CBSE Class 9  >  Class 9 Notes  >  Science   >  Unit Test (Solutions): Gravitation

Unit Test (Solutions): Gravitation

Time: 1 hour 
M.M. 30 
Attempt all questions. 
Question numbers 1 to 5 carry 1 mark each. 
Question numbers 6 to 8 carry 2 marks each. 
Question numbers 9 to 11 carry 3 marks each. 
Question numbers 12 & 13 carry 5 marks each.

Q1. What is the force that keeps the moon in its orbit around the Earth? (1 Mark)

Ans: Gravitational force

Q2. Define centripetal force. (1 Mark)

Ans: It is the force that acts towards the center of a circular path and keeps a body moving along that path.

Q3. What is the SI unit of the universal gravitational constant (G)? (1 Mark)

Ans: N m2 kg-2

Q4. What is the acceleration due to gravity on Earth's surface (approximate value)? (1 Mark)

Ans: 9.8 m s-2

Q5. Why do objects float in a liquid? (1 Mark)

Ans: Objects float when their density is less than the liquid's density.

Q6. State the universal law of gravitation. (2 Marks)

Ans: According to the universal law of gravitation, every object in the universe attracts every other object with a force which is directly proportional to the product of their masses and inversely proportional to the square of the distance between them.

Q7. Why does a sheet of paper fall slower than a crumpled ball? (2 Marks)

Ans: The sheet of paper has a larger surface area, so it experiences greater air resistance than the crumpled ball, which falls faster due to lesser air resistance.

Q8. Define thrust and pressure. (2 Marks)

Ans: 

  • Thrust is the force acting normally on a surface.

  • Pressure is the thrust per unit area. Its SI unit is Pascal (Pa).

Q9. Calculate the gravitational force between the Earth and a 1 kg object on its surface. Given: Mass of Earth = 6 × 1024 kg, Radius of Earth = 6.4 × 106 m, G = 6.7 × 10-11 N m2 kg-2.  Explain why this force is significant. (3 Marks)

Ans: Using F = G × (M × m) / d2
F = (6.7 × 10-11 × 6 × 1024 × 1) / (6.4 × 106)2
F = (6.7 × 6 × 1013) / (4.096 × 1013)
F = 40.2 / 4.096 × 100 = 9.81 N
Significance:
This is the gravitational force acting on a 1 kg object on Earth, also called its weight. It causes the object to accelerate downward at 9.8 m/s², which keeps everything grounded on Earth and governs the motion of falling objects.

Q10. Describe Archimedes' principle with an example. (3 Marks)

Ans: Archimedes' principle states that when a body is immersed fully or partially in a fluid, it experiences an upward force (buoyant force) equal to the weight of the fluid displaced by it.
Example: A ship floats in water because the upward buoyant force balances its weight.

Q11. How does the gravitational force between two objects change if:
(i) The mass of one object is doubled?
(ii) the distance between them is halved?
(iii) Both masses are doubled?   (3 Marks)

Ans: (i) The gravitational force doubles.
(ii) The gravitational force becomes four times (since F ∝ 1/d²).
(iii) The gravitational force becomes four times (F ∝ m₁ × m₂).

Q12.  Explain why the weight of an object on the moon is 1/6th its weight on Earth.  (5 Marks)

Ans: 

The weight of an object is the force with which it is attracted towards a celestial body and is given by the formula:
W = m × g,
where m is the mass of the object and g is the acceleration due to gravity.

The mass of the Moon is much smaller (7.36 × 10²² kg) and its radius is also smaller (1.74 × 10⁶ m) compared to the Earth (5.98 × 10²⁴ kg, 6.37 × 10⁶ m).
Using the formula for gravitational acceleration,
g = G × M / R²,
we find that the Moon's gravitational acceleration is approximately 1/6th that of Earth's.

Hence, the weight of an object on the Moon is 1/6th of its weight on Earth, because weight depends on gravitational acceleration.

Q13. A stone is dropped from a 100 m tower, and another is projected upward from the ground at 25 m/s simultaneously. Taking g = 10 m/s2, calculate when and where they meet. (5 Marks)

Ans: Let time of meeting be t seconds.

For stone dropped from the tower:
Initial velocity, u₁ = 0
Distance covered = s₁ = ½ g t² = 5t²

For stone thrown upward:
Initial velocity, u₂ = 25 m/s
Distance covered = s₂ = ut - ½ g t² = 25t - 5t²

Since s₁ + s₂ = 100 (total height of the tower):
5t² + (25t - 5t²) = 100
25t = 100
t = 4 seconds

Now, distance covered by first stone:
s₁ = 5 × (4)² = 80 m from the top
So, height from ground = 100 - 80 = 20 m

Final Answer:
The stones meet after 4 seconds, at a height of 20 metres above the ground.

The document Unit Test (Solutions): Gravitation is a part of the Class 9 Course Science Class 9.
All you need of Class 9 at this link: Class 9

FAQs on Unit Test (Solutions): Gravitation

1. What is the universal law of gravitation?
Ans. The universal law of gravitation, formulated by Sir Isaac Newton, states that every point mass attracts every other point mass in the universe with a force that is directly proportional to the product of their masses and inversely proportional to the square of the distance between their centers. The mathematical expression for this law is F = G(m₁m₂/r²), where F is the gravitational force, G is the gravitational constant, m₁ and m₂ are the masses, and r is the distance between the centers of the two masses.
2. How does gravity affect objects on Earth?
Ans. Gravity is the force that pulls objects toward the center of the Earth. This force gives weight to physical objects and is responsible for holding everything on the ground. For example, when you drop an object, it falls to the ground because of the gravitational force acting on it. The acceleration due to gravity on Earth is approximately 9.81 m/s², which means that the speed of a falling object increases by about 9.81 meters per second every second.
3. What role does gravity play in the solar system?
Ans. Gravity plays a crucial role in the structure and behavior of the solar system. It is the force that keeps planets, moons, and other celestial bodies in orbit around the Sun. The Sun's massive gravitational pull keeps the planets in their elliptical orbits, preventing them from drifting away into space. Additionally, gravity is responsible for the tides on Earth, caused by the gravitational interaction between the Earth and the Moon.
4. What is the significance of the gravitational constant (G)?
Ans. The gravitational constant (G) is a fundamental physical constant used in the calculation of the gravitational force between two masses. Its value is approximately 6.674 × 10⁻¹¹ N(m/kg)². G is significant because it allows scientists to quantify the strength of the gravitational force and is crucial for understanding gravitational interactions in both classical mechanics and modern astrophysics, including the behavior of stars, galaxies, and the universe as a whole.
5. How did historical discoveries about gravity influence modern physics?
Ans. Historical discoveries about gravity, particularly those made by Sir Isaac Newton in the 17th century, laid the foundation for classical mechanics and significantly influenced modern physics. Newton's laws of motion and the universal law of gravitation provided a framework for understanding motion and forces. Later, Albert Einstein's theory of general relativity expanded on these concepts by describing gravity as the curvature of spacetime caused by mass. This shift in understanding has had profound implications for cosmology, astrophysics, and our comprehension of the universe.
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