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For the following exercises, use Keplers Law, which states that the square of the time, T (measured in Earth years), require
For the following exercises, use Keplers Law, which states that the square of the time, T (measured in Earth years), require
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According to Kepler's Law, the square of the time "T" (measured in Earth years) required for a planet to orbit the sun varies directly with the cube of the mean distance "a" (measure in billions of miles) that the planet is from the sun, i.e.

T? = kg

where "k" is the constant.

a.

Time required by planet Mars to orbit the sun, Tm = 2

Mean distance of planet Mars from the sun, am = 0.142 billion miles.

On substituting the above values in the Kepler's Law equation, we get -

(2)2 = k(0.142)

4= k(0.002863)

= 139713

Therefore, we can write the equation for Kepler's Law as -

T2 = (1397.1)

b.

Mean distance of planet Pluto from the sun, ap = 3.67 billion miles.

Time required by planet Pluto to orbit the sun, Tp = ?

We can use the equation of the Kepler's Law for calculating the time required by planet Pluto to orbit the sun as -

Tº = (1397.1) (3.67)

T2 = (1397.1) (49.430863)

T2 = 69059.8587

::T=V69059.8587

  = 262,792

Thus, the time required by planet Pluto to orbit the sun is 262.792 Earth years.

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