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Edexcel A Level (IAL) Physics-5.33 Gravitational Field due to a Point Mass- Study Notes- New Syllabus

Edexcel A Level (IAL) Physics -5.33 Gravitational Field due to a Point Mass- Study Notes- New syllabus

Edexcel A Level (IAL) Physics -5.33 Gravitational Field due to a Point Mass- Study Notes -Edexcel A level Physics – per latest Syllabus.

Key Concepts:

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Edexcel A level Physics-Study Notes- All Topics

Derivation and Use of the Gravitational Field Equation for a Point Mass

The gravitational field strength due to a point mass can be derived directly from Newton’s law of universal gravitation and the definition of gravitational field strength.

Starting Definitions

Newton’s law of universal gravitation:

\( F = \dfrac{G M m}{r^2} \)

  • \( M \) = mass creating the gravitational field (kg)
  • \( m \) = test mass (kg)
  • \( r \) = distance from the centre of mass \( M \) (m)
  • \( G \) = gravitational constant

Definition of gravitational field strength:

\( g = \dfrac{F}{m} \)

 Derivation of \( g = \dfrac{GM}{r^2} \)

Substitute the gravitational force into the definition of field strength:

\( g = \dfrac{F}{m} = \dfrac{1}{m}\left(\dfrac{G M m}{r^2}\right) \)

Cancel the mass \( m \):

\( g = \dfrac{G M}{r^2} \)

Conclusion: The gravitational field strength due to a point mass depends only on the mass creating the field and the distance from it.

Meaning of the Equation

\( g = \dfrac{G M}{r^2} \)

  • \( g \) = gravitational field strength (N kg⁻¹)
  • \( M \) = mass producing the field (kg)
  • \( r \) = distance from the centre of the mass (m)

Key ideas:

  • Gravitational field strength follows an inverse-square law.
  • Doubling \( r \) reduces \( g \) by a factor of 4.
  • The field strength is independent of the test mass.

Direction of the Gravitational Field

  • The gravitational field is radial.
  • It always acts towards the centre of the mass.
  • The direction of \( g \) is the direction of the force on a unit mass.

Application to the Earth

For the Earth:

  • \( M \) = mass of the Earth
  • \( r \) = distance from the centre of the Earth

Near the Earth’s surface:

\( g \approx 9.8\,\mathrm{N\,kg^{-1}} \)

This explains why \( g \) decreases with altitude.

Using the Equation in Calculations

  • Ensure all quantities are in SI units.
  • Use distance from the centre of the mass, not the surface.
  • Apply inverse-square reasoning where appropriate.

Rearranged forms:

\( M = \dfrac{g r^2}{G} \)

\( r = \sqrt{\dfrac{G M}{g}} \)

Example (Easy)

Explain why the gravitational field strength decreases as distance from a planet increases.

▶️ Answer / Explanation

Gravitational field strength follows an inverse-square law, so increasing distance reduces the field strength.

Example (Medium)

Calculate the gravitational field strength \( 1.0\times10^{7}\,\mathrm{m} \) from the centre of the Earth \( (M = 6.0\times10^{24}\,\mathrm{kg}) \).

▶️ Answer / Explanation

\( g = \dfrac{(6.67\times10^{-11})(6.0\times10^{24})}{(1.0\times10^{7})^2} \)

\( g \approx 4.0\,\mathrm{N\,kg^{-1}} \)

Example (Hard)

The gravitational field strength at a distance \( r \) from a planet is \( g \). What is the field strength at distance \( 2r \)?

▶️ Answer / Explanation

Using the inverse-square law:

\( g_{\text{new}} = \dfrac{g}{4} \)

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