TABLE 7.3Useful Planetary DataBodyMercuryVenusEarthMarsJupiterSaturnUranusNeptunePlutoaMoonSunMass (kg)3.18 x 10234.88 X 10245.98 X 10246.42 x 10231.90 X 10275.68 X 10268.68 × 10251.03 × 10261.27 x 10237.36 ×10221.991 × 1030MeanRadius (m)2.43 X 1066.06 X 1066.38 X 1063.37 X 1066.99 X 1075.85 X 1072.33 X 1072.21 × 1071.14 X 1061.74 X 1066.96 X 108Period (s)7.60 X 1061.94 X 1073.156 X1075.94 X 1073.74 X 1089.35 × 1082.64 × 10⁹5.22 × 10⁹7.82 X 10⁹MeanDistancefrom Sun (m)5.79 x 10101.08 × 10¹11.496 × 10¹12.28 × 10¹17.78 x 10¹11.43 × 10¹22.87 X 10¹24.50 × 10¹25.91 X 10¹2T²7-3 10-192.972.992.972.982.972.992.952.992.968²Sm"In August 2006, the International Astronomical Union adopted a definition of a planet that separates Pluto fromthe other eight planets. Pluto is now defined as a "dwarf planet" like the asteroid Ceres. 38. Use the data of Table 7.3 to find the point between Earthand the Sun at which an object can be placed so that thenet gravitational force exerted by Earth and the Sun onthat object is zero.

The mass of the sun The mass of the earth The mass of the object = m kgThe distance from the sun to…

Answered: 38. Use the data of Table 7.3 to find…

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38. Use the data of Table 7.3 to find the point between Earth and the Sun at which an object can be placed so that the net gravitational force exerted by Earth and the Sun on that object is zero.