The mean diameters of X and Y, two planets in the same solar system, are 6.4 ✕ 103 km and 2.0 ✕ 104 km, respectively. The mass of X is 0.17 times the mass of Y. The value of g on Y is 9.0 m/s2.
(a) What is the ratio of the mean density of X to that of Y?
ρX |
ρY |
=
(b) What is the value of g on X?
m/s2
(c) The mass of Y is 1.349 ✕
1025 kg. What is the escape speed on X?
m/s
(a)
Radius of planet x,
Rx = 6.4*10^6 m / 2 = 3.2*10^6 m
Radius of planet y,
Ry = 2*10^7 m / 2 = 1*10^7 m
Volume of x / Volume of y = (4/3)*pi*(3.2*10^6 )^3 / (4/3)*pi*(1*10^7)^3
Vx / Vy = 0.0327
ratio of the mean density of X to that of Y,
x / y = (Mx / My) / (Vx / Vy)
x / y = (0.17) / (0.0327)
x / y = 5.18
(b)
Gravitational acceleration is given by,
g = GM / r^2
value of g on X = g on y * [(Mx / My) / (Rx / Ry)^2]
value of g on X = 9 * (0.0327) / (0.32)^2
value of g on X = 2.88 m/s^2
(c)
Escape speed is given by,
ve = sqrt (2GM / r)
escape speed on y = sqrt [(2*6.67*10^(-11)*1.349*10^25) / (1*10^7)]
escape speed on y = 13412.68 m/s
escape speed on X = escape speed on y * sqrt [(Mx / My) / (Rx / Ry)]
escape speed on X = 13412.68 * sqrt [0.17 / 0.32]
escape speed on X = 9776.08 m/s
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