Large‐scale topography of Io: Implications for internal structure and heat transfer

Geophysical Research Letters

Volumn 15, Issue 6, 1988, Pages 581-584

  Gaskell, Robert W ^a   Synnott, Stephen P ^a   McEwen, Alfred S ^b   Schaber, Gerald G ^b  

^a CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^b U S GEOLOGICAL SURVEY   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0023724766     PISSN: 00948276     EISSN: 19448007     Source Type: Journal    
DOI: 10.1029/GL015i006p00581     Document Type: Article

References (21)

1. Numerical and approximate solutions for lithospheric thickening and thinning
2. Coordinates of features on the Galilean satellites
3. Shapes and gravitational moments of satellites and asteroids
4. Shape and topography of Io
5. Digital identification of cartographic control points
6. How fast do Galilean satellites spin?
7. Heat flow from Io (Jl)
8. Hot‐spot tectonics on Io, In Conf. on Heat and Detachment in Crustal Extension on Continents and Planets
9. Volcanic hot spots on Io: Correlation with lowalbedo calderas
10. Constraints on rift thermal processes from heat flow and uplift
11. Hot spot heat transfer: Its application to Venus and implications to Venus and Earth
12. Magma transport of heat on Io: A mechanism allowing a thick lithosphere
13. Melting of Io by tidal dissipation
14. Io: Shield volcanism, tidally forced viscous heating, and the shift of active volcanism from the sub‐Jupiter and anti‐Jupiter points
15. Tidal dissipation, surface heat flow, and figure of viscoelastic models of Io
16. Shape of Io
17. Thermal origin of the Hawaiian swell: Heat flow evidence and thermal models