Q. 34.0( 41 Votes )

# Suppose there existed a planet that went around the sun twice as fast as the earth.

What would be its orbital size as compared to that of the earth?

Answer :

Now planet revolves in orbit around sun due to attractive gravitational force between planet and sun, from Kepler’s third law of planetary motion we know that square of time period one complete rotation of planet T around the sun is proportional to the cube of mean distance (average distance) between the planet and sun R

T^{2}∝ R^{3}

Le the Time taken by the earth for one complete revolution be T_{e}

T_{e} = 1 Year

Let mean distance of the earth from the sun or orbital radius be R_{e}

Since the planet is moving twice as fast as earth the time taken by the planet to complete one complete revolution is half of that taken by earth

Let the Time period of revolution of the planet be T_{p}, then we have

T_{P} = 1/2T_{e} = 1/2 year

Let, the orbital radius of this planet be R_{P}

Now, according to the Kepler’s third law of planetary motion, we have

And

Using both equations we get the relation

Or we can say

Simplifying we get the relation for the orbital radius of the planet as

Since planet took half as much time as earth so we have

T_{p}/T_{e} = 1/2

i.e. the radius of the planet is

Therefore, the radius of the orbit of this planet is 0.63 times the radius of the orbit of the Earth.

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A Saturn year is 29.5 times the earth year. How far is the Saturn from the sun if the earth is 1.50 × 10^{8} km away from the sun?

(a) Find the radius of the circular orbit of a satellite moving with an angular speed equal to the angular speed of earth’s rotation.

(b) If the satellite is directly above the North Pole at some instant, find the time it takes to come over the equatorial plane.

Mass of the earth = 6 × 10^{24} Kg.

HC Verma - Concepts of Physics Part 1

A Mars satellite moving in an orbit of radius 9.4 × 10^{3} Km takes 27540 s to complete one revolution. Calculate the mass of Mars.

The moon takes about 27.3 days to revolve round the earth in a nearly circular orbit of radius 3.84 × 10^{5} Km. Calculate the mass of the earth from these data.