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Suppose the rocket in the Example was initially on a circular orbit around Earth with a period of 1.6 days. Hint (a) What is its orbital speed (in m/s)? m/s (b) If we want to propel a portion of the rocket to infinity (in the direction tangential to the circular orbit), what's the escape speed from there (in m/s)? m/s

1 Answer

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Answer:

a

The orbital speed is
v= 2.6*10^(3) m/s

b

The escape velocity of the rocket is
v_e= 3.72 *10^3 m/s

Step-by-step explanation:

Generally angular velocity is mathematically represented as


w = (2 \pi)/(T)

Where T is the period which is given as 1.6 days =
1.6 *24 *60*60 = 138240 sec

Substituting the value


w = (2 \pi)/(138240)


= 4.54*10^ {-5} rad /sec

At the point when the rocket is on a circular orbit

The gravitational force = centripetal force and this can be mathematically represented as


(GMm)/(r^2) = mr w^2

Where G is the universal gravitational constant with a value
G = 6.67*10^(-11)

M is the mass of the earth with a constant value of
M = 5.98*10^(24)kg

r is the distance between earth and circular orbit where the rocke is found

Making r the subject


r = \sqrt[3]{(GM)/(w^2) }


= \sqrt[3]{(6.67*10^(-11) * 5.98*10^(24))/((4.45*10^(-5))^2) }


= 5.78 *10^7 m

The orbital speed is represented mathematically as


v=wr

Substituting value


v= (5.78*10^7)(4.54*10^(-5))


v= 2.6*10^(3) m/s

The escape velocity is mathematically represented as


v_e = \sqrt{(2GM)/(r) }

Substituting values


= \sqrt{(2(6.67*10^(-11))(5.98*10^(24)))/(5.78*10^7) }


v_e= 3.72 *10^3 m/s

User Marcel Hansemann
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