The role of an internal heat source for the eruptive plumes on Triton

N. S. Duxbury, R. H. Brown

Research output: Contribution to journalArticle

19 Scopus citations

Abstract

For the first time the role of the internal heat source, due to radioactive decay in Triton's core, is investigated with respect to geyser-like plumes. Triton is one of only three known objects in the Solar System (the other two are Earth and the jovian satellite Io) where eruptive activity has been definitely observed. A new mechanism of energy supply to the Tritonian eruptive plumes is proposed. This mechanism is based on heat transport in the solid-nitrogen polar caps due to thermal convection, in addition to conduction. The conductive-convective model shows that a 1 K increase in the N2ice subsurface temperature over the surface value is reached much closer to the surface in the region of an upwelling subsurface plume compared with a pure conductive case. This temperature rise is sufficient to double the nitrogen vapor pressure. Therefore, it is enough to drive the atmospheric plumes to the observed height of ≈8 km, provided 1 K warmer nitrogen ice encounters a vent and hence is exposed to the ≈15-μbar Tritonian atmosphere. Solid-state convection onsets if a nitrogen layer is sufficiently thick and the average solid N2grain size is small enough. Critical values of these parameters are presented for Triton. A possible origin of the subsurface vents on Triton is also suggested.

Original languageEnglish (US)
Pages (from-to)83-93
Number of pages11
JournalIcarus
Volume125
Issue number1
DOIs
StatePublished - Jan 1 1997

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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