The orbit of Earth around the Sun is almost circular: The closest and farthest distances are 1.47 x 108 km and 1.52 x 108 km respectively. Determine the corresponding variations in (a) total energy, (b) gravitational potential energy, (c) kinetic energy, and (d) orbital speed. (a) Number 8.9e+31 Units (b) Number 1.8e+32 Units (c) Number i 8.9e+31 Units (d) Number i 5.0e+2 Units km/s

College Physics
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Author:Raymond A. Serway, Chris Vuille
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Chapter1: Units, Trigonometry. And Vectors
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I’m still stuck with part A can you please explain it clear for me ? I need to understand this problem thank you.
The orbit of Earth around the Sun is almost circular: The closest and farthest distances are 1.47 x 108 km and 1.52 × 10® km
respectively. Determine the corresponding variations in (a) total energy, (b) gravitational potential energy, (c) kinetic energy, and (d)
orbital speed.
(a) Number
8.9e+31
Units
(b) Number
1.8e+32
Units
J
(c) Number
i
8.9e+31
Units
(d) Number
i
5.0e+2
Units
km/s
Transcribed Image Text:The orbit of Earth around the Sun is almost circular: The closest and farthest distances are 1.47 x 108 km and 1.52 × 10® km respectively. Determine the corresponding variations in (a) total energy, (b) gravitational potential energy, (c) kinetic energy, and (d) orbital speed. (a) Number 8.9e+31 Units (b) Number 1.8e+32 Units J (c) Number i 8.9e+31 Units (d) Number i 5.0e+2 Units km/s
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