A komatiite analog to potential ultramafic materials on Io

David Williams, Allan H. Wilson, Ronald Greeley

Research output: Contribution to journalArticle

33 Citations (Scopus)

Abstract

Ultramafic volcanism is one model which fits currently available data for some eruptions on Jupiter's moon, Io. Assuming that such activity does occur, it is possible to apply komatiitic analogs and terrestrial ultramafic flow models to Io. We have used such analogs and models along with Galileo data to investigate the nature of ultramafic materials that are assumed to occur at high-temperature hotspots on Io. The unusual komatiites of the Commondale greenstone belt, South Africa, are consistent with available Galileo data on the temperatures and composition of potential Ionian ultramafic materials. These komatiites had high SiO 2 (∼50 wt %) and MgO (∼31 wt %) contents, which are inferred to result in high liquidus temperatures (∼1610°C), low dynamic viscosities (∼0.2 Pa s), and low densities (∼2680 kg/m 3) and in the crystallization of orthopyroxene phenocrysts (not found in other komatiites). We used the Commondale composition and the model of Williams et al. [1998] to investigate potential ultramafic flow behavior on Io. Compared to their terrestrial counterparts, Ionian ultramafic lava flows would have less potential for turbulent flow, lower maximum emplacement distances, and lower thermal erosion rates because of the lower Ionian gravity and their more silicic composition. Shallow (<10 m deep) thermal erosion channels are predicted to occur more proximally to the lava source than on Earth. Deep (>10 m) thermal erosion channels seem less likely on Io, unless (1) lavas are superheated, (2) lavas are more ultramafic (>31% MgO), (3) eruption rates, eruption durations, or flow volumes are high, or (4) substrates are unconsolidated, partly consolidated, or volatile-rich and thus more erodable. If volatiles are present in the lava as vesicles, then increasing lava vesicularity results in decreasing maximum emplacement distances, decreasing thermal erosion rates, and decreasing erosion channel depths for given eruption durations.

Original languageEnglish (US)
Article number1999JE001157
Pages (from-to)1671-1684
Number of pages14
JournalJournal of Geophysical Research E: Planets
Volume105
Issue numberE1
StatePublished - 2000

Fingerprint

komatiite
Io
volcanic eruptions
erosion
Erosion
lava
volcanic eruption
analogs
erosion rate
emplacement
Chemical analysis
potential flow
Republic of South Africa
Potential flow
liquidus
Moon
natural satellites
greenstone belt
Crystallization
vesicle

ASJC Scopus subject areas

  • Oceanography
  • Astronomy and Astrophysics
  • Atmospheric Science
  • Space and Planetary Science
  • Earth and Planetary Sciences (miscellaneous)
  • Geophysics
  • Geochemistry and Petrology

Cite this

Williams, D., Wilson, A. H., & Greeley, R. (2000). A komatiite analog to potential ultramafic materials on Io. Journal of Geophysical Research E: Planets, 105(E1), 1671-1684. [1999JE001157].

A komatiite analog to potential ultramafic materials on Io. / Williams, David; Wilson, Allan H.; Greeley, Ronald.

In: Journal of Geophysical Research E: Planets, Vol. 105, No. E1, 1999JE001157, 2000, p. 1671-1684.

Research output: Contribution to journalArticle

Williams, D, Wilson, AH & Greeley, R 2000, 'A komatiite analog to potential ultramafic materials on Io', Journal of Geophysical Research E: Planets, vol. 105, no. E1, 1999JE001157, pp. 1671-1684.
Williams, David ; Wilson, Allan H. ; Greeley, Ronald. / A komatiite analog to potential ultramafic materials on Io. In: Journal of Geophysical Research E: Planets. 2000 ; Vol. 105, No. E1. pp. 1671-1684.
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