Abstract
High pressures and temperatures in the deep interiors of the giant planets are accessed in the laboratory by shock compression of liquid specimens using a two-stage light-gas gun. Measurements of properties of dense fluids comprising these planets are described and discussed.
Access this chapter
Tax calculation will be finalised at checkout
Purchases are for personal use only
Preview
Unable to display preview. Download preview PDF.
Similar content being viewed by others
References
Chacham H, Louie SG (1991) Metallization of solid hydrogen at megabar pressures: a first-principles quasiparticle study. Phys Rev Lett 66:64–67
Garcia AT, Barbee TW, Cohen ML, Silvera IF (1990) Band gap closure and metallization of molecular solid hydrogen. Europhys Lett 13:355–360
Gudkova TV, Zharkov VN, Leontev VV (1988) Models of Uranus and Neptune with partially mixed envelopes, Astron Vestn (in Russian) 22:23–40
Hamilton DC, Nellis WJ, Mitchell AC, Ree FH, van Thiel M (1988) Electrical conductivity and equation of state of shock-compressed liquid oxygen. J Chem Phys 88:5042–5050
Hubbard WB, Marley MS (1989) Optimized Jupiter, Saturn, and Uranus interior models. Icarus 78:102–118
Hubbard WB, Nellis WJ, Mithell AC, Holmes NC, Limaye SS, McCandless PC (1991) Interior structure of Neptune: comparison with Uranus. Science 253:648–651 Kirk RL
Stevenson DJ (1987) Hydromagnetic constraints on deep zonal flow in the giant planets. Astrophys J 316:836–846
Mitchell AC, Nellis WJ (1981) Diagnostic system of the Lawrence Livermore National Laboratory two-stage light-gas gun. Rev Sci Instrum 52:347–359
Nellis WJ, Mitchell AC (1980) Shock compression of liquid argon, nitrogen, and oxygen. J Chem Phys 73:6137–6145
Nellis WJ, Mitchell AC, van Thiel M, Devine GJ, Trainor RJ, Brown N (1983) Equation-of-state data for molecular hydrogen and deuterium at shock pressures in the range 2–76 GPa (20–760 kbar). J Chem Phys 79:1480–1486
Nellis WJ, Holmes NC, Mitchell AC, Radousky HB, Hamilton D (1986) Condensed matter at high shock pressures. In: Bershader D, Hanson R (eds) Shock Waves and Shock Tubes, Proc 15th Intl Symp on Shock Waves and Shock Tubes, Berkeley, Stanford Univ Press, pp 15–26
Nellis WJ, Hamilton DC, Holmes NC, Radousky HB, Ree FH, Mitchell AC, Nicol M (1988) The nature of the interior of Uranus based on studies of planetary ices at high dynamic pressures. Science 240:779–781
Nellis WJ, Mitchell AC, McCandless PC, Erskine DJ (1991) submitted to Phys Rev Lett Podolak M, Reynolds RT (1987) The rotation rate of Uranus, its internal structure, and the process of planetary accretion. Icarus 70:31–36
Radousky HB, Mitchell AC, Nellis WJ (1990) Shock temperature measurements of planetary ices: NH3, CH4, and “synthetic Uranus”. J Chem Phys 93:8235–8239
Ross M (1982) Shock-wave studies: modeling the giant planets. In: Backman C-M, Johannisson T, Tegner L (eds) High pressure in research and industry, Arkitektkopia, Uppsala, pp 721–727
Stevenson DJ (1987) Uranus, Bull Amer Astron Soc 19:851
Author information
Authors and Affiliations
Editor information
Editors and Affiliations
Rights and permissions
Copyright information
© 1992 Springer-Verlag Berlin Heidelberg
About this paper
Cite this paper
Nellis, W.J., Mitchell, A.C., Holmes, N.C., McCandless, P.C. (1992). Planetary fluids at high shock pressures and temperatures. In: Takayama, K. (eds) Shock Waves. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-77648-9_61
Download citation
DOI: https://doi.org/10.1007/978-3-642-77648-9_61
Publisher Name: Springer, Berlin, Heidelberg
Print ISBN: 978-3-642-77650-2
Online ISBN: 978-3-642-77648-9
eBook Packages: Springer Book Archive