GRADE 10 · KINEMATICS
Free fall and circular motion
Fall without resistance and the kinematics of uniform rotation.
Read the full lesson theory here without an account. In the interactive lesson, the same theory is presented as cards, followed by questions with feedback and practice problems. Your progress is saved.
Understanding step by step
At the top of a vertical throw, a ball stops for an instant. A point on a uniformly rotating wheel keeps the same speed. Why is there acceleration in both cases? Let us examine changes in the magnitude and direction of velocity separately.
Free fall
Release a compact heavy object and a compact light one together; they fall almost together. In the model without air resistance, gravity alone acts on both: this is free fall. Near Earth's surface, g\approx9{,}8\,\text{м/с}^2 points downwards and is independent of mass. This is an experimental finding; later, dynamics will connect it with gravitational force and inertia. A sheet of paper falling in air tests a different model.
Upward motion can also be free fall
The hand gives a ball its initial velocity during a throw, but stops pushing once it lets go. Gravity keeps changing the velocity downwards: it reduces the upward velocity on the way up and increases the downward velocity on the way down. Thus free fall includes upward motion when gravity is the only force. Free describes the conditions, not the direction of the trajectory.
Released from rest
Release a body without a push and point the axis downwards. Then v_0=0, a=g, and the familiar velocity relation becomes v=gt. With g=10 m/s², speed increases by 10 m/s each second. Doubling time doubles speed; reducing g reduces it for the same time. At t=0, the formula gives zero, as release from rest requires. Throwing the body initially would require a different initial condition.
Distance grows faster
During the first second the body is still slow; during the next it is faster. The average speed from release to time t is gt/2, so h=gt^2/2. Here h is the downward distance in metres. Doubling time quadruples this distance because both time and average speed double. The model requires constant g, an initial state of rest and negligible resistance; it cannot describe an entire parachute descent.
When height is known
If the height is known, find how long the velocity has to build up. From h=gt^2/2 we get t=\sqrt{2h/g}, then v=\sqrt{2gh}. Choose the positive root: these are a duration and a speed. Quadrupling height doubles both time and speed. With smaller g, a body falls from the same height for longer but reaches a lower speed: the longer time does not fully compensate for the smaller acceleration.
At the top of the throw
Compare instants just before and after the top of a throw: the ball was moving up and will soon be moving down. Its velocity changes even as it passes through zero. At the top, v=0, but acceleration remains g downwards. Let H be the rise above the launch point and v_0 the initial speed. If acceleration also vanished and never returned, the ball would remain at rest at the top.
Maximum height
Point the axis upwards: a_x=-g, and at the top v_x=0. From v_x^2-v_{0x}^2=2a_xs_x we obtain H=v_0^2/(2g). Doubling launch speed quadruples the height: the ball starts faster and takes longer to lose its speed. Larger g reduces the rise. At v_0=0, there is no rise. We neglect air resistance and variation of g with height.
Turning the velocity vector
Mark a point on the rim of a uniformly rotating wheel. Over a short time its speed stays the same, but the velocity arrow turns. The difference between two nearby arrows points towards the centre, so acceleration points there too. Velocity itself is tangent to the circle: it is the instantaneous direction of motion. Radius R is measured in metres. Turning velocity is a change of vector even with a constant speedometer reading.
How sharp is the turn?
In time \Delta t, velocity turns through an angle of about v\Delta t/R. The change in the velocity arrow is then about v\times v\Delta t/R. Divide by time and take the limit of a short interval to obtain a_{\text{ц}}=v^2/R. One factor v comes from the arrow's length, the other from how quickly it turns. Doubling speed requires four times the acceleration; at the same speed, a larger radius makes the turn gentler.
Period and frequency
Time one complete return of the mark on the wheel. This is period T, in seconds. Frequency \nu counts revolutions per second and is measured in hertz: \nu=1/T. If a revolution takes 2 s, half a revolution occurs per second: 0.5 Hz. Halving the period doubles frequency. Very slow rotation has a long period and a frequency close to zero; a stationary point has no finite revolution period.
Linear speed
In one period the mark travels the full circumference 2\pi R. Therefore v=2\pi R/T=2\pi R\nu. At fixed radius, halving the period doubles speed. At fixed period, a point at twice the radius covers twice the distance and moves twice as fast. To predict a change, state what is held constant: equal periods and equal linear speeds are different conditions.
Angle per second
Two points on the same wheel turn through the same angle each second but travel different distances. Angular velocity \omega gives a shared description: for uniform rotation, \omega=\varphi/t=2\pi\nu, in rad/s. Here \varphi is the angle swept from the chosen starting position in time t; a full revolution contains 2\pi radians. Radians link arc length to radius: arc length equals radius times angle in radians.
Two descriptions of rotation
The arc travelled per second equals radius times angle per second: v=\omega R. Substitution gives a_{\text{ц}}=\omega^2R. A larger radius now seems to increase acceleration, whereas in v^2/R it decreased it. There is no contradiction: here \omega is fixed, so the outer point also moves faster. As R\to0 at fixed \omega, its linear speed and acceleration approach zero.
Work through an example
A point particle is released from rest. How far does it travel in 2 s without air resistance? Take g=10 м/с².
Let's look at an example · 1
The conditions match release from rest with constant g.
Let's look at an example · 2
We need distance from time, so choose h=gt²/2.
Let's look at an example · 3
Substitute: h=10×2²/2=20 м. Final speed v=gt=20 м/с.
Worked example · 4
Check using average speed: (0+20)/2×2=20 м.
Let's check the result
In 2 s, the body travels 20 m downwards and reaches a speed of 20 m/s. Its average speed was 10 m/s: it covered only 5 m in the first second, then 15 m in the second.
Key idea · 1
Zero velocity at one instant does not imply zero acceleration: gravity continues changing the ball's velocity at the top.
Key idea · 2
The formulas v = gt and h = gt²/2 describe release from rest with constant g and no resistance.
Key idea · 3
In circular motion, acceleration turns the velocity. Discuss the radius dependence together with what is held constant: v or ω.
Where do we go next?
Next we connect acceleration with the net force.
Basic Concepts
Free fall
Motion under gravity alone, neglecting resistance from the surrounding medium.
When air resistance is negligible, mass does not affect free-fall acceleration: all bodies have the same g.
Uniform circular motion
Motion along a circle at constant speed.
The magnitude of the velocity is constant, but its direction is constantly changing, so the body has an acceleration towards the center of the circle.
Physical quantities
Free-fall acceleration
gAcceleration of a body in free fall near the surface of a celestial body.
Unit: metre per second squared · \frac{\mathrm{м}}{\mathrm{с}^2}
Maximum height
HThe greatest height a body rises.
Unit: meter · \mathrm{м}
Radius
RThe distance from the center of a circle to its point.
Unit: meter · \mathrm{м}
Orbital period
TThe time for one complete revolution.
Unit: second · \mathrm{с}
Revolution frequency
\nuThe number of complete revolutions per unit time.
Unit: hertz · \mathrm{Гц}
Angular velocity
\omegaThe rate of change of the rotation angle.
Unit: radians per second · \frac{\mathrm{рад}}{\mathrm{с}}
Rotation angle
\varphiThe angle swept by the radius to the body.
Unit: radian · \mathrm{рад}
Centripetal acceleration
a_{\text{ц}}Acceleration directed towards the center of the circle.
Unit: metre per second squared · \frac{\mathrm{м}}{\mathrm{с}^2}
Lesson formulas
Free-fall speed
v=gtThe speed of a body released from rest grows in proportion to time.
Fall distance from time
h=\frac{gt^2}{2}The distance fallen freely from rest is determined by time and acceleration.
Maximum rise height
H=\frac{v_0^2}{2g}The maximum height of a vertical throw is determined by initial speed.
Speed from fall height
v=\sqrt{2gh}Free-fall speed from rest is determined by the vertical distance fallen.
Fall time from height
t=\sqrt{\frac{2h}{g}}The time to fall freely from rest is determined by the fall height.
Linear speed in circular motion
v=\frac{2\pi R}{T}=2\pi R\nuIn one period, the body travels one full circumference.
Relation between linear and angular speeds
v=\omega RLinear speed equals angular speed multiplied by radius.
Angular velocity
\omega=\frac{\varphi}{t}=2\pi\nuFor uniform rotation, angular speed is the angle swept divided by time, and also two pi times frequency.
Centripetal acceleration from speed
a_{\text{ц}}=\frac{v^2}{R}Centripetal acceleration grows with the square of speed and, at fixed speed, decreases as radius increases.
Centripetal acceleration from angular speed
a_{\text{ц}}=\omega^2RCentripetal acceleration equals angular speed squared multiplied by radius.
Test the relationship
Make a prediction first. The button changes the stated quantity; then compare the result and explore other values.
Uniform circular motion
ω = v/R; x = R cos(ωt); y = R sin(ωt); a = v²/R; T = 2πR/v (v > 0)
A point particle moves counterclockwise around a circle at constant speed, starting at (R, 0) when t = 0. Arrows show directions; their lengths are schematic. This is a kinematic model: the source of force is not specified. At v = 0 the particle is at rest and the period is undefined.
At R = 2 m, speed increases from 2 to 4 m/s. How will the magnitude of acceleration change?
Initial values
Calculated result
- |v|
- 2 м/с
- a
- 2 м/с²
- T
- 6.283 с
- vₓ
- 0 м/с
- vᵧ
- 2 м/с
Explaining the result
Doubling v quadruples the acceleration magnitude, from 2 to 8 m/s². At fixed v, doubling R halves a. Velocity is tangent to the circle; acceleration points toward the centre, perpendicular to velocity. The graphs of vₓ and vᵧ change, but √(vₓ² + vᵧ²) = v stays constant. A real net force must provide this acceleration on a circular orbit.
Related formulas
The same formulas in the reference, with symbols and units.
Problems on this topic
Statements, answer options and the walkthrough.