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If the distance between the sun and the ...

If the distance between the sun and the earth is increased by three times, then attraction between two will

A

remains constant

B

decrease by 63 %

C

increase by 63 %

D

decrease by 89 %

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To solve the problem, we will use Newton's law of universal gravitation, which states that the gravitational force \( F \) between two masses \( M_1 \) and \( M_2 \) separated by a distance \( R \) is given by the formula: \[ F = \frac{G M_1 M_2}{R^2} \] Where \( G \) is the gravitational constant. ### Step-by-Step Solution: 1. **Identify Initial Conditions**: - Let the initial distance between the Sun and the Earth be \( R \). - The initial gravitational force \( F \) can be expressed as: \[ F = \frac{G M_1 M_2}{R^2} \] 2. **Change in Distance**: - According to the problem, the distance is increased by three times. Therefore, the new distance \( R' \) is: \[ R' = 3R \] 3. **Calculate New Gravitational Force**: - The new gravitational force \( F' \) when the distance is increased to \( 3R \) is: \[ F' = \frac{G M_1 M_2}{(3R)^2} \] - Simplifying this gives: \[ F' = \frac{G M_1 M_2}{9R^2} = \frac{F}{9} \] 4. **Determine the Change in Force**: - The attraction between the two bodies has decreased from \( F \) to \( F' \). The change in force can be calculated as: \[ \text{Change in Force} = F - F' = F - \frac{F}{9} = \frac{8F}{9} \] 5. **Calculate Percentage Decrease**: - The percentage decrease in the gravitational force is given by: \[ \text{Percentage Decrease} = \left(\frac{\text{Change in Force}}{F}\right) \times 100 = \left(\frac{\frac{8F}{9}}{F}\right) \times 100 \] - This simplifies to: \[ \text{Percentage Decrease} = \frac{8}{9} \times 100 \approx 88.89\% \] ### Conclusion: The attraction between the Sun and the Earth will decrease by approximately 89%.

To solve the problem, we will use Newton's law of universal gravitation, which states that the gravitational force \( F \) between two masses \( M_1 \) and \( M_2 \) separated by a distance \( R \) is given by the formula: \[ F = \frac{G M_1 M_2}{R^2} \] Where \( G \) is the gravitational constant. ...
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DC PANDEY ENGLISH-GRAVITATION-Check Point 10.1
  1. Kepler's second law is based on

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  2. When a planet moves around the sun

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  3. A planet moves around the sun. It is closest to sun to sun at a distan...

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  4. For a satellite in elliptical orbit which of the following quantities ...

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  5. The motion of planets in the solar system in an example of conservatio...

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  6. Kepler's law starts that square of the time period of any planet movin...

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  7. The ratio of mean distances of three planets from the sun are 0.5 : 1:...

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  8. The time of revolution of planet A round the sun is 8 times that of an...

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  9. The distance of the two planets from the Sun are 10^(13)m and 10^(12) ...

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  10. A satellite having time period same as that of the earth's rotation ab...

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  11. A body is orbiting around earth at a mean radius which is two times a...

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  12. Two point masses each equal to 1 kg attract one another with a force o...

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  13. Gravitational force between a point mass m and M separated by a distan...

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  14. Three equal masses of 2kg each are placed at the vertices of an equila...

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  15. The force of gravitation is

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  16. Which of the following statements about the gravitational constant is ...

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  17. The distance of the centres of moon the earth is D. The mass of earth ...

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  18. Two identical spheres of radius R made of the same material are kept a...

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  19. If the distance between the sun and the earth is increased by three ti...

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  20. A spherical planet far out in space has mass 2M and radius a. A partic...

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