%0 Journal Article %1 Keszthelyi2004 %A Keszthelyi, L. %A Jaeger, W. L. %A Turtle, E. P. %A Milazzo, M. %A Radebaugh, J. %D 2004 %J Icarus %K ACTIVE DISSIPATION; DISTRIBUTION; GLOBAL HEAT-FLOW; HOT-SPOTS; INTERNAL IO; JUPITERS MAGMA MODELS; MOON SILICATE STRUCTURE; TIDAL VISCOELASTIC VOLCANISM; %N 1 %P 271--286 %T A post-Galileo view of Io's interior %V 169 %X We present a self-consistent model for the interior of Io, taking the recent Galileo data into account. In this model, to has a completely molten core, substantially molten mantle, and a very cold lithosphere. Heat from magmatic activity can mobilize volatile compounds such as SO2 in the lithosphere, and the movement of such cryogenic fluids may be important in the formation of surface features including sapping scarps and paterae. Published by Elsevier Inc.

@article{Keszthelyi2004, abstract = {We present a self-consistent model for the interior of Io, taking the recent Galileo data into account. In this model, to has a completely molten core, substantially molten mantle, and a very cold lithosphere. Heat from magmatic activity can mobilize volatile compounds such as SO2 in the lithosphere, and the movement of such cryogenic fluids may be important in the formation of surface features including sapping scarps and paterae. Published by Elsevier Inc.}, added-at = {2009-11-03T20:21:25.000+0100}, author = {Keszthelyi, L. and Jaeger, W. L. and Turtle, E. P. and Milazzo, M. and Radebaugh, J.}, biburl = {https://www.bibsonomy.org/bibtex/2e27eaad44eef150511403a55848c5a32/svance}, citedreferences = {ANDERSON DL, 1989, THEORY EARTH, P366 ; ANDERSON JD, 2001, J GEOPHYS RES-PLANET, V106, P32963 ; BLANEY DL, 1995, Icarus, V113, P220 ; BRETT R, 1973, GEOCHIM COSMOCHIM AC, V37, P165 ; CARR MH, 1979, Nature, V280, P729 ; CARR MH, 1986, J GEOPHYS RES-SOLID, V91, P3521 ; CARR MH, 1998, Icarus, V135, P146 ; CLOW GD, 1980, Icarus, V44, P729 ; DAVIES AG, 2000, Icarus, V148, P211 ; DAVIES AG, 2001, J GEOPHYS RES-PLANET, V106, P33079 ; FISCHER HJ, 1990, Icarus, V83, P39 ; GALILEI G, 1610, SIDEREUS NUNCIUS ; GEISSLER P, 2004, Icarus, V169, P29 ; GEISSLER PE, 1999, Icarus, V140, P265 ; GEISSLER PE, 2001, J GEOPHYS RES-SPACE, V106, P26137 ; GHIORSO MS, 1995, CONTRIB MINERAL PETR, V119, P197 ; HANEL R, 1979, Science, V204, P972 ; JAEGER WL, 2002, P LUN PLAN SCI C 33 ; JAEGER WL, 2003, J GEOPHYS RES, V108 ; JOHNSON TV, 1979, Nature, V280, P746 ; JOHNSON TV, 1988, Science, V242, P1280 ; KESZTHELYI L, 1997, Icarus, V130, P437 ; KESZTHELYI L, 1999, Icarus, V141, P415 ; KESZTHELYI L, 2001, J GEOPHYS RES-PLANET, V106, P33025 ; KIEFFER SW, 2000, Science, V288, P1204 ; KIVELSON MG, 2002, 83 AGU ; KUSKOV OL, 2001, Icarus, V151, P204 ; LEONE G, 2001, J GEOPHYS RES-PLANET, V106, P32983 ; LOPES RMC, 2004, Icarus, V169, P140 ; LOPESGAUTIER R, 1999, Icarus, V140, P243 ; LOPESGAUTIER R, 2000, Science, V288, P1201 ; MCCAULEY JF, 1979, Nature, V280, P736 ; MCEWEN AS, 1983, Icarus, V55, P191 ; MCEWEN AS, 1985, J GEOPHYS RES, V90, P12345 ; MCEWEN AS, 1997, GEOPHYS RES LETT, V24, P2443 ; MCEWEN AS, 1998, Icarus, V135, P181 ; MCEWEN AS, 1998, Science, V281, P87 ; MCEWEN AS, 2000, Science, V288, P1193 ; MCEWEN AS, 2003, JUPITER PLANET SATEL ; MCKENZIE D, 1985, EARTH PLANET SC LETT, V74, P81 ; MCKINNON WB, 2001, Geology, V29, P103 ; MCKINNON WB, 2003, P LUN PLAN SCI C 34 ; MILAZZO MP, 2001, J GEOPHYS RES-PLANET, V106, P33121 ; MONNEREAU M, 2002, Icarus, V158, P450 ; MOORE JM, 1996, Icarus, V122, P63 ; MOORE JM, 2001, J GEOPHYS RES-PLANET, V106, P33223 ; MOORE WB, 2001, Icarus, V154, P548 ; MORABITO LA, 1979, Science, V204, P972 ; MORRISON D, 1977, PLANETARY SATELLITES, P269 ; NIMMO F, 2002, Geology, V30, P987 ; Ojakangas GW, 1986, Icarus, V66, P341 ; OREILLY TC, 1981, GEOPHYS RES LETT, V8, P313 ; Peale SJ, 1979, Science, V203, P892 ; PHILLIPS CB, 2000, THESIS U ARIZONA TUC ; PHILPOTTS AR, 1998, Nature, V395, P343 ; RADEBAUGH J, 2001, J GEOPHYS RES-PLANET, V106, P33005 ; RATHBUN JA, 2004, Icarus, V169, P127 ; ROSS MN, 1985, Icarus, V64, P391 ; ROSS MN, 1990, Icarus, V85, P309 ; SAGAN C, 1979, Nature, V280, P750 ; SALAMA F, 1990, Icarus, V110, P292 ; SCHABER GG, 1982, SATELLITES JUPITER, P435 ; SCHENK P, 2001, J GEOPHYS RES-PLANET, V106, P33201 ; SCHENK PM, 1998, Science, V279, P1514 ; Schmitt B, 2003, J GEOPHYS RES, V108 ; Schubert G, 1986, SATELLITES, P224 ; SEGATZ M, 1988, Icarus, V75, P187 ; SINTON WM, 1982, Icarus, V51, P563 ; SMITH BA, 1979, Nature, V280, P738 ; SMITH BA, 1979, Science, V204, P951 ; SMYTHE WD, 2000, B AM ASTRON SOC, V32, P1047 ; SPENCER JR, 1996, ANNU REV EARTH PL SC, V24, P125 ; SPENCER JR, 1997, Icarus, V127, P221 ; SPENCER JR, 2000, Science, V288, P1198 ; SPENCER JR, 2000, Science, V288, P1208 ; Stevenson DJ, 1991, ANNU REV FLUID MECH, V23, P305 ; Stevenson DJ, 2002, EUROPA TITAN EOS T ; TACKLEY PJ, 2001, Icarus, V149, P79 ; Turcotte DL, 1982, GEODYNAMICS ; TURTLE EP, 2001, J GEOPHYS RES-PLANET, V106, P33175 ; TURTLE EP, 2004, Icarus, V169, P3 ; VEEDER GJ, 1994, J GEOPHYS RES, V99, P17095 ; WAMSTEKER W, 1974, Icarus, V23, P417 ; WEBB EK, 1987, Icarus, V70, P348 ; WILLIAMS DA, 2000, J GEOPHYS RES-PLANET, V105, P1671 ; WILLIAMS DA, 2002, J GEOPHYS RES, V107 ; WILLIAMS DA, 2004, Icarus, V169, P80}, interhash = {2b69d63cad12ec9b2166178959a3a323}, intrahash = {e27eaad44eef150511403a55848c5a32}, journal = {Icarus}, keywords = {ACTIVE DISSIPATION; DISTRIBUTION; GLOBAL HEAT-FLOW; HOT-SPOTS; INTERNAL IO; JUPITERS MAGMA MODELS; MOON SILICATE STRUCTURE; TIDAL VISCOELASTIC VOLCANISM;}, number = 1, owner = {svance}, pages = {271--286}, timestamp = {2009-11-03T20:21:54.000+0100}, title = {A post-Galileo view of Io's interior}, volume = 169, year = 2004 }