Implications from Galileo observations on the interior structure and chemistry of the Galilean satellites

Icarus

Volumn 157, Issue 1, 2002, Pages 104-119

  Sohl, F ^a   Spohn, T ^a   Breuer, D ^a   Nagel, K ^a  

^a UNIVERSITY OF MÜNSTER   (Germany)

Author keywords

Callisto; Europa; Ganymede; Interiors; Io; Satellites of Jupiter

Indexed keywords

EID: 0036084190     PISSN: 00191035     EISSN: None     Source Type: Journal    
DOI: 10.1006/icar.2002.6828     Document Type: Article

References (46)

1. Galileo gravity results and the internal structure of Io
2. Gravitational constraints on the internal structure of Ganymede
3. Europa’s differentiated internal structure: Inferences from two Galileo encounters
4. Distribution of rock, metals, and ices in Callisto
5. Europa’s differentiated internal structure: Inferences from four Galileo encounters
6. Shape, mean radius, gravity field, and interior structure of Callisto
7. Io’s gravity field and interior structure
8. Phase transitions and convection in icy satellites
9. Density profile of an SNC model martian interior and the moment of inertia factor of Mars
10. 2 at high pressure and high temperature
11. Thermal-orbital histories of visco-elastic models of Io (J1)
12. Thermal equilibrium states of Europa’s ice shell: Implications for interior structure
13. Meteorites and the Early Solar System
14. Induced magnetic fields as evidence for subsurface oceans in Europa and Callisto
15. Discovery of Ganymede’s magnetic field by the Galileo spacecraft
16. Galileo magnetometer measurements: A stronger case for a subsurface ocean at Europa
17. The permanent and inductive magnetic moments of Ganymede
18. Io: Geochemistry of sulfur
19. Upper bound on Io’s heat flow
20. Salts on Europa’s surface detected by Galileo’s near infrared mapping spectrometer
21. High-temperature silicate volcanism on Jupiter’s moon Io
22. Mystery of Callisto: Is it undifferentiated?
23. Ganymede and Callisto
24. A model of the evolution and incomplete differentiation of Callisto
25. Numerical Recipes
26. Rheology of the Earth
27. Tidal heating in an internal ocean model of Europa
28. Fault offsets and lateral crustal movement on Europa: Evidence for a mobile ice shell
29. Thermal histories, compositions and internal structure of the moons of the Solar System
30. The magnetic field and internal structure of Ganymede
31. Tidal dissipation, surface heat flow, and figure of viscoelastic models of Io
32. Computer Solution of Ordinary Differential Equations
33. The Galilean satellites
34. Thermodynamic properties of high pressure ices: Implications for the dynamics and internal structure of large icy satellites
35. Tides of Io
36. Implications from Galileo observations on the interior structure and evolution of the Galilean satellites
37. Oceans in the icy Galilean satellites of Jupiter?
38. The tectonics of icy satellites
39. Applications of thermodynamics to fundamental Earth physics
40. Finite strain theories and comparisons with seismological data
41. Magnetism and thermal evolution of the terrestrial planets
42. Crater relaxation as a probe of Europa’s interior
43. The shape of Io from Galileo limb measurements
44. Io’s heat flow from infrared radiometry: 1983-1993
45. Cooling of the Earth in the Archean: Consequences of pressure-release melting in a hotter mantle
46. Subsurface oceans on Europa and Callisto: Constraints from Galileo magnetometer observations