • planets and satellites: individual (Jupiter)
  • planets and satellites: interiors
  • planets and satellites: physical evolution

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