Gm,m2 F, 2GM 2nr GM r2 , dc = V 3= T R2 , Vesc = R Gm,m2 Gm,m2 КЕ — E = KE +U, , Ecircular G = 6.674 x 10¬11 N· m²/kg? 2r Problem 1: Let's assume the Earth and Jupiter orbit the Sun in circular orbits. The distance between the Earth and the Sun is rE = 1.5 x 1011 m and the orbital period of the Earth around the Sun is TE = 1 year. The distance between Jupiter and the Sun is rj = 7.8 x 1011 m. Calculate TJ, the orbital period of Jupiter around the Sun, in years. 1 year = 3.154 × 107 sec.

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Chapter1: Units, Trigonometry. And Vectors
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2GM
Gmim2
F, =
GM
2nr
V =
9 =
T
, Vesc =
R2
ac =
r2
R
Gm¡m2
Gm¡m2
KE = ;mv² , U,
E = KE+U, , Ecircular
G = 6.674 x 10-11 N· m²/kg?
2r
Problem 1: Let's assume the Earth and Jupiter orbit the Sun in circular orbits. The distance between the
Earth and the Sun is rE = 1.5 x 1011 m and the orbital period of the Earth around the Sun is TE = 1 year.
The distance between Jupiter and the Sun is rj = 7.8 x 1011 m. Calculate TJ, the orbital period of Jupiter
around the Sun, in years. 1 year = 3.154 x 107 sec.
Transcribed Image Text:2GM Gmim2 F, = GM 2nr V = 9 = T , Vesc = R2 ac = r2 R Gm¡m2 Gm¡m2 KE = ;mv² , U, E = KE+U, , Ecircular G = 6.674 x 10-11 N· m²/kg? 2r Problem 1: Let's assume the Earth and Jupiter orbit the Sun in circular orbits. The distance between the Earth and the Sun is rE = 1.5 x 1011 m and the orbital period of the Earth around the Sun is TE = 1 year. The distance between Jupiter and the Sun is rj = 7.8 x 1011 m. Calculate TJ, the orbital period of Jupiter around the Sun, in years. 1 year = 3.154 x 107 sec.
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