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Metallization and electrical conductivity of hydrogen in Jupiter.
Nellis, W J; Weir, S T; Mitchell, A C.
Afiliação
  • Nellis WJ; Lawrence Livermore National Laboratory, University of California, Livermore, CA 94550, USA.
Science ; 273(5277): 936-8, 1996 Aug 16.
Article em En | MEDLINE | ID: mdl-8688072
Electrical conductivities of molecular hydrogen in Jupiter were calculated by scaling electrical conductivities measured at shock pressures in the range of 10 to 180 gigapascals (0.1 to 1.8 megabars) and temperatures to 4000 kelvin, representative of conditions inside Jupiter. Jupiter's magnetic field is caused by convective dynamo motion of electrically conducting fluid hydrogen. The data imply that Jupiter should become metallic at 140 gigapascals in the fluid, and the electrical conductivity in the jovian molecular envelope at pressures up to metallization is about an order of magnitude larger than expected previously. The large magnetic field is produced in the molecular envelope closer to the surface than previously thought.
Assuntos
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Coleções: 01-internacional Base de dados: MEDLINE Assunto principal: Júpiter / Hidrogênio Idioma: En Revista: Science Ano de publicação: 1996 Tipo de documento: Article País de afiliação: Estados Unidos País de publicação: Estados Unidos
Buscar no Google
Coleções: 01-internacional Base de dados: MEDLINE Assunto principal: Júpiter / Hidrogênio Idioma: En Revista: Science Ano de publicação: 1996 Tipo de documento: Article País de afiliação: Estados Unidos País de publicação: Estados Unidos