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Mnemonics: Gravitation | Physics Class 11 - NEET PDF Download

Master the complexities of gravitation with ease! This document provides creative and efficient mnemonics for key concepts like escape velocity and Kepler's laws, ensuring quick understanding and application in numericals. Accelerate your learning journey with these memorable tools!

Mnemonics: Gravitation | Physics Class 11 - NEET1. Escape Velocity

Mnemonic: "Whole Root Two Gravity Rocket Escapes at 11.2!"

  • Whole Root: Indicates the square root symbol in the escape velocity formula: Mnemonics: Gravitation | Physics Class 11 - NEET
  • Two: Refers to the factor of 2 in the formula.
  • Gravity: Represents gg, the acceleration due to gravity.
  • Rocket : Represents Radius of the planet (6.37×106m for Earth)
  • Escapes: Highlights that the escape velocity is the speed needed for a rocket or object to escape Earth's gravitational pull.

  • At 11.2: Refers to the approximate escape velocity of Earth, which is 11.2 km/s.

Wil be used in many numericals. So learn the formula!

2. Kepler's Laws of Planetary Motion

Mnemonic: "Planets Eat Fruits at Equal Interval 2/3 Times"

  •  Planet Eat Fruits:  - Refers to Kepler's First Law: Planets move in Elliptical orbits, with the Sun at one of the Foci.
  • Equal Interval - Refers to Kepler's Second Law: A line joining a planet and the Sun sweeps out Equal areas in Equal intervals of time, irrespective of the planet's position in its orbit.
  •  2/3 Times" - Refers to Kepler's Third Law: The square of the planet’s orbital period (T2) is proportional to the cube of the semi-major axis (R3)

T^2 \propto R^3T2 ∝ R3

Mnemonics: Gravitation | Physics Class 11 - NEET


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FAQs on Mnemonics: Gravitation - Physics Class 11 - NEET

1. What is the law of universal gravitation?
Ans. The law of universal 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. This can be mathematically expressed as F = G(m1*m2)/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 gravitational force vary with distance?
Ans. Gravitational force varies inversely with the square of the distance between two objects. This means that as the distance between the objects increases, the gravitational force decreases rapidly. Specifically, if the distance is doubled, the gravitational force becomes one-fourth of its original value, demonstrating that distance has a significant effect on the strength of the gravitational attraction.
3. What is the significance of the gravitational constant (G)?
Ans. The gravitational constant (G) is a key quantity in the law of universal gravitation. It quantifies the strength of gravity in the universe and is essential for calculations involving gravitational force. Its approximate value is 6.674 × 10⁻¹¹ N(m/kg)². G is crucial for understanding gravitational interactions between masses, including planetary motion, satellite orbits, and the behavior of objects in a gravitational field.
4. How does gravity affect objects in free fall?
Ans. In free fall, all objects experience the same acceleration due to gravity, regardless of their mass. This acceleration is approximately 9.81 m/s² near the Earth's surface. This means that in a vacuum, where air resistance is negligible, two objects dropped simultaneously will fall at the same rate and hit the ground at the same time, demonstrating that gravitational acceleration is uniform for all objects.
5. What are some real-life applications of gravitational principles?
Ans. Gravitational principles are applied in various real-life scenarios, including satellite navigation systems (like GPS), where the gravitational pull of Earth influences satellite orbits. Additionally, engineers use gravitational calculations in constructing buildings to ensure stability and safety. Understanding gravitation is also essential in astronomy for calculating the motion of celestial bodies and predicting phenomena such as eclipses and tides.
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