The thermal emission of Kuiper Belt objects

Nicolas Thomas*, Alan Fitzsimmons, Wing Huen Ip

*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

3 Citations (Scopus)

Abstract

A thermophysical model, previously used to compute the surface tempeature distribution of spherical asteroids taking into account thermal inertia and rotational characteristics, has been developed to incorproate tri-axial ellipsoidal geometry and arbitrary spin axis orientation. The numerical model has been used to predict the thermal IR fluxes from Kuiper Belt objects (KBOs), particularly at wavelengths at which detection by the ISOPHOT instrument on ISO appears feasible. The dependence of the fluxes on the magnitude of a thermal parameter, the orientation of the spin axis, and the ratio of the major and minor axes are described for an assumed prolate ellipsoid. Comparisons with ground-based observation of 2060 Chiron are made showing that values of the thermal parameter less than I can be reconciled with the data. The effects of sublimation have been incorporated into the model and it is shown that sublimation of CO2 ice KBOs will have little effect on the surface temperature while out-gassing rates in excess: of 1016 molecule m-2δ-1 are possible.

Original languageEnglish
Pages (from-to)295-309
Number of pages15
JournalPlanetary and Space Science
Volume45
Issue number3
DOIs
Publication statusPublished - 01 Jan 1997

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Fingerprint Dive into the research topics of 'The thermal emission of Kuiper Belt objects'. Together they form a unique fingerprint.

Cite this