A planet moves in an elliptical orbit around the sun. The mass of the sun is Ms. The minimum and maximum distances of the planet from the sun are R₁ and R₂, respectively. Part A Using Kepler's 3rd law and Newton's law of universal gravitation, find the period of revolution P of the planet as it moves around the sun. Assume that the mass of the planet is much smaller than the mass of the sun. Use G for the gravitational constant. Express the period in terms of G, Ms, R₁, and R₂. ► View Available Hint(s) P= 15] ΑΣΦ Xb √x vx x x √√₁²(R₁ + R₂)³ 2GM IXXI ? X.10n X Review | Constants

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A planet moves in an elliptical orbit around the sun. The mass
of the sun is M§. The minimum and maximum distances of
the planet from the sun are R₁ and R2, respectively.
Part A
Using Kepler's 3rd law and Newton's law of universal gravitation, find the period of revolution P of the planet as it moves around the sun. Assume
that the mass of the planet is much smaller than the mass of the sun.
Use G for the gravitational constant.
Express the period in terms of G, Ms, R₁, and R₂.
► View Available Hint(s)
P =
IVE ΑΣΦ
xa
Xb
010
√x vx x
л² (R₁ + R₂)³
2GM
S
<४
?
|X| X.10n
X
Review | Constants
=
Transcribed Image Text:A planet moves in an elliptical orbit around the sun. The mass of the sun is M§. The minimum and maximum distances of the planet from the sun are R₁ and R2, respectively. Part A Using Kepler's 3rd law and Newton's law of universal gravitation, find the period of revolution P of the planet as it moves around the sun. Assume that the mass of the planet is much smaller than the mass of the sun. Use G for the gravitational constant. Express the period in terms of G, Ms, R₁, and R₂. ► View Available Hint(s) P = IVE ΑΣΦ xa Xb 010 √x vx x л² (R₁ + R₂)³ 2GM S <४ ? |X| X.10n X Review | Constants =
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