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Gravitation

Physics

Useful for: OSSC RHT — Regular High School Teacher, OSEPA Upper Primary — Science, OSSC Science, OSSSC Govt TGT Science — PCM, SSB Lecturer (Degree Colleges), SSB TGT PCM

Overview

Gravitation is the attractive force between all masses; it keeps planets in orbit and gives objects weight.

Key points

  • Newton’s law of gravitation: F = G m₁ m₂ / r², with G ≈ 6.67 × 10⁻¹¹ N m² kg⁻².
  • Acceleration due to gravity on Earth is about 9.8 m/s².
  • Weight = mg; mass stays constant everywhere, weight changes.
  • An object weighs about one-sixth as much on the Moon as on Earth.
  • Kepler’s laws: elliptical orbits, equal areas in equal times, T² ∝ r³.
  • Escape velocity from Earth is about 11.2 km/s.

Explanation

  • g decreases with altitude and depth and is slightly higher at the poles.
  • Geostationary satellites orbit at about 36,000 km with a 24-hour period.
  • Free fall: all objects fall with the same acceleration without air resistance.
  • Tides are caused mainly by the Moon’s gravity.
  • Doubling distance reduces force to one-quarter.

Step by step

  1. Identify the concept, law or fact asked.
  2. Recall the definition, formula, example or year.
  3. Apply it and eliminate mismatched options.

Examples

  • A 60 kg person weighs about 588 N on Earth (60 × 9.8).
  • On the Moon the same person weighs about one-sixth, about 98 N.
  • Doubling the distance between two masses → force becomes one-quarter.

Traps and advanced points

  • Trap: Saying mass changes on the Moon.
  • Trap: Heavier objects fall faster (in vacuum they don’t).
  • Trap: Wrong escape velocity.

Quick revision

  • F ∝ 1/r².
  • g ≈ 9.8 m/s²; Moon weight 1/6.
  • Escape velocity 11.2 km/s.

Practice MCQs

  1. The force with which the Earth pulls objects towards it is —

    1. friction
    2. gravity
    3. magnetism
    4. tension

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    Answer: (b) gravity. Gravity gives objects weight.

  2. Acceleration due to gravity on Earth is about —

    1. 6.67 m/s²
    2. 9.8 m/s²
    3. 11.2 m/s²
    4. 1.6 m/s²

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    Answer: (b) 9.8 m/s². g ≈ 9.8 m/s².

  3. A 60 kg person weighs about how much on Earth?

    1. 600 kg
    2. 6 N
    3. 60 N
    4. 588 N

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    Answer: (d) 588 N. 60 × 9.8 = 588 N.

  4. On the Moon, an object weighs about —

    1. six times
    2. double
    3. the same
    4. one-sixth

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    Answer: (d) one-sixth. Moon’s g is about 1/6.

  5. Mass of an object on the Moon —

    1. stays the same
    2. doubles
    3. becomes zero
    4. becomes one-sixth

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    Answer: (a) stays the same. Mass does not change.

  6. If the distance between two masses doubles, the force becomes —

    1. half
    2. one-quarter
    3. double
    4. four times

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    Answer: (b) one-quarter. Inverse square law.

  7. Escape velocity from Earth is about —

    1. 7.9 km/s
    2. 11.2 km/s
    3. 3 km/s
    4. 30 km/s

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    Answer: (b) 11.2 km/s. 11.2 km/s.

  8. Kepler’s third law states that —

    1. T ∝ r
    2. F ∝ 1/r
    3. orbits are circles
    4. T² ∝ r³

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    Answer: (d) T² ∝ r³. Harmonic law.

  9. The value of G is about —

    1. 3 × 10⁸
    2. 1.6 × 10⁻¹⁹
    3. 9.8
    4. 6.67 × 10⁻¹¹ N m² kg⁻²

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    Answer: (d) 6.67 × 10⁻¹¹ N m² kg⁻². Universal constant.

  10. In a vacuum, a feather and a coin dropped together —

    1. do not fall
    2. the coin lands first
    3. land together
    4. the feather lands first

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    Answer: (c) land together. Same acceleration.

More topics in this chapter

Notes and questions are written by Kundali IQ for practice. They are not official papers; always check the latest official notification for the syllabus and pattern.