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33. A spherical particle of density p= 5.00- cm? and 2.00 mm radius is located at the same distance from the Sun as the Earth, RSE =1.5 x 1011 m. Nm? G= 6.67 x 10-11 S= 1 365 kg on the particle by the Sun is · Mg = 1.99 x 10" kg. If the particle absorbs 100 percent of the sunlight reaching it, the ratio of the force exerted by the solar radiation to the force of gravity exerted m2 a. 5.8 x 105. b. 0.58. c. 1.0. d. 1.7. e. 1.7 x 104|

33. A spherical particle of density p= 5.00- cm? and 2.00 mm radius is located at the same distance from the Sun as the Earth, RSE =1.5 x 1011 m. Nm? G= 6.67 x 10-11 S= 1 365 kg on the particle by the Sun is · Mg = 1.99 x 10" kg. If the particle absorbs 100 percent of the sunlight reaching it, the ratio of the force exerted by the solar radiation to the force of gravity exerted m2 a. 5.8 x 105. b. 0.58. c. 1.0. d. 1.7. e. 1.7 x 104|

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33. A spherical particle of density p= 5.00- cm? and 2.00 mm radius is located at the same distance from the Sun as the Earth, RSE =1.5 x 1011 m. Nm? G= 6.67 x 10-11 S= 1 365 kg on the particle by the Sun is · Mg = 1.99 x 10" kg. If the particle absorbs 100 percent of the sunlight reaching it, the ratio of the force exerted by the solar radiation to the force of gravity exerted m2 a. 5.8 x 105. b. 0.58. c. 1.0. d. 1.7. e. 1.7 x 104|
Transcribed Image Text:33. A spherical particle of density p= 5.00- cm? and 2.00 mm radius is located at the same distance from the Sun as the Earth, RSE =1.5 x 1011 m. Nm? G= 6.67 x 10-11 S= 1 365 kg on the particle by the Sun is · Mg = 1.99 x 10" kg. If the particle absorbs 100 percent of the sunlight reaching it, the ratio of the force exerted by the solar radiation to the force of gravity exerted m2 a. 5.8 x 105. b. 0.58. c. 1.0. d. 1.7. e. 1.7 x 104|
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