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Kepler constants provide information about the dynamics of orbiting satellites on the parent planet, including the satellite orbit system on Jupiter's planet. Kepler's constant can be calculated from the ratio between the square of the satellite revolution time and the power of three of satellite distances to the parent planet. The time data of revolution and distance with digital images of satellites and their parent planet using robotic telescope and CCD. Robotic telescopes can be directed by the program. Data within the estimated time range includes satellites at the furthest point from Jupiter. Digital image data is processed with image processing software. Macros Excel is used to calculate Kepler constants from digital image data enclosures. Kepler's constants on the Io and Jupiter satellite systems are 920.8 tahun² / SA³.