Hydrologic modelling with variable fluid properties : a liquid sulfur aquifer beneath the surface of Io
The return of the first Voyager images of Io in 1979 provoked a controversy over the importance of sulfur versus silicate volcanism in resurfacing the satellite. The debate involves both the strength of crustal material as well as the mode of mass and heat transport to the surface of Io. The dyna...
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ndltd-UBC-oai-circle.library.ubc.ca-2429-42242018-01-05T17:31:51Z Hydrologic modelling with variable fluid properties : a liquid sulfur aquifer beneath the surface of Io Wijns, Christopher P. The return of the first Voyager images of Io in 1979 provoked a controversy over the importance of sulfur versus silicate volcanism in resurfacing the satellite. The debate involves both the strength of crustal material as well as the mode of mass and heat transport to the surface of Io. The dynamics of sulfur magma transport will depend upon the properties of liquid sulfur. Unlike the Newtonian behaviour of silicate magmas, molten sulfur has anomalies in the heat capacity (a A-like transistion at 432 K) and in the viscosity (a maximum at 460 K) due to a polymerization reaction. Numerical modelling of a pure liquid sulfur supply region at depth in a porous crust shows that the fluid supply rate from such a magma reservoir is about seven orders of magnitude less than the observed mass and heat fluxes at the surface of Io. This requires accumulation of magma in a reservoir prior to eruption at the surface, but the accumulation time on the order of tens of thousands of years is much longer than would be consistent with the level of volcanic activity observed on Io. Low sulfur magma supply rates suggest that sulfur is not the dominant resurfacing material for the satellite. This is consistent with calculations performed for the viscous relaxation of topography on Io. Surface features of a largely sulfur crust would disappear within months because of material weakness. Significant topographic highs and steep slopes on Io provide evidence for a crust with stronger mechanical properties. Sulfur convection in the crust can still provide a large fraction of the global heat flow, within certain conditions on the permeability. Previous estimates of resurfacing rates have equated the cooling of erupted material to the entire global energy budget. Significant convective transfer of heat by liquid sulfur may call for a downward revision of resurfacing rates. Science, Faculty of Earth, Ocean and Atmospheric Sciences, Department of Graduate 2009-02-06T21:27:20Z 2009-02-06T21:27:20Z 1995 1996-05 Text Thesis/Dissertation http://hdl.handle.net/2429/4224 eng For non-commercial purposes only, such as research, private study and education. Additional conditions apply, see Terms of Use https://open.library.ubc.ca/terms_of_use. 3606266 bytes application/pdf |
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The return of the first Voyager images of Io in 1979 provoked a controversy over the
importance of sulfur versus silicate volcanism in resurfacing the satellite. The debate
involves both the strength of crustal material as well as the mode of mass and heat
transport to the surface of Io. The dynamics of sulfur magma transport will depend
upon the properties of liquid sulfur. Unlike the Newtonian behaviour of silicate magmas,
molten sulfur has anomalies in the heat capacity (a A-like transistion at 432 K) and in the
viscosity (a maximum at 460 K) due to a polymerization reaction. Numerical modelling
of a pure liquid sulfur supply region at depth in a porous crust shows that the fluid
supply rate from such a magma reservoir is about seven orders of magnitude less than
the observed mass and heat fluxes at the surface of Io. This requires accumulation of
magma in a reservoir prior to eruption at the surface, but the accumulation time on the
order of tens of thousands of years is much longer than would be consistent with the
level of volcanic activity observed on Io. Low sulfur magma supply rates suggest that
sulfur is not the dominant resurfacing material for the satellite. This is consistent with
calculations performed for the viscous relaxation of topography on Io. Surface features
of a largely sulfur crust would disappear within months because of material weakness.
Significant topographic highs and steep slopes on Io provide evidence for a crust with
stronger mechanical properties. Sulfur convection in the crust can still provide a large
fraction of the global heat flow, within certain conditions on the permeability. Previous
estimates of resurfacing rates have equated the cooling of erupted material to the entire
global energy budget. Significant convective transfer of heat by liquid sulfur may call for
a downward revision of resurfacing rates. === Science, Faculty of === Earth, Ocean and Atmospheric Sciences, Department of === Graduate |
author |
Wijns, Christopher P. |
spellingShingle |
Wijns, Christopher P. Hydrologic modelling with variable fluid properties : a liquid sulfur aquifer beneath the surface of Io |
author_facet |
Wijns, Christopher P. |
author_sort |
Wijns, Christopher P. |
title |
Hydrologic modelling with variable fluid properties : a liquid sulfur aquifer beneath the surface of Io |
title_short |
Hydrologic modelling with variable fluid properties : a liquid sulfur aquifer beneath the surface of Io |
title_full |
Hydrologic modelling with variable fluid properties : a liquid sulfur aquifer beneath the surface of Io |
title_fullStr |
Hydrologic modelling with variable fluid properties : a liquid sulfur aquifer beneath the surface of Io |
title_full_unstemmed |
Hydrologic modelling with variable fluid properties : a liquid sulfur aquifer beneath the surface of Io |
title_sort |
hydrologic modelling with variable fluid properties : a liquid sulfur aquifer beneath the surface of io |
publishDate |
2009 |
url |
http://hdl.handle.net/2429/4224 |
work_keys_str_mv |
AT wijnschristopherp hydrologicmodellingwithvariablefluidpropertiesaliquidsulfuraquiferbeneaththesurfaceofio |
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1718586719984418816 |