Jupiter planetary tables

After the formation of Jupiter and Saturn, nebula gas dissipated for some reason. Under these conditions, collision velocities reach 10-30 km/s, and catastrophic disruption of planets occurs. All of the processes related to the mechanism of planetary formation introduced above are summarized in Table 9.5. 

Table 1 compares physical parameters of the planetary atmospheres discussed below. We separate these into two groups (1) the terrestrial planets (Venus, Earth, and Mars), and (2) the gas giant planets (Jupiter, Saturn, Uranus, and Neptune). Properties for the terrestrial planets are given at the observed surface conditions. Properties for the gas giant planets, which do not have observable solid surfaces, are given at the 1 bar atmospheric level. 

Table 1 gives the relevant optical properties for each of the three cameras. Camera 1 is difiBraction limited at 1.0 mm and has the same pixel size on the sky as the planetary camera of WFPC. Our definition of diffiaction limited is five pixels between the zeros of the point spread function for the wavelength under consideration. Camera 2 is diffraction limited at 1.75 mm and Camera 3 is a wide field camera with a field of view of 51 arc seconds. The field of view in this camera is slightly larger than the disk of Jupiter. 

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