Gravitational fields and Newton's law of gravitationEdexcel International A Level Physics: Flashcards
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What is a gravitational field?
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- What is a gravitational field?
- A region where a mass experiences a force because of its mass.
- Define gravitational field strength.
- The force per unit mass at a point in the field: g = F/m (unit N kg⁻¹).
- State Newton's law of universal gravitation.
- : attractive, proportional to the product of the masses and inversely proportional to the square of the distance between centres.
- How does g change if the distance from a point mass is doubled?
- It falls to one quarter (inverse square law).
- Derive the field strength of a point mass.
- g = F/m = (GMm/r²)/m = GM/r², as m cancels.
- What does r mean in gravitational equations?
- The distance from the centre of the mass, not the height above the surface.
- Define gravitational potential.
- The work done per unit mass in bringing a small mass from infinity to the point.
- Give the equation for gravitational potential of a point mass.
- (J kg⁻¹)
- Why is gravitational potential negative?
- It is zero at infinity and the field does work as the mass moves in, so energy must be supplied to return it to infinity.
- What is a neutral point?
- A point where the fields of two bodies are equal and opposite, so the resultant field strength is zero.
- State one similarity between gravitational and electric fields.
- Both are radial and obey an inverse square law.
- State one difference between gravitational and electric forces.
- Gravitational forces are always attractive; electric forces can be attractive or repulsive.
- Why is gravity weak compared with electric force in an atom?
- G is very small compared with k; the ratio for an electron and proton is about 10³⁹.
Exam questions on Gravitational fields and Newton's law of gravitation
- Treat the Earth as a uniform sphere of mass 5.97 × 10²⁴ kg and radius 6.37 × 10⁶ m. A communications satellite of mass 450 kg is 3.59 × 10⁷ m above the Earth's surface. The gravitational constant G = 6.67 × 10⁻¹¹ N m² kg⁻².Calculate the gravitational potential at the position of the satellite.2 marks
- The Earth has mass 5.97 × 10²⁴ kg and the Moon has mass 7.35 × 10²² kg. The distance between their centres is 3.84 × 10⁸ m. Treat both as point masses at their centres. G = 6.67 × 10⁻¹¹ N m² kg⁻².Calculate the gravitational field strength of the Moon at the centre of the Earth, and state its direction.2 marks
- In a hydrogen atom an electron and a proton are separated by 5.3 × 10⁻¹¹ m. The electron has mass 9.11 × 10⁻³¹ kg and the proton has mass 1.67 × 10⁻²⁷ kg. Each has a charge of magnitude 1.60 × 10⁻¹⁹ C. G = 6.67 × 10⁻¹¹ N m² kg⁻² and the constant in Coulomb's law, k = 1/(4πε₀), is 8.99 × 10⁹ N m² C⁻².Calculate the gravitational force between the electron and the proton.3 marks
Written by the Exaim team, led by Shaun Daswani (Head of Upper Secondary, Improve ME Institute; MSc Financial Mathematics, Imperial College London; BSc, UCL) and Jason Daswani (operational lead, Improve ME Institute; LSE).