Further investigations of Jupiter models

Icarus

Volumn 25, Issue 4, 1975, Pages 627-634

  Podolak, M ^a   Cameron, A G W ^b  

^a YESHIVA UNIVERSITY   (United States)

^b SMITHSONIAN ASTROPHYSICAL OBSERVATORY   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0013536103     PISSN: 00191035     EISSN: 10902643     Source Type: Journal    
DOI: 10.1016/0019-1035(75)90044-5     Document Type: Article

References (28)

1. Structure of the Jovian envelope from Pioneer 10 gravity data
2. Gravity results from Pioneer 10 doppler data
3. Accumulation processes in the primitive solar nebular
4. Abundances of the elements in the solar system
5. Experimental determination of the compressibility of hydrogen between 0.5 and 3 g/cc. Metalization of hydrogen
6. Thermal models of Jupiter and Saturn
7. Statistical mechanics of light elements at high pressure I Theory and results for metallic hydrogen with simple screening
8. Structure of Jupiter and Saturn
9. On the secular stability of rapidly rotating stars of arbitrary structure
10. Gruneisen constant in the Thomas-Fermi approximation
11. On the formation of Jupiter and Saturn
12. The temperature gradient in the solar nebula
13. Diatomic molecules according to the wave mechanics. II. Vibrational levels
14. The structure and composition of Jupiter and Saturn
15. Hydrodynamic instability of the solar nebula in the presence of a planetary core
16. Models of the giant planets
17. On the densities of methane metallic ammonium water and neon at planetary pressures
18. Models of Uranus and Neptune
19. Equation of state of water to 250 kilobars
20. Theoretical high pressure equations of state including correlation energy
21. Molecular abundance in stellar atmospheres
22. Pressure dissociation and molecular hydrogen
23. The figure of planets with a uniform or two-component density distribution