Internal structure and cryovolcanism on Trans-Neptunian objects

Aurélie Guilbert-Lepoutre, Dina Prialnik, Robin Métayer

Research output: Chapter in Book/Report/Conference proceedingChapterpeer-review

Abstract

Modeling the evolution and internal structure of large- and mid-size Trans-Neptunian objects (TNOs) is a challenging task, owing to the strong dependence on the thermophysical and structural parameters involved, which are poorly constrained. Thus the outcome of evolutionary tracks for a given object may range from fully pristine to completely differentiated and need to be further constrained by detailed observations of TNOs’ physical and chemical properties. The key question remains, whether knowing surface and bulk properties is sufficient for inferring internal properties and more ambitiously, the evolutionary course of a TNO from formation to present day. Recent models of Charon involve a complex evolution, including the formation of subsurface oceans and past cryovolcanism. This perspective should trigger the development of new comprehensive models, which-combined with new observations-should lead to significant progress in our understanding of how the whole population formed and evolved.

Original languageEnglish
Title of host publicationThe Trans-Neptunian Solar System
PublisherElsevier
Pages183-201
Number of pages19
ISBN (Electronic)9780128164907
DOIs
StatePublished - 1 Jan 2019

Keywords

  • Heat conduction
  • Interiors
  • Kuiper belt: general
  • Methods: numerical
  • Minor planets: general

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