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Gravitational – 2

Welcome to your Gravitational - 2

1. 
Kepler’s first law states that planets move in

2. 
Two planets revolve around Sun in circular orbits of radii r and 4r. Ratio of angular speeds is

3. 
If semi-major axis of planet A is 4 times that of planet B, ratio of their periods is

4. 
A planet moves slowest when it is

5. 
For planets revolving around Sun, central force is

6. 
Law of areas implies

7. 
The farthest point of planet from Sun is

8. 
Newton used Kepler’s laws to establish

9. 
In an elliptical orbit, sum of distances from foci is

10. 
A planet farther from Sun has

11. 
A satellite moving under gravity sweeps equal areas in equal times about

12. 
Areal velocity of planet in elliptical orbit is

13. 
If gravitational force suddenly disappears, planet will move in

14. 
Circular orbit is a special case of

15. 
Kepler’s third law is valid for

16. 
Kepler’s third law states that T² is proportional to

17. 
Dimensions of gravitational constant G are

18. 
Which of the following is NOT explained by Kepler’s laws?

19. 
According to Kepler’s second law, area swept in equal time intervals is

20. 
Which scientist explained Kepler’s laws theoretically?

21. 
If radius of circular orbit of a planet is doubled, its time period becomes

22. 
Which quantity remains constant for a planet in circular orbit?

23. 
Which law explains variation of speed of planet?

24. 
The closest point of planet from Sun is called

25. 
For a planet in elliptical orbit, maximum speed occurs at

26. 
The direction of velocity at any point of orbit is along

27. 
Gravitational force between two masses varies inversely as

28. 
For elliptical orbit, total energy of planet is

29. 
Kepler’s second law is a consequence of conservation of

30. 
Kepler’s laws are valid for

31. 
Kepler’s second law is equivalent to conservation of

32. 
A planet moves fastest when it is

33. 
SI unit of gravitational constant G is

34. 
Kepler’s laws were derived from

35. 
Gravitational force between two bodies is always

36. 
A comet moving in highly elliptical orbit has very high speed at

37. 
Elliptical orbit becomes circular when

38. 
Kepler’s third law relates

39. 
Who provided data for Kepler’s laws?

40. 
In an elliptical orbit, the Sun is located at

41. 
Semi-major axis of ellipse is

42. 
Newton’s law of gravitation states that force between two masses is proportional to

43. 
If mass of Sun increases, time period of Earth will

44. 
If a planet suddenly stops obeying Kepler’s second law, which quantity is not conserved?

45. 
Kepler’s second law is also known as

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