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GCSE Physics Revision

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GCSE Physics revision

Newton's First Law

Forces, accelerations and Newton's Laws of motion

AQA 4.5.6.2.1
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AQA student objectives

Learning pathway

All · Most · Some

ALL 🎯

Apply Newton’s First Law to explain the motion of objects moving with a uniform velocity and objects where the speed and/or direction changes.

MOST 🎯🎯

Interpret results or representations related to newton's first law.

SOME 🎯🎯🎯

Analyse an unfamiliar problem involving newton's first law and justify the method or conclusion.

Revision summary

Key knowledge

Read on screen, then print for Cornell-style active revision.

Newton's First Law of Motion

  • Newton's first law states that a resultant force is required to change the motion of an object — without one, motion stays the same.
  • A stationary object with zero resultant force will remain stationary, and a moving object with zero resultant force will continue at the same velocity.
  • This law applies to both stationary and moving objects, meaning balanced forces always result in unchanged motion.

Resultant Force and Unbalanced Forces

  • A resultant force is the single overall force that results from combining all forces acting on an object.
  • If force arrows are unequal in opposite directions, there is a non-zero resultant force, causing the object to accelerate in the direction of the larger force.
  • A non-zero resultant force means the forces are unbalanced, which is the condition required for acceleration to occur.

Newton's Second Law of Motion

  • Newton's second law states that a non-zero resultant force acting on an object will cause it to accelerate.
  • The resultant force is directly proportional to the acceleration it produces — doubling the force doubles the acceleration.
  • The relationship is expressed as F = ma, where F is resultant force in newtons (N), m is mass in kilograms (kg), and a is acceleration in m/s².

Five Possible Effects of Acceleration

  • If a stationary object experiences a resultant force, it will begin to move in the direction of that force.
  • If an object is already moving in the same direction as the resultant force, it will speed up.
  • If the resultant force acts opposite to the direction of motion, the object will slow down or potentially stop entirely.
  • A resultant force can also cause a change in direction without a change in speed, which still counts as acceleration.

Circular Motion and Changing Velocity

  • Acceleration is defined as the change in velocity divided by the change in time: a = Δv
  • Δt
  • .
  • Velocity is a vector quantity determined by both speed and direction, so a change in direction alone constitutes a change in velocity.
  • The Moon orbits the Earth at a constant speed but is always accelerating because its direction continuously changes.
  • The Earth's gravitational pull acts perpendicular to the Moon's motion, keeping it in a circular orbit with a constantly changing velocity.

Applying F = ma: Worked Example

  • To find acceleration, first calculate the resultant force by subtracting the smaller force from the larger: e.g. 42 N − 30 N = 12 N to the right.
  • Rearranging F = ma gives a = m F
  • , so with a mass of 0.25 kg and a resultant force of 12 2
  • 12 N, the acceleration is 0.25
  • = 48 m/s .

Inertia and Inertial Mass

  • Inertia is the tendency of an object to resist changes to its motion — objects at rest stay at rest and objects in motion stay in motion unless acted on by a resultant force.
  • Inertial mass measures how difficult it is to change an object's velocity, and is found using m = Fa from Newton's second law.
  • A larger inertial mass means a greater force is needed to produce the same acceleration, so massive objects like the Moon are very hard to accelerate.