Chin. Phys. Lett.  2003, Vol. 20 Issue (1): 170-172    DOI:
Original Articles |
Structure of Callisto and Ice Holes on Its Surface
ZHANG Jian-Hui;CHEN Chu-Xin
School of Earth and Space Sciences, University of Science and Technology of China, Hefei 230026
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ZHANG Jian-Hui, CHEN Chu-Xin 2003 Chin. Phys. Lett. 20 170-172
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Abstract The discovery of the induced magnetic field of Callisto that is a satellite of Jupiter has been interpreted as evidence for a subsurface salty liquid-water ocean, so we consider a layered structure of Callisto, i.e., a rock-metal core, an outer layer of ice and a middle layer of ocean. For the rock-metal core we try to indicate how the temperature, pressure and mass density depend on the depth. Due to motion across the magnetic field of Jupiter in a plasma environment, the ice shell of Callisto must be broken down by electric current.
Keywords: 96.30.Kf      96.35.Mz      96.35.Pb     
Published: 01 January 2003
PACS:  96.30.Kf (Jupiter)  
  96.35.Mz  
  96.35.Pb  
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https://cpl.iphy.ac.cn/       OR      https://cpl.iphy.ac.cn/Y2003/V20/I1/0170
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ZHANG Jian-Hui
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