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A saturn year is 29.5 times the earth ye...

A saturn year is 29.5 times the earth year. How far is the saturn from the sun if the earth is `1.5xx10^(8)` away from the sun?

A

`-1.4xx10^(6)km`

B

`1.4xx10^(7)km`

C

`1.4xx10^(8)km`

D

`1.4xx10^(9)km`

Text Solution

AI Generated Solution

The correct Answer is:
To find the distance of Saturn from the Sun given that a Saturn year is 29.5 times an Earth year and the distance of Earth from the Sun is \(1.5 \times 10^8\) km, we can use Kepler's Third Law of planetary motion. ### Step-by-step Solution: 1. **Identify the relationship from Kepler's Third Law**: Kepler's Third Law states that the square of the orbital period (T) of a planet is directly proportional to the cube of the semi-major axis (r) of its orbit. This can be expressed as: \[ \frac{T_{saturn}^2}{T_{earth}^2} = \frac{r_{saturn}^3}{r_{earth}^3} \] 2. **Define the known values**: - Let \(T_{earth} = 1\) year (the period of Earth). - Thus, \(T_{saturn} = 29.5\) years. - The distance of Earth from the Sun, \(r_{earth} = 1.5 \times 10^8\) km. 3. **Substitute the known values into the equation**: \[ \frac{(29.5)^2}{(1)^2} = \frac{r_{saturn}^3}{(1.5 \times 10^8)^3} \] 4. **Calculate \(T_{saturn}^2\)**: \[ T_{saturn}^2 = (29.5)^2 = 870.25 \] 5. **Rearranging the equation**: \[ r_{saturn}^3 = 870.25 \times (1.5 \times 10^8)^3 \] 6. **Calculate \((1.5 \times 10^8)^3\)**: \[ (1.5)^3 = 3.375 \quad \text{and} \quad (10^8)^3 = 10^{24} \] Thus, \[ (1.5 \times 10^8)^3 = 3.375 \times 10^{24} \] 7. **Substituting back into the equation**: \[ r_{saturn}^3 = 870.25 \times 3.375 \times 10^{24} \] 8. **Calculating the product**: \[ r_{saturn}^3 = 2945.57875 \times 10^{24} \] 9. **Taking the cube root to find \(r_{saturn}\)**: \[ r_{saturn} = (2945.57875 \times 10^{24})^{1/3} \] 10. **Calculating the cube root**: - The cube root of \(2945.57875\) is approximately \(14.2\). - Thus, \[ r_{saturn} \approx 14.2 \times 10^{8} \text{ km} = 1.42 \times 10^{9} \text{ km} \] ### Final Answer: The distance of Saturn from the Sun is approximately \(1.42 \times 10^9\) km.

To find the distance of Saturn from the Sun given that a Saturn year is 29.5 times an Earth year and the distance of Earth from the Sun is \(1.5 \times 10^8\) km, we can use Kepler's Third Law of planetary motion. ### Step-by-step Solution: 1. **Identify the relationship from Kepler's Third Law**: Kepler's Third Law states that the square of the orbital period (T) of a planet is directly proportional to the cube of the semi-major axis (r) of its orbit. This can be expressed as: \[ \frac{T_{saturn}^2}{T_{earth}^2} = \frac{r_{saturn}^3}{r_{earth}^3} ...
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A2Z-GRAVITATION-Chapter Test
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  2. A satellite of the earth is revolving in a circular orbit with a unifo...

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  3. The earth E moves in an elliptical orbit with the sun S at one of the ...

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  4. Different points in the earth are at slightly different distance from ...

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  5. A body weighs 700gm wt on the surface of the earth. How much will it w...

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  6. If the mass of a planet is 10% less than that of the earth and the rad...

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  7. Determine the speed with which the earth would have to rotate on its a...

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  8. In order to shift a body of mass m from a circular orbit of radius 3R ...

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  9. A tunnel is dug along a diameter of the earth. Find the force on a par...

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  10. The value of g at a certain height h above the free surface of the ear...

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  11. Suppose that the acceleration of a free fall at the surface of a dista...

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  12. Three uniform spheres each having a mass M and radius a are kept in su...

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  14. A man weighs 80 kg on the surface of earth of radius r. At what height...

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  15. The gravitational potential energy of an isolated system of three part...

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  16. Consider two solid uniform spherical objects of the same density rho. ...

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  17. A body starts from rest from a point distant r(0) from the centre of t...

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  18. If the radius of the earth decreases by 10%, the mass remaining unchan...

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  19. Suppose the gravitational force varies inversely as the nth power of d...

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  20. A satellite of mass m revolves around the earth of radius R at a hight...

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