A body weighs \(72~\text{N}\) on the surface of the earth. What is the gravitational force on it at a height equal to half the radius of the earth?
1. | \(32~\text{N}\) | 2. | \(30~\text{N}\) |
3. | \(24~\text{N}\) | 4. | \(48~\text{N}\) |
What is the depth at which the value of acceleration due to gravity becomes 1/n times the value of that at the surface of the earth? (radius of earth = R)
(1) R/
(2) R(n – 1)/n
(3) Rn/(n – 1)
(4) R/n
Choose the correct alternative.
1. | Acceleration due to gravity increases with increasing altitude. |
2. | Acceleration due to gravity remains unchanged with increasing altitude. |
3. | Acceleration due to gravity increases with increasing depth (assume the earth to be a sphere of uniform density). |
4. | Acceleration due to gravity decreases with increasing depth (assume the earth to be a sphere of uniform density). |
Acceleration due to gravity is:
1. | independent of the mass of the earth. |
2. | independent of the mass of the body. |
3. | independent of both the mass of the earth and the body. |
4. | dependent on both the mass of the earth and the body. |
Suppose there existed a planet that went around the sun twice as fast as the Earth. Then its orbital size as compared to that of the Earth would be:
1. | \(0.63\) times greater than that of Earth. |
2. | \(0.73\) times smaller than that of Earth. |
3. | \(0.63\) times smaller than that of Earth. |
4. | \(0.73\) times greater than that of Earth. |
One of the satellites of Jupiter has an orbital period of \(1.769\) days and the radius of the orbit is \(4.22 \times 10^{8}\) m. The ratio of the mass of Jupiter and the mass of the sun nearly is: (Mass of the sun \(\approx 2\times 10^{30}~\text{kg}\))
1. \(1000:1\)
2. \(1:1000\)
3. \(1:1\)
4. \(2000:3\)
Choose the correct alternative.
1. | If the zero of potential energy is at infinity, the total energy of an orbiting satellite is negative of its kinetic energy. |
2. | If the zero of potential energy is at infinity, the total energy of an orbiting satellite is negative of its potential energy. |
3. | The energy required to launch an orbiting satellite out of earth’s gravitational influence is more than the energy required to project a stationary object at the same height (as the satellite) out of earth’s influence. |
4. | Both (1) and (3) are correct. |
Let us assume that our galaxy consists of 2.5 × stars each of one solar mass. How long will a star at a distance of 50,000 ly from the galactic centre take to complete one revolution? (The diameter of the milky way is ly.)
1. 3.55 × 108 years
2. 4.55 × 108 years
3. 3.55 × 107 years
4. 4.55 × 107 years
The escape speed of a body from the Earth depends on:
1. | the mass of the body. |
2. | the location from where it is projected. |
3. | the direction of projection. |
4. | the height of the location from where the body is launched. |
A comet orbits the sun in a highly elliptical orbit. The comet has a constant:
1. linear speed
2. angular speed
3. angular momentum
4. kinetic energy