Thermal state and complex geology of a heterogeneous salty crust of Jupiter's satellite, Europa
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[1] Jeffrey S. Kargel,et al. Europa's Crust and Ocean: Origin, Composition, and the Prospects for Life , 2000 .
[2] S. Ishihara,et al. Standard Reference Materials: Enthalpy and heat capacity standard reference material , 1977 .
[3] Tilman Spohn,et al. Oceans in the icy Galilean satellites of Jupiter , 2002 .
[4] C. T. Russell,et al. Induced magnetic fields as evidence for subsurface oceans in Europa and Callisto , 1998, Nature.
[5] Stephen H. Kirby,et al. The strength and rheology of methane clathrate hydrate , 2003 .
[6] D. Stevenson,et al. Volcanism and igneous processes in small icy satellites , 1982, Nature.
[7] Clark R. Chapman,et al. Does Europa have a subsurface ocean? Evaluation of the geological evidence , 1999 .
[8] F. Fanale,et al. An experimental estimate of Europa's “ocean” composition independent of Galileo orbital remote sensing , 2001 .
[9] James Charles Granahan,et al. Non‐water‐ice constituents in the surface material of the icy Galilean satellites from the Galileo near‐infrared mapping spectrometer investigation , 1998 .
[10] J. Ruiz,et al. Heat flow, lenticulae spacing, and possibility of convection in the ice shell of europa , 2003 .
[11] R. E. Johnson,et al. Sulfuric acid on Europa and the radiolytic sulfur cycle. , 1999, Science.
[12] M. White,et al. Origin of glassy crystalline behavior in the thermal properties of clathrate hydrates: a thermal conductivity study of tetrahydrofuran hydrate , 1988 .
[13] James Charles Granahan,et al. Hydrated salt minerals on Europa's surface from the Galileo near‐infrared mapping spectrometer (NIMS) investigation , 1999 .
[14] S. D. Kadel,et al. Chaos on Europa , 1999 .
[15] Doris Breuer,et al. Implications from Galileo Observations on the Interior Structure and Chemistry of the Galilean Satellites , 2002 .
[16] B. C. Edwards,et al. Radar Detectability of a Subsurface Ocean on Europa , 1998 .
[17] C. Russell,et al. Galileo magnetometer measurements: a stronger case for a subsurface ocean at Europa. , 2000, Science.
[18] D. Stevenson,et al. Thermal state of an ice shell on Europa , 1989 .
[19] Hitoshi,et al. Geochemical Aspects of the McMurdo Saline Lakes with Special Emphasis on the Distribution of Nutrient Matters , 1975 .
[20] C. de Bergh,et al. Solar system ices , 1998 .
[21] W. Durham. RHEOLOGICAL PROPERTIES OF WATER ICE—APPLICATIONS TO SATELLITES OF THE OUTER PLANETS 1 , 2001 .
[22] J. Kirschvink,et al. Life in Ice-Covered Oceans , 1999, Science.
[23] S. M. Marcus,et al. Thermal conductivity of polymers, glasses and ceramics by modulated DSC , 1994 .
[24] J. K. Crowley,et al. Salts on Europa's surface detected by Galileo's near infrared mapping spectrometer. The NIMS Team. , 1998, Science.
[25] R. Greeley,et al. Geological evidence for solid-state convection in Europa's ice shell , 1998, Nature.
[26] W. Durham,et al. Rheology of planetary ices , 1998 .
[27] Christopher T. Russell,et al. Europa and Callisto: Induced or intrinsic fields in a periodically varying plasma environment , 1999 .
[28] Hauke Hussmann,et al. Thermal Equilibrium States of Europa's Ice Shell: Implications for Internal Ocean Thickness and Surface Heat Flow , 2002 .
[29] R. C. Weast. CRC Handbook of Chemistry and Physics , 1973 .
[30] Michael J. S. Belton,et al. Galileo's Multiinstrument Spectral View of Europa's Surface Composition , 1999 .
[31] R. G. Ross,et al. Thermal Conductivity of Solar System Ices, with Special Reference to Martian Polar Caps , 1998 .
[32] G. Marion. A molal-based model for strong acid chemistry at low temperatures (<200 to 298 K) , 2002 .
[33] Stephen H. Kirby,et al. Peculiarities of Methane Clathrate Hydrate Formation and Solid-State Deformation, Including Possible Superheating of Water Ice , 1996, Science.
[34] J. Kargel,et al. Evaluation of the Possible Presence of CO2-Clathrates in Europa's Icy Shell or Seafloor , 2004 .
[35] W. McKinnon,et al. Convective instability in Europa's floating ice shell , 1997 .
[36] Stefan M. Sarge,et al. Temperature, heat and heat flow rate calibration of scanning calorimeters in the cooling mode , 2000 .
[37] G. Schubert,et al. Europa's differentiated internal structure: inferences from two Galileo encounters. , 1997, Science.
[38] Jeffrey S. Kargel,et al. Brine volcanism and the interior structures of asteroids and icy satellites , 1991 .
[39] M. Zolensky,et al. Sulfate content of Europa's ocean and shell: evolutionary considerations and some geological and astrobiological implications. , 2003, Astrobiology.
[40] E. D. West,et al. Enthalpy and Heat-Capacity Standard Reference Material: Synthetic Sapphire (α-Al2O3) from 10 to 2250 K. , 1982, Journal of research of the National Bureau of Standards.
[41] T. McCord,et al. Thermal and radiation stability of the hydrated salt minerals epsomite, mirabilite, and natron under Europa environmental conditions , 2001 .
[42] David P. O'Brien,et al. A melt-through model for chaos formation on Europa , 2002 .
[43] J. Delaney,et al. Evidence for a weakly stratified Europan ocean sustained by seafloor heat flux , 2001 .
[44] R. Carlson,et al. Sulfuric Acid Production on Europa: The Radiolysis of Sulfur in Water Ice , 2002 .
[45] E. Hanitzsch. Modification of the conventional measuring method to determine the specific heat capacity using a Perkin-Elmer DSC 2 , 1991 .
[46] E. Gaidos,et al. Strike‐slip motion and double ridge formation on Europa , 2002 .
[47] J. Kargel,et al. Magnesium Sulfate-Water to 400 MPa Using a Novel Piezometer: Densities, Phase Equilibria, and Planetological Implications , 1995 .
[48] Everett L. Shock,et al. Energy for biologic sulfate reduction in a hydrothermally formed ocean on Europa , 2003 .
[49] A model of Europa's crustal structure: Recent Galileo results and implications for an ocean , 2001 .
[50] B. R. Tufts,et al. Evidence for a subsurface ocean on Europa , 1998, Nature.
[51] M. N. Poglazova,et al. Microflora in the basal strata at Antarctic ice core above the Vostok lake. , 2001, Advances in space research : the official journal of the Committee on Space Research.