Experimental study of transition of Jupiter and Saturn atmosphere to conducting state

被引:0
作者
Ternovoi, V. Ya. [1 ]
Kvitov, S. V. [1 ]
Nikolaev, A. N. [1 ]
Pyalling, A. A. [1 ]
Filimonov, A. S. [1 ]
Fortov, V. E. [1 ]
机构
[1] Russian Acad Sci, Inst Problems Chem Phys, ESM Dept, Chernogolovka 142432, Moscow Region, Russia
来源
SHOCK COMPRESSION OF CONDENSED MATTER - 2005, PTS 1 AND 2 | 2006年 / 845卷
关键词
Jupiter; Saturn; helium-hydrogen mixture; conductivity;
D O I
暂无
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
The modified equation of state of helium-hydrogen mixtures was used for ID hydrodynamic simulation of performed experiments the multiple shock compression of Jupiter and Saturn model atmospheres. That permitted us to obtain the isentropic compression at third and later steps of compression in pressure region 20-150 GPa. It was shown, that the helium-hydrogen mixtures become conductive due to appearance of hydrogen conductance. The intervals of pressure temperature - density states of these transitions are 30-50 GPa - 4400-5000 K - 0.4-0.5 g/cm(3) for Jupiter and 60-80 GPa - 4600-4800 K - 0.53-0.6 g/cm(3) for Saturn in accordance with our new and previous experiments with pure hydrogen and gas mixtures.
引用
收藏
页码:1492 / 1495
页数:4
相关论文
共 13 条
  • [1] Shock-compression experiments and reflectivity measurements in deuterium up to 3.5 Mbar using the Nova laser
    Collins, GW
    Celliers, PM
    Gold, DM
    Da Silva, LB
    Cauble, R
    [J]. CONTRIBUTIONS TO PLASMA PHYSICS, 1999, 39 (1-2) : 13 - 16
  • [2] Ebeling W., 1991, Thermophysical Properties of Hot Dense Plasmas
  • [3] Pressure-produced ionization of nonideal plasma in a megabar range of dynamic pressures
    Fortov, VE
    Ternovoi, VY
    Zhernokletov, MV
    Mochalov, MA
    Mikhailov, AL
    Filimonov, AS
    Pyalling, AA
    Mintsev, VB
    Gryaznov, VK
    Iosilevskii, IL
    [J]. JOURNAL OF EXPERIMENTAL AND THEORETICAL PHYSICS, 2003, 97 (02) : 259 - 278
  • [4] Models of Jupiter and Saturn after Galileo mission
    Gudkova, TV
    Zharkov, VN
    [J]. PLANETARY AND SPACE SCIENCE, 1999, 47 (10-11) : 1201 - 1210
  • [5] A comparison of the interiors of Jupiter and Saturn
    Guillot, T
    [J]. PLANETARY AND SPACE SCIENCE, 1999, 47 (10-11) : 1183 - 1200
  • [6] Ichimaru S, 1994, STAT PLASMA PHYS
  • [7] Molecular dissociation in hot, dense hydrogen
    Magro, WR
    Ceperley, DM
    Pierleoni, C
    Bernu, B
    [J]. PHYSICAL REVIEW LETTERS, 1996, 76 (08) : 1240 - 1243
  • [8] Metallization of fluid hydrogen at 140 GPa (1.4 Mbar): implications for Jupiter
    Nellis, WJ
    [J]. PLANETARY AND SPACE SCIENCE, 2000, 48 (7-8) : 671 - 677
  • [9] FLUID HYDROGEN AT HIGH-DENSITY - THE PLASMA PHASE-TRANSITION
    SAUMON, D
    CHABRIER, G
    [J]. PHYSICAL REVIEW LETTERS, 1989, 62 (20) : 2397 - 2400
  • [10] AN EQUATION OF STATE FOR LOW-MASS STARS AND GIANT PLANETS
    SAUMON, D
    CHABRIER, G
    VANHORN, HM
    [J]. ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 1995, 99 (02) : 713 - 741