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Agniveer Air Force Gravitation — practice questions

Explore 27 free Gravitation questions in Agniveer Air Force Physics. Open each question or exercise to read its content, reference answers and available explanation.

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Gravitation questions and exercises with answers

Showing questions 1–27 of 27.

The universal gravitational constant $G$ has the SI value approximately:Read the answer and worked solution →For a satellite of mass $m$ orbiting Earth at radius $r$ (from the centre), the orbital velocity is:Read the answer and worked solution →The escape velocity from the Earth's surface is approximately ($R = 6.4 \times 10^6$ m, $g = 9.8$ m/s²):Read the answer and worked solution →Newton's law of gravitation states the force between two masses is:Read the answer and worked solution →At the surface of Earth, acceleration due to gravity g equals:Read the answer and worked solution →At a height h above Earth's surface where h ≪ R, g' equals:Read the answer and worked solution →Weigh up Earth's gravity and speedsRead the answer and worked solution →Conserved, or not conserved?Read the answer and worked solution →True or false: conservation under gravityRead the answer and worked solution →Complete the weightlessness explanationRead the answer and worked solution →True or false: weightlessnessRead the answer and worked solution →Kepler's third lawRead the answer and worked solution →Assertion and reasonRead the answer and worked solution →Two are true, one is notRead the answer and worked solution →Three of these are wrong. Find the one that holds.Read the answer and worked solution →Tap every quantity conserved for orbital motionRead the answer and worked solution →Flip and pair: law with what it saysRead the answer and worked solution →Spot the one that does not belongRead the answer and worked solution →Order the reasoning: why an astronaut floatsRead the answer and worked solution →True or false: Kepler's lawsRead the answer and worked solution →Which law is being described?Read the answer and worked solution →Orbits and satellitesRead the answer and worked solution →Tap every true statement about orbital motionRead the answer and worked solution →Complete Kepler's third lawRead the answer and worked solution →Spot the one that does not belongRead the answer and worked solution →Flip and pair: statement with its subjectRead the answer and worked solution →Assertion and reason: orbitsRead the answer and worked solution →

Worked practice questions

The universal gravitational constant $G$ has the SI value approximately:

  1. $6.67 \times 10^{-11}\,\mathrm{N\,m^2/kg^2}$
  2. $9.81\,\mathrm{m/s^2}$
  3. $6.022 \times 10^{23}\,\mathrm{/mol}$
  4. $1.6 \times 10^{-19}\,\mathrm{C}$
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Correct answer: A. $6.67 \times 10^{-11}\,\mathrm{N\,m^2/kg^2}$

Universal gravitational constant $G = 6.67 \times 10^{-11}$ N·m²/kg² in SI units, the same everywhere in the universe. The units come from Newton's law $F = G m_1 m_2 / r^2$: $\dfrac{\text{kg} \cdot \text{kg}}{\text{m}^2} \cdot [G] = \text{N}$ so $[G] = \text{N} \cdot \text{m}^2 / \text{kg}^2$. Option B is the local acceleration due to gravity $g$ (not constant). Option C is Avogadro. Option D is the electronic charge.

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For a satellite of mass $m$ orbiting Earth at radius $r$ (from the centre), the orbital velocity is:

  1. $v = \sqrt{\dfrac{GM}{r}}$
  2. $v = \sqrt{2 GM r}$
  3. $v = \dfrac{GM}{r^2}$
  4. $v = G M$
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Correct answer: A. $v = \sqrt{\dfrac{GM}{r}}$

Set gravitational force equal to centripetal force on the satellite: $\dfrac{GMm}{r^2} = \dfrac{mv^2}{r}$ The $m$ cancels. Solve for $v$: $v^2 = \dfrac{GM}{r}$, so $v = \sqrt{\dfrac{GM}{r}}$. Orbital velocity at Earth's surface is about $7.9$ km/s (about 28,000 km/h). Option B looks similar but has a 2 inside the square root — that's the **escape velocity** $v_e = \sqrt{2GM/r}$, which is $\sqrt{2}$ times the orbital speed at the same radius. A textbook trap.

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The escape velocity from the Earth's surface is approximately ($R = 6.4 \times 10^6$ m, $g = 9.8$ m/s²):

  1. $7.9$ km/s
  2. $11.2$ km/s
  3. $20$ km/s
  4. $1000$ m/s
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Correct answer: B. $11.2$ km/s

Escape velocity from Earth's surface: $v_e = \sqrt{2gR}$ (using the surface relation $GM/R^2 = g$). $v_e = \sqrt{2 \times 9.8 \times 6.4 \times 10^6} = \sqrt{1.25 \times 10^8} \approx 1.12 \times 10^4$ m/s $= 11.2$ km/s. Option A ($7.9$ km/s) is the *orbital* velocity at Earth's surface, smaller by a factor of $\sqrt{2}$. That trap is identical to the one in the orbital-velocity question.

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