What is Gravitation ? āĻŽāĻšāĻžāĻ•ā§°ā§āώāĻŖ āĻ•āĻŋ ?


What is Gravitation ? | āĻŽāĻšāĻžāĻ•ā§°ā§āώāĻŖ āĻ•āĻŋ?


Definition: Gravitation : Gravitation (or Gravity) is a fundamental natural force by which all objects having mass attract each other.
It is the force responsible for pulling objects together and for maintaining the structure of the universe.


Key Points



  • Gravitation is a universal force because every object in the universe attracts every other object.

  • The gravitational force increases with increase in mass and decreases with increase in distance.

  • Gravitation is responsible for many natural phenomena such as objects falling towards the Earth, tides in the oceans, and planets revolving around the Sun.

  • According to Isaac Newton, the gravitational force between two objects is directly proportional to the product of their masses and inversely proportional to the square of the distance between them.


āĻŽāĻšāĻžāĻ•ā§°ā§āώāĻŖ (Gravitation) :āϏāĻ‚āĻœā§āĻžāĻž : āĻŽāĻšāĻžāĻ•ā§°ā§āώāĻŖ (Gravitation) āĻšā§ˆāϛ⧇ āĻāϟāĻž āĻŽā§ŒāϞāĻŋāĻ• āĻĒā§ā§°āĻžāĻ•ā§ƒāϤāĻŋāĻ• āĻŦāϞ, āϝāĻžā§° āĻĻā§āĻŦāĻžā§°āĻž āĻ­ā§° āĻĨāĻ•āĻž āϏāĻ•āϞ⧋ āĻŦāĻ¸ā§āĻ¤ā§ā§ąā§‡ āχāĻŸā§‹ā§ąā§‡ āϏāĻŋāĻŸā§‹āĻ• āύāĻŋāϜ⧰ āĻĢāĻžāϞ⧇ āφāĻ•ā§°ā§āώāĻŖ āϕ⧰⧇āĨ¤ āĻāχ āĻŦāϞ⧇āχ āĻŦāĻ¸ā§āϤ⧁āϏāĻŽā§‚āĻšāĻ• āĻāϕ⧇āϞāϗ⧇ āϧ⧰āĻŋ ā§°āĻžāϖ⧇ āφ⧰⧁ āĻŦāĻŋāĻļā§āĻŦāĻŦā§ā§°āĻšā§āĻŽāĻžāĻŖā§āĻĄ āĻ¸ā§āĻĨāĻŋā§° āϕ⧰āĻŋ ā§°āĻžāϖ⧇āĨ¤


āĻŽā§āĻ–ā§āϝ āĻĻāĻŋāĻļāϏāĻŽā§‚āĻš



  • āĻŽāĻšāĻžāĻ•ā§°ā§āώāĻŖ āĻšā§ˆāϛ⧇ āĻāϟāĻž āϏāĻžā§°ā§āĻŦāϜāύ⧀āύ āĻŦāϞ, āĻ•āĻŋāϝāĻŧāύ⧋ āĻŦāĻŋāĻļā§āĻŦāĻŦā§ā§°āĻšā§āĻŽāĻžāĻŖā§āĻĄā§° āĻĒā§ā§°āϤāĻŋāĻŸā§‹ āĻŦāĻ¸ā§āĻ¤ā§ā§ąā§‡ āφāύ āĻĒā§ā§°āϤāĻŋāĻŸā§‹ āĻŦāĻ¸ā§āϤ⧁āĻ• āφāĻ•ā§°ā§āώāĻŖ āϕ⧰⧇āĨ¤

  • āĻŦāĻ¸ā§āϤ⧁⧰ āĻ­ā§° āϝāĻŋāĻŽāĻžāύ⧇āχ āĻŦ⧇āĻ›āĻŋ, āĻŽāĻšāĻžāĻ•ā§°ā§āώāĻŖ āĻŦāϞ āϏāĻŋāĻŽāĻžāύ⧇āχ āĻŦ⧇āĻ›āĻŋ āĻšāϝāĻŧ āφ⧰⧁ āĻŦāĻ¸ā§āϤ⧁⧰ āĻŽāĻžāϜ⧰ āĻĻā§‚ā§°āĻ¤ā§āĻŦ āĻŦāĻžāĻĸāĻŧāĻŋāϞ⧇ āĻŽāĻšāĻžāĻ•ā§°ā§āώāĻŖ āĻŦāϞ āĻ•āĻŽāĻŋ āϝāĻžāϝāĻŧāĨ¤

  • āĻŽāĻšāĻžāĻ•ā§°ā§āώāĻŖ āĻŦāϞ⧰ āĻĢāϞāϤ⧇āχ āĻŦāĻ¸ā§āϤ⧁ āĻŽāĻžāϟāĻŋā§° āĻĢāĻžāϞ⧇ āĻĒ⧰⧇, āϏāĻžāĻ—ā§°āϤ āĻœā§‹ā§ąāĻžā§°-āĻ­āĻžāϟāĻž āĻšāϝāĻŧ āφ⧰⧁ āĻ—ā§ā§°āĻšāϏāĻŽā§‚āĻš āĻ¸ā§‚ā§°ā§āϝ⧰ āϚāĻžā§°āĻŋāĻ“āĻĢāĻžāϞ⧇ āĻ˜ā§‚ā§°āĻŋ āĻĨāĻžāϕ⧇āĨ¤

  • Isaac Newton ā§° āĻŽāϤ⧇, āĻĻ⧁āϟāĻž āĻŦāĻ¸ā§āϤ⧁⧰ āĻŽāĻžāϜ⧰ āĻŽāĻšāĻžāĻ•ā§°ā§āώāĻŖ āĻŦāϞ āĻŦāĻ¸ā§āϤ⧁ āĻĻ⧁āϟāĻžā§° āĻ­ā§°ā§° āϗ⧁āĻŖāĻĢāϞ⧰ āϏāĻŽāĻžāύ⧁āĻĒāĻžāϤāĻŋāĻ• āφ⧰⧁ āϏāĻŋāĻšāρāϤ⧰ āĻŽāĻžāϜ⧰ āĻĻā§‚ā§°āĻ¤ā§āĻŦā§° āĻŦā§°ā§āĻ—ā§° āĻŦā§āϝāĻ¸ā§āϤāĻžāύ⧁āĻĒāĻžāϤāĻŋāĻ•āĨ¤


Exam Writing Tip



  • Definition āϞāĻŋāĻ–āĻžā§° āĻĒāĻŋāĻ›āϤ 3–4 points āϞāĻŋāĻ–āĻŋāĻŦ

  • Newton’s law āωāĻ˛ā§āϞ⧇āĻ– āϕ⧰āĻŋāϞ⧇ āĻĒā§‚ā§°ā§āĻŖ āύāĻŽā§āĻŦā§° āĻĒā§‹ā§ąāĻž āϝāĻžāϝāĻŧ


Uses of Gravitation : Importance of Gravitation


Uses : āĻŦā§āĻ¯ā§ąāĻšāĻžā§°



  1. Gravitation keeps us and all objects on the Earth. āϗ⧁⧰⧁āĻ¤ā§āĻŦāĻžāĻ•āĻ°ā§āώāϪ⧇ āφāĻŽāĻžāĻ• āĻĒ⧃āĻĨāĻŋā§ąā§€āϤ āĻ¸ā§āĻĨāĻŋā§° āϕ⧰āĻŋ ā§°āĻžāϖ⧇āĨ¤

  2. It helps planets revolve around the Sun. āĻ—ā§ā§°āĻšāĻŦā§‹ā§° āĻ¸ā§‚ā§°ā§āϝ⧰ āϚāĻžā§°āĻŋāĻ“āĻĢāĻžāϞ⧇ āĻ˜ā§‚ā§°āĻŋāĻŦāϞ⧈ āϏāĻšāĻžāϝāĻŧ āϕ⧰⧇āĨ¤

  3. It causes objects to fall towards the ground. āĻŦāĻ¸ā§āϤ⧁āĻŦā§‹ā§° āĻŽāĻžāϟāĻŋāϞ⧈ āĻĒā§°āĻŋāĻŦāϞ⧈ āϏāĻšāĻžāϝāĻŧ āϕ⧰⧇āĨ¤

  4. It helps in the formation of tides in oceans. āϏāĻžāĻ—ā§°āϤ āĻœā§‹ā§ąāĻžā§°-āĻ­āĻžāϟāĻž āϏ⧃āĻˇā§āϟāĻŋ āϕ⧰⧇āĨ¤

  5. It is responsible for the motion of satellites. āωāĻĒāĻ—ā§ā§°āĻšāĻŦā§‹ā§°āĻ• āĻ•āĻ•ā§āώāĻĒāĻĨāϤ ā§°āĻžāϖ⧇āĨ¤

  6. It gives weight to objects. āĻŦāĻ¸ā§āϤ⧁⧰ āĻ­āĻžā§° āύāĻŋā§°ā§āϧāĻžā§°āĻŖ āϕ⧰⧇āĨ¤


Effects of Gravitation (Effects / Consequences of Gravitation) : āĻŽāĻšāĻžāĻ•ā§°ā§āώāĻŖ āĻ•āĻŋ?


Effects : āĻĒā§ā§°āĻ­āĻžā§ą :



  1. Falling of objects towards Earth. āĻŦāĻ¸ā§āϤ⧁āĻŦā§‹ā§° āĻĒ⧃āĻĨāĻŋā§ąā§€ā§° āĻĢāĻžāϞ⧇ āĻĒ⧰⧇āĨ¤

  2. Weight of objects exists due to gravitation. āĻŦāĻ¸ā§āϤ⧁⧰ āĻ­āĻžā§° āĻĨāĻžāϕ⧇ āϗ⧁⧰⧁āĻ¤ā§āĻŦāĻžāĻ•āĻ°ā§āώāĻŖā§° āĻŦāĻžāĻŦ⧇āĨ¤

  3. Tides are formed in seas and oceans. āϏāĻžāĻ—ā§°āϤ āĻœā§‹ā§ąāĻžā§°-āĻ­āĻžāϟāĻž āϏ⧃āĻˇā§āϟāĻŋ āĻšāϝāĻŧāĨ¤

  4. Planets and satellites move in fixed orbits. āĻ—ā§ā§°āĻš āφ⧰⧁ āωāĻĒāĻ—ā§ā§°āĻšāĻŦā§‹ā§° āύāĻŋā§°ā§āĻĻāĻŋāĻˇā§āϟ āĻ•āĻ•ā§āώāĻĒāĻĨāϤ āĻ˜ā§‚ā§°ā§‡āĨ¤

  5. Atmosphere remains bound to the Earth. āĻŦāĻžāϝāĻŧ⧁āĻŽāĻŖā§āĻĄāϞ āĻĒ⧃āĻĨāĻŋā§ąā§€ā§° āϏ⧈āϤ⧇ āϏāĻ‚āϝ⧁āĻ•ā§āϤ āĻšā§ˆ āĻĨāĻžāϕ⧇āĨ¤

  6. Free fall and weightlessness occur due to gravity. āĻŽā§āĻ•ā§āϤ āĻĒāϤāύ āφ⧰⧁ āĻ­āĻžā§°āĻļā§‚āĻ¨ā§āϝāϤāĻž āϘāĻŸā§‡āĨ¤


Note (Exam Friendly)



  • Gravitation = Universal Attractive Force (āϗ⧁⧰⧁āĻ¤ā§āĻŦāĻžāĻ•āĻ°ā§āώāĻŖ = āϏāĻžā§°ā§āĻŦāϜāύ⧀āύ āφāĻ•ā§°ā§āώāĻŖ āĻŦāϞ)

  • Acts between all masses

  • Important for life and motion in the universe


1. Who discovered gravitation ? āĻĒā§ā§°āĻļā§āύ: āϗ⧁⧰⧁āĻ¤ā§āĻŦāĻžāĻ•āĻ°ā§āώāĻŖ āϕ⧋āύ⧇ āφāĻŦāĻŋāĻˇā§āĻ•āĻžā§° āϕ⧰āĻŋāĻ›āĻŋāϞ ?
Ans: Isaac Newton
Exp: Newton discovered gravitation after observing a falling apple.
āĻŦā§āϝāĻžāĻ–ā§āϝāĻž: āφāĻĒ⧇āϞ āϤāϞāϞ⧈ āĻĒā§°āĻžā§° āϘāϟāύāĻžā§° āĻĒā§°āĻž āύāĻŋāωāϟāύ⧇ āϗ⧁⧰⧁āĻ¤ā§āĻŦāĻžāĻ•āĻ°ā§āώāĻŖ āĻ†ā§ąāĻŋāĻˇā§āĻ•āĻžā§° āϕ⧰āĻŋāĻ›āĻŋāϞāĨ¤


2. What is the formula of gravitational force ? āĻĒā§ā§°āĻļā§āύ: āϗ⧁⧰⧁āĻ¤ā§āĻŦāĻžāĻ•āĻ°ā§āώāĻŖ āĻŦāϞ⧰ āϏ⧂āĻ¤ā§ā§° āĻ•āĻŋ ?
Ans: F = G m₁m₂ / r²
Exp: It shows force depends on masses and distance.
āĻŦā§āϝāĻžāĻ–ā§āϝāĻž: āĻŦāϞ āĻ­ā§° āφ⧰⧁ āĻĻā§‚ā§°āĻ¤ā§āĻŦā§° āĻ“āĻĒā§°āϤ āύāĻŋā§°ā§āĻ­ā§° āϕ⧰⧇āĨ¤


3. What is the value of gravitational constant (G) ? āĻĒā§ā§°āĻļā§āύ: āϗ⧁⧰⧁āĻ¤ā§āĻŦāĻžāĻ•āĻ°ā§āώāĻŖ āĻ§ā§ā§°ā§ā§ąāĻ• G-ā§° āĻŽāĻžāύ āĻ•āĻŋāĻŽāĻžāύ ?
Ans: 6.67 × 10âģ¹¹ Nm²/kg²
Exp: G is a universal constant. āĻŦā§āϝāĻžāĻ–ā§āϝāĻž: G āĻāϟāĻž āϏāĻžā§°ā§āĻŦāϜāύ⧀āύ āĻ§ā§ā§°ā§ā§ąāĻ•āĨ¤


4. Is the value of G same everywhere ? āĻĒā§ā§°āĻļā§āύ: G-ā§° āĻŽāĻžāύ āϏāĻ•āϞ⧋ āĻ āĻžāχāϤ⧇ āĻāϕ⧇ āύ⧇ ? 
Ans: Yes
Exp: G does not change with place. āĻŦā§āϝāĻžāĻ–ā§āϝāĻž: G āĻ āĻžāχ āĻ…āύ⧁āϏ⧰āĻŋ āϏāϞāύāĻŋ āύāĻšāϝāĻŧāĨ¤


5. What is the average value of g on Earth ? āĻĒā§ā§°āĻļā§āύ: āĻĒ⧃āĻĨāĻŋā§ąā§€āϤ g-ā§° āĻ—āĻĄāĻŧ āĻŽāĻžāύ āĻ•āĻŋāĻŽāĻžāύ ?
Ans: 9.8 m/s²
Exp: It represents acceleration due to gravity. āĻŦā§āϝāĻžāĻ–ā§āϝāĻž: āĻāχāĻŸā§‹ āϗ⧁⧰⧁āĻ¤ā§āĻŦāϜāύāĻŋāϤ āĻ¤ā§āĻŦā§°āĻŖ āĻŦ⧁āϜāĻžāϝāĻŧāĨ¤


6. Where is g maximum on Earth ? āĻĒā§ā§°āĻļā§āύ: āĻĒ⧃āĻĨāĻŋā§ąā§€āϤ āĻ•’āϤ g āĻ¸ā§°ā§āĻŦāĻžāϧāĻŋāĻ• ?
Ans: At the poles
Exp: Radius is smaller at poles. āĻŦā§āϝāĻžāĻ–ā§āϝāĻž: āĻ§ā§ā§°ā§ā§ąāϤ āĻĒ⧃āĻĨāĻŋā§ąā§€ā§° āĻŦā§āϝāĻžāϏāĻžā§°ā§āϧ āĻ•āĻŽāĨ¤


7. What happens to g with increase in height ? āĻĒā§ā§°āĻļā§āύ: āωāĻšā§āϚāϤāĻž āĻŦāĻžāĻĸāĻŧāĻŋāϞ⧇ g-ā§° āĻŽāĻžāύ āĻ•āĻŋ āĻšāϝāĻŧ ?
Ans: Decreases
Exp: Distance from Earth’s center increases. āĻŦā§āϝāĻžāĻ–ā§āϝāĻž: āĻĒ⧃āĻĨāĻŋā§ąā§€ā§° āϕ⧇āĻ¨ā§āĻĻā§ā§°ā§° āĻĒā§°āĻž āĻĻā§‚ā§°āĻ¤ā§āĻŦ āĻŦāĻžāĻĸāĻŧ⧇āĨ¤


8. What is the value of g at Earth’s center ? āĻĒā§ā§°āĻļā§āύ: āĻĒ⧃āĻĨāĻŋā§ąā§€ā§° āϕ⧇āĻ¨ā§āĻĻā§ā§°āϤ g-ā§° āĻŽāĻžāύ āĻ•āĻŋāĻŽāĻžāύ ?
Ans: 0
Exp: Gravitational forces cancel each other. āĻŦā§āϝāĻžāĻ–ā§āϝāĻž: āϏāĻ•āϞ⧋ āĻĻāĻŋāĻļā§° āĻŦāϞ āĻāϕ⧇ āĻšā§ˆ āĻŦāĻžāϤāĻŋāϞ āĻšāϝāĻŧāĨ¤


9. What is the value of g on the Moon ? āĻĒā§ā§°āĻļā§āύ: āϚāĻ¨ā§āĻĻā§ā§°āϤ g-ā§° āĻŽāĻžāύ āĻ•āĻŋāĻŽāĻžāύ ?
Ans: 1/6 of Earth
Exp: Moon has less mass. āĻŦā§āϝāĻžāĻ–ā§āϝāĻž: āϚāĻ¨ā§āĻĻā§ā§°ā§° āĻ­ā§° āĻ•āĻŽāĨ¤


10. What is the formula of weight ? āĻĒā§ā§°āĻļā§āύ: āĻ­āĻžā§°ā§° āϏ⧂āĻ¤ā§ā§° āĻ•āĻŋ ?
Ans: W = mg
Exp: Weight depends on gravity. āĻŦā§āϝāĻžāĻ–ā§āϝāĻž: āĻ­āĻžā§° g-ā§° āĻ“āĻĒā§°āϤ āύāĻŋā§°ā§āĻ­ā§°āĻļā§€āϞāĨ¤


11. Is gravitational force attractive or repulsive ? āĻĒā§ā§°āĻļā§āύ: āϗ⧁⧰⧁āĻ¤ā§āĻŦāĻžāĻ•āĻ°ā§āώāĻŖ āĻŦāϞ āφāĻ•ā§°ā§āώāĻŖā§€āϝāĻŧ āύ⧇ āĻŦāĻŋāĻ•āĻ°ā§āώāĻŖā§€āϝāĻŧ ?
Ans: Attractive
Exp: It pulls objects towards each other. āĻŦā§āϝāĻžāĻ–ā§āϝāĻž: āĻŦāĻ¸ā§āϤ⧁āĻŦā§‹ā§° āĻāϕ⧇ āφāύāϞ⧈ āϟāĻžāύ⧇āĨ¤


12. What is the SI unit of g ? āĻĒā§ā§°āĻļā§āύ: g-ā§° SI āĻāĻ•āĻ• āĻ•āĻŋ ?
Ans: m/s²
Exp: It is an acceleration. āĻŦā§āϝāĻžāĻ–ā§āϝāĻž: g āĻāϟāĻž āĻ¤ā§āĻŦā§°āĻŖāĨ¤


13. What is the SI unit of G ? āĻĒā§ā§°āĻļā§āύ: G-ā§° SI āĻāĻ•āĻ• āĻ•āĻŋ ?  
Ans: Nm²/kg²
Exp: Derived from gravitational formula. āĻŦā§āϝāĻžāĻ–ā§āϝāĻž: āϗ⧁⧰⧁āĻ¤ā§āĻŦāĻžāĻ•āĻ°ā§āώāĻŖ āϏ⧂āĻ¤ā§ā§°ā§° āĻĒā§°āĻž āĻĒā§‹ā§ąāĻžāĨ¤


14. What is the mass of the Earth ? āĻĒā§ā§°āĻļā§āύ: āĻĒ⧃āĻĨāĻŋā§ąā§€ā§° āĻ­ā§° āĻ•āĻŋāĻŽāĻžāύ ?
Ans: 5.97 × 10²â´ kg
Exp: Large mass causes strong gravity. āĻŦā§āϝāĻžāĻ–ā§āϝāĻž: āĻĄāĻžāϙ⧰ āϭ⧰⧇ āĻļāĻ•ā§āϤāĻŋāĻļāĻžāϞ⧀ āϗ⧁⧰⧁āĻ¤ā§āĻŦ āϏ⧃āĻˇā§āϟāĻŋ āϕ⧰⧇āĨ¤


15. What is the average radius of the Earth ? āĻĒā§ā§°āĻļā§āύ: āĻĒ⧃āĻĨāĻŋā§ąā§€ā§° āĻ—āĻĄāĻŧ āĻŦā§āϝāĻžāϏāĻžā§°ā§āϧ āĻ•āĻŋāĻŽāĻžāύ ?
Ans: 6371 km
Exp: Used in gravity calculations. āĻŦā§āϝāĻžāĻ–ā§āϝāĻž: āϗ⧁⧰⧁āĻ¤ā§āĻŦ āĻ—āĻŖāύāĻžāϤ āĻŦā§āĻ¯ā§ąāĻšāĻžā§° āĻšāϝāĻŧāĨ¤


16. Does weight change with place ? āĻĒā§ā§°āĻļā§āύ: āĻ­āĻžā§° āĻ āĻžāχ āĻ…āύ⧁āϏ⧰āĻŋ āϏāϞāύāĻŋ āĻšāϝāĻŧ āύ⧇ ?
Ans: Yes
Exp: Because g changes. āĻŦā§āϝāĻžāĻ–ā§āϝāĻž: āĻ•āĻžā§°āĻŖ g āϏāϞāύāĻŋ āĻšāϝāĻŧāĨ¤


17. Does mass change with place ? āĻĒā§ā§°āĻļā§āύ: āĻ­ā§° āĻ āĻžāχ āĻ…āύ⧁āϏ⧰āĻŋ āϏāϞāύāĻŋ āĻšāϝāĻŧ āύ⧇ ?
Ans: No
Exp: Mass is constant. āĻŦā§āϝāĻžāĻ–ā§āϝāĻž: āĻ­ā§° āĻ¸ā§°ā§āĻŦāĻĻāĻž āĻāϕ⧇ āĻĨāĻžāϕ⧇āĨ¤


18. What happens to g below the Earth’s surface ? āĻĒā§ā§°āĻļā§āύ: āĻĒ⧃āĻĨāĻŋā§ąā§€ā§° āĻ­āĻŋāϤ⧰āϞ⧈ āĻ—’āϞ⧇ g-ā§° āĻŽāĻžāύ āĻ•āĻŋ āĻšāϝāĻŧ ?
Ans: Decreases
Exp: Effective mass decreases. āĻŦā§āϝāĻžāĻ–ā§āϝāĻž: āĻ•āĻžā§°ā§āϝāϕ⧰ āĻ­ā§° āĻ•āĻŽā§‡āĨ¤


19. Which force acts during free fall ? āĻĒā§ā§°āĻļā§āύ: āĻŽā§āĻ•ā§āϤ āĻĒāϤāύāϤ āϕ⧋āύāĻŸā§‹ āĻŦāϞ āĻ•āĻžā§°ā§āϝ āϕ⧰⧇ ?
Ans: Only gravitational force
Exp: No other force acts. āĻŦā§āϝāĻžāĻ–ā§āϝāĻž: āĻ…āĻ¨ā§āϝ āϕ⧋āύ⧋ āĻŦāϞ āύāĻžāĻĨāĻžāϕ⧇āĨ¤


20. What is weightlessness ? āĻĒā§ā§°āĻļā§āύ: āĻ­āĻžā§°āĻļā§‚āĻ¨ā§āϝāϤāĻž āĻ•āĻŋ ?
Ans: Condition of free fall
Exp: Apparent weight becomes zero. āĻŦā§āϝāĻžāĻ–ā§āϝāĻž: āĻ…āύ⧁āĻ­ā§‚āϤ āĻ­āĻžā§° āĻļā§‚āĻ¨ā§āϝ āĻšāϝāĻŧāĨ¤


21. Who proved all bodies fall with same g ? āĻĒā§ā§°āĻļā§āύ: āϏāĻ•āϞ⧋ āĻŦāĻ¸ā§āϤ⧁ āĻāϕ⧇ g-⧰⧇ āĻĒ⧰⧇ āĻŦ⧁āϞāĻŋ āϕ⧋āύ⧇ āĻĒā§ā§°āĻŽāĻžāĻŖ āϕ⧰āĻŋāĻ›āĻŋāϞ ?
Ans: Galileo Galilei
Exp: He dropped objects from height. āĻŦā§āϝāĻžāĻ–ā§āϝāĻž: āϤ⧇āĻ“āρ āωāĻšā§āϚāϤāĻžā§° āĻĒā§°āĻž āĻŦāĻ¸ā§āϤ⧁ āĻĒ⧇āϞāĻžāχ āĻĒā§°ā§€āĻ•ā§āώāĻž āϕ⧰āĻŋāĻ›āĻŋāϞāĨ¤


22. Gravitational force is proportional to what?āĻĒā§ā§°āĻļā§āύ: āϗ⧁⧰⧁āĻ¤ā§āĻŦāĻžāĻ•āĻ°ā§āώāĻŖ āĻŦāϞ āĻ•āĻŋāĻšā§° āϏāĻŽāĻžāύ⧁āĻĒāĻžāϤāĻŋāĻ• ?
Ans: Product of masses
Exp: More mass → more force. āĻŦā§āϝāĻžāĻ–ā§āϝāĻž: āĻ­ā§° āĻŦ⧇āĻ›āĻŋ āĻš’āϞ⧇ āĻŦāϞ āĻŦ⧇āĻ›āĻŋāĨ¤


23. Gravitational force is inversely proportional to what ? āĻĒā§ā§°āĻļā§āύ: āϗ⧁⧰⧁āĻ¤ā§āĻŦāĻžāĻ•āĻ°ā§āώāĻŖ āĻŦāϞ āĻ•āĻŋāĻšā§° āĻŦā§āϝ⧁āĻ¤ā§āĻ•ā§ā§°āĻŽ āĻ…āύ⧁āĻĒāĻžāϤāĻŋāĻ• ?
Ans: Square of distance
Exp: Distance increases → force decreases. āĻŦā§āϝāĻžāĻ–ā§āϝāĻž: āĻĻā§‚ā§°āĻ¤ā§āĻŦ āĻŦāĻžāĻĸāĻŧāĻŋāϞ⧇ āĻŦāϞ āĻ•āĻŽā§‡āĨ¤


24. Who measured the value of G experimentally ? āĻĒā§ā§°āĻļā§āύ: G-ā§° āĻŽāĻžāύ āϕ⧋āύ⧇ āĻĒā§ā§°āϝāĻŧā§‹āϗ⧇⧰⧇ āύāĻŋā§°ā§āĻŖāϝāĻŧ āϕ⧰āĻŋāĻ›āĻŋāϞ ?
Ans: Cavendish
Exp: Using torsion balance. āĻŦā§āϝāĻžāĻ–ā§āϝāĻž: āĻŸā§°ā§āϚāύ āĻŦā§āϝāĻžāϞ⧇āĻ¨ā§āϏ āĻŦā§āĻ¯ā§ąāĻšāĻžā§° āϕ⧰āĻŋāĨ¤


25. If distance becomes double, force becomes ? āĻĒā§ā§°āĻļā§āύ: āĻĻā§‚ā§°āĻ¤ā§āĻŦ āĻĻā§‹āϗ⧁āĻŖ āĻš’āϞ⧇ āĻŦāϞ āĻ•āĻŋāĻŽāĻžāύ āĻšāϝāĻŧ ?
Ans: 1/4
Exp: Due to inverse square law. āĻŦā§āϝāĻžāĻ–ā§āϝāĻž: āĻŦā§āϝ⧁āĻ¤ā§āĻ•ā§ā§°āĻŽ āĻŦā§°ā§āĻ— āύāĻŋāϝāĻŧāĻŽā§° āĻŦāĻžāĻŦ⧇āĨ¤


26. If mass becomes double, force becomes ? āĻĒā§ā§°āĻļā§āύ: āĻ­ā§° āĻĻā§‹āϗ⧁āĻŖ āĻš’āϞ⧇ āĻŦāϞ āĻ•āĻŋ āĻšāϝāĻŧ ?
Ans: Double
Exp: Force ∝ mass. āĻŦā§āϝāĻžāĻ–ā§āϝāĻž: āĻŦāϞ āĻ­ā§°ā§° āϏāĻŽāĻžāύ⧁āĻĒāĻžāϤāĻŋāĻ•āĨ¤


27. Why does the Moon revolve around the Earth ? āĻĒā§ā§°āĻļā§āύ: āϚāĻ¨ā§āĻĻā§ā§° āĻĒ⧃āĻĨāĻŋā§ąā§€ā§° āϚāĻžā§°āĻŋāĻ“āĻĢāĻžāϞ⧇ āĻ•āĻŋāϝāĻŧ āĻ˜ā§‚ā§°ā§‡ ?
Ans: Due to gravitation
Exp: Earth’s gravity provides centripetal force. āĻŦā§āϝāĻžāĻ–ā§āϝāĻž: āĻĒ⧃āĻĨāĻŋā§ąā§€ā§° āϗ⧁⧰⧁āĻ¤ā§āĻŦ āϕ⧇āĻ¨ā§āĻĻā§ā§°āĻžāĻ­āĻŋāĻŽā§āĻ– āĻŦāϞ āĻĒā§ā§°āĻĻāĻžāύ āϕ⧰⧇āĨ¤


28. Why does Earth revolve around the Sun ? āĻĒā§ā§°āĻļā§āύ: āĻĒ⧃āĻĨāĻŋā§ąā§€ āĻ¸ā§‚ā§°ā§āϝ⧰ āϚāĻžā§°āĻŋāĻ“āĻĢāĻžāϞ⧇ āĻ•āĻŋāϝāĻŧ āĻ˜ā§‚ā§°ā§‡ ?
Ans: Gravitational force
Exp: Sun’s gravity holds Earth in orbit. āĻŦā§āϝāĻžāĻ–ā§āϝāĻž: āĻ¸ā§‚ā§°ā§āϝ⧰ āϗ⧁⧰⧁āĻ¤ā§āĻŦ⧇ āĻĒ⧃āĻĨāĻŋā§ąā§€āĻ• āĻ•āĻ•ā§āώāĻĒāĻĨāϤ ā§°āĻžāϖ⧇āĨ¤


29. Is gravitational force always attractive ? āĻĒā§ā§°āĻļā§āύ: āϗ⧁⧰⧁āĻ¤ā§āĻŦāĻžāĻ•āĻ°ā§āώāĻŖ āĻŦāϞ āϏāĻĻāĻžāϝāĻŧ āφāĻ•ā§°ā§āώāĻŖā§€āϝāĻŧ āύ⧇ ?
Ans: Yes
Exp: No repulsive gravity exists. āĻŦā§āϝāĻžāĻ–ā§āϝāĻž: āϗ⧁⧰⧁āĻ¤ā§āĻŦāĻžāĻ•āĻ°ā§āώāĻŖ āĻŦāĻŋāĻ•āĻ°ā§āώāĻŖā§€āϝāĻŧ āύāĻšāϝāĻŧāĨ¤


30. Is gravity zero in space ? āĻĒā§ā§°āĻļā§āύ: āĻŽāĻšāĻžāĻ•āĻžāĻļāϤ āϗ⧁⧰⧁āĻ¤ā§āĻŦ āĻļā§‚āĻ¨ā§āϝ āύ⧇ ?
Ans: No
Exp: Gravity is weak but present. āĻŦā§āϝāĻžāĻ–ā§āϝāĻž: āϗ⧁⧰⧁āĻ¤ā§āĻŦ āĻ•āĻŽ āĻšāϞ⧇āĻ“ āĻĨāĻžāϕ⧇āĨ¤


31. How is gravity in a black hole ? āĻĒā§ā§°āĻļā§āύ: āĻŦā§āϞ⧇āĻ• āĻš’āϞāϤ āϗ⧁⧰⧁āĻ¤ā§āĻŦ āϕ⧇āύ⧇āĻ•ā§ā§ąāĻž ?
Ans: Extremely strong
Exp: Even light cannot escape. āĻŦā§āϝāĻžāĻ–ā§āϝāĻž: āĻĒā§‹āĻšā§°ā§‹ āĻĒāϞāĻžāĻŦ āĻ¨ā§‹ā§ąāĻžā§°ā§‡āĨ¤


32. According to Einstein, what is gravity ? āĻĒā§ā§°āĻļā§āύ: āφāχāύāĻˇā§āϟāĻžāχāύ⧰ āĻŽāϤ⧇ āϗ⧁⧰⧁āĻ¤ā§āĻŦ āĻ•āĻŋ ?
Ans: Curvature of space-time
Exp: Mass bends space-time. āĻŦā§āϝāĻžāĻ–ā§āϝāĻž: āϭ⧰⧇ āĻ¸ā§āĻĨāĻžāύ-āĻ•āĻžāϞ āĻŦ⧇āρāĻ•āĻžāϝāĻŧ


33. Tides are caused due to what ? āĻĒā§ā§°āĻļā§āύ: āĻœā§‹ā§ąāĻžā§°-āĻ­āĻžāϟāĻž āĻ•āĻŋāĻšā§° āĻŦāĻžāĻŦ⧇ āĻšāϝāĻŧ ?
Ans: Moon and Sun’s gravity
Exp: Gravitational pull of Moon is dominant. āĻŦā§āϝāĻžāĻ–ā§āϝāĻž: āϚāĻ¨ā§āĻĻā§ā§°ā§° āϗ⧁⧰⧁āĻ¤ā§āĻŦ āĻŦ⧇āĻ›āĻŋ āĻĒā§ā§°āĻ­āĻžā§ąāĻļāĻžāϞ⧀āĨ¤


34. Weightlessness occurs in which condition ? āĻĒā§ā§°āĻļā§āύ: āĻ­āĻžā§°āĻļā§‚āĻ¨ā§āϝāϤāĻž āϕ⧋āύ āĻ…ā§ąāĻ¸ā§āĻĨāĻžāϤ āĻšāϝāĻŧ ?
Ans: Free fall
Exp: No normal reaction acts. āĻŦā§āϝāĻžāĻ–ā§āϝāĻž: āϕ⧋āύ⧋ āĻ…āĻ­āĻŋāϞāĻŽā§āĻŦ āĻŦāϞ āύāĻžāĻĨāĻžāϕ⧇āĨ¤


35. In which direction does Earth pull objects ? āĻĒā§ā§°āĻļā§āύ: āĻĒ⧃āĻĨāĻŋā§ąā§€āϝāĻŧ⧇ āĻŦāĻ¸ā§āϤ⧁ āϕ⧋āύ āĻĻāĻŋāĻļ⧇ āϟāĻžāύ⧇ ?
Ans: Downwards
Exp: Towards Earth’s center. āĻŦā§āϝāĻžāĻ–ā§āϝāĻž: āĻĒ⧃āĻĨāĻŋā§ąā§€ā§° āϕ⧇āĻ¨ā§āĻĻā§ā§°ā§° āĻĻāĻŋāĻļ⧇āĨ¤


36. On which planet is g more ? āĻĒā§ā§°āĻļā§āύ: āϕ⧋āύ āĻ—ā§ā§°āĻšāϤ g āĻŦ⧇āĻ›āĻŋ ?
Ans: On more massive planets
Exp: Greater mass → greater gravity. āĻŦā§āϝāĻžāĻ–ā§āϝāĻž: āĻ­ā§° āĻŦ⧇āĻ›āĻŋ → āϗ⧁⧰⧁āĻ¤ā§āĻŦ āĻŦ⧇āĻ›āĻŋāĨ¤


37. Why is weight less on the Moon ? āĻĒā§ā§°āĻļā§āύ: āϚāĻ¨ā§āĻĻā§ā§°āϤ āĻ­āĻžā§° āĻ•āĻŽ āĻ•āĻŋāϝāĻŧ ?
Ans: g is less
Exp: Moon has smaller mass. āĻŦā§āϝāĻžāĻ–ā§āϝāĻž: āϚāĻ¨ā§āĻĻā§ā§°ā§° āĻ­ā§° āĻ•āĻŽāĨ¤


38. How does g change with height and depth ? āĻĒā§ā§°āĻļā§āύ: āωāĻšā§āϚāϤāĻž āφ⧰⧁ āĻ—āϭ⧀⧰āϤāĻžā§° āϏ⧈āϤ⧇ g āϕ⧇āύ⧇āĻ•ā§ˆ āϏāϞāύāĻŋ āĻšāϝāĻŧ ?
Ans: Decreases
Exp: Distance from effective mass changes. āĻŦā§āϝāĻžāĻ–ā§āϝāĻž: āĻ•āĻžā§°ā§āϝāϕ⧰ āĻĻā§‚ā§°āĻ¤ā§āĻŦ āϏāϞāύāĻŋ āĻšāϝāĻŧāĨ¤


39. What keeps planets in their orbits ? āĻĒā§ā§°āĻļā§āύ: āĻ—ā§ā§°āĻšāĻŦā§‹ā§°āĻ• āĻ•āĻ•ā§āώāĻĒāĻĨāϤ āĻ•āĻŋāĻšā§‡ ā§°āĻžāϖ⧇ ?
Ans: Sun’s gravitational force
Exp: Provides centripetal force. āĻŦā§āϝāĻžāĻ–ā§āϝāĻž: āϕ⧇āĻ¨ā§āĻĻā§ā§°āĻžāĻ­āĻŋāĻŽā§āĻ– āĻŦāϞ āĻĒā§ā§°āĻĻāĻžāύ āϕ⧰⧇āĨ¤


40. Gravitation is which type of force ? āĻĒā§ā§°āĻļā§āύ: āϗ⧁⧰⧁āĻ¤ā§āĻŦāĻžāĻ•āĻ°ā§āώāĻŖ āϕ⧇āύ⧇āĻ•ā§ā§ąāĻž āĻŦāϞ?
Ans: Universal force
Exp: Acts between any two masses. āĻŦā§āϝāĻžāĻ–ā§āϝāĻž: āϝāĻŋāϕ⧋āύ⧋ āĻĻ⧁āϟāĻž āĻ­ā§°ā§° āĻŽāĻžāϜāϤ āĻ•āĻžā§°ā§āϝ āϕ⧰⧇āĨ¤