Kinematics (Extended Treatment)
This document extends the core kinematics material with deeper derivations, multi-stage problems,
projectile motion in two dimensions, and the calculus approach to variable acceleration.
This page complements the core kinematics notes. Readers should already be comfortable with the
SUVAT equations and basic calculus definitions of velocity and acceleration.
1. Equations of Motion (SUVAT) -- Rigorous Derivation
1.1 Derivation from first principles
Starting from the definition of constant acceleration:
a = d v d t a = \frac{dv}{dt} a = d t d v
Integrating with respect to t t t :
∫ 0 t a d t = ∫ u v d v ⟹ a t = v − u ⟹ v = u + a t \int_0^t a\,dt = \int_u^v dv \implies at = v - u \implies v = u + at ∫ 0 t a d t = ∫ u v d v ⟹ a t = v − u ⟹ v = u + a t
This is SUVAT equation 1 . We now derive the remaining four.
Equation 2: s = u t + 1 2 a t 2 s = ut + \tfrac{1}{2}at^2 s = u t + 2 1 a t 2
Since v = d s d t = u + a t v = \dfrac{ds}{dt} = u + at v = d t d s = u + a t , integrate:
∫ 0 s d s = ∫ 0 t ( u + a t ) d t ⟹ s = u t + 1 2 a t 2 \int_0^s ds = \int_0^t (u + at)\,dt \implies s = ut + \frac{1}{2}at^2 ∫ 0 s d s = ∫ 0 t ( u + a t ) d t ⟹ s = u t + 2 1 a t 2
Equation 3: s = 1 2 ( u + v ) t s = \dfrac{1}{2}(u + v)t s = 2 1 ( u + v ) t
Substitute v = u + a t v = u + at v = u + a t into Equation 2:
s = u t + 1 2 ( v − u ) t = 1 2 ( 2 u + v − u ) t = 1 2 ( u + v ) t s = ut + \frac{1}{2}(v - u)t = \frac{1}{2}(2u + v - u)t = \frac{1}{2}(u + v)t s = u t + 2 1 ( v − u ) t = 2 1 ( 2 u + v − u ) t = 2 1 ( u + v ) t
Equation 4: v 2 = u 2 + 2 a s v^2 = u^2 + 2as v 2 = u 2 + 2 a s
From v = u + a t v = u + at v = u + a t , square both sides:
v 2 = ( u + a t ) 2 = u 2 + 2 u a t + a 2 t 2 v^2 = (u + at)^2 = u^2 + 2uat + a^2t^2 v 2 = ( u + a t ) 2 = u 2 + 2 u a t + a 2 t 2
Factor 2 a 2a 2 a from the last two terms:
v 2 = u 2 + 2 a ( u t + 1 2 a t 2 ) = u 2 + 2 a s v^2 = u^2 + 2a\!\left(ut + \frac{1}{2}at^2\right) = u^2 + 2as v 2 = u 2 + 2 a ( u t + 2 1 a t 2 ) = u 2 + 2 a s
Equation 5: s = v t − 1 2 a t 2 s = vt - \tfrac{1}{2}at^2 s = v t − 2 1 a t 2
Substitute u = v − a t u = v - at u = v − a t into Equation 2:
s = ( v − a t ) t + 1 2 a t 2 = v t − 1 2 a t 2 s = (v - at)t + \frac{1}{2}at^2 = vt - \frac{1}{2}at^2 s = ( v − a t ) t + 2 1 a t 2 = v t − 2 1 a t 2
1.2 Selecting the correct equation
The key skill is identifying which variable is unknown and which is not needed :
Unknown Do not use displacement s s s v 2 = u 2 + 2 a s v^2 = u^2 + 2as v 2 = u 2 + 2 a s final velocity v v v s = 1 2 ( u + v ) t s = \tfrac{1}{2}(u+v)t s = 2 1 ( u + v ) t time t t t v 2 = u 2 + 2 a s v^2 = u^2 + 2as v 2 = u 2 + 2 a s acceleration a a a s = 1 2 ( u + v ) t s = \tfrac{1}{2}(u+v)t s = 2 1 ( u + v ) t initial velocity u u u s = v t − 1 2 a t 2 s = vt - \tfrac{1}{2}at^2 s = v t − 2 1 a t 2
1.3 Worked example: multi-stage motion
Problem. A car accelerates uniformly from rest at 2 m s − 2 2\;\mathrm{m\,s^{-2}} 2 m s − 2 for 6 seconds, then
decelerates uniformly at 3 m s − 2 3\;\mathrm{m\,s^{-2}} 3 m s − 2 until it comes to rest. Find the total distance
travelled.
Stage 1: Acceleration.
v = u + a t = 0 + 2 × 6 = 12 m s − 1 v = u + at = 0 + 2 \times 6 = 12\;\mathrm{m\,s^{-1}} v = u + a t = 0 + 2 × 6 = 12 m s − 1
s 1 = u t + 1 2 a t 2 = 0 + 1 2 ( 2 ) ( 36 ) = 36 m s_1 = ut + \frac{1}{2}at^2 = 0 + \frac{1}{2}(2)(36) = 36\;\mathrm{m} s 1 = u t + 2 1 a t 2 = 0 + 2 1 ( 2 ) ( 36 ) = 36 m
Stage 2: Deceleration. Now u = 12 u = 12 u = 12 , v = 0 v = 0 v = 0 , a = − 3 a = -3 a = − 3 .
t 2 = v − u a = 0 − 12 − 3 = 4 s t_2 = \frac{v - u}{a} = \frac{0 - 12}{-3} = 4\;\mathrm{s} t 2 = a v − u = − 3 0 − 12 = 4 s
s 2 = 1 2 ( u + v ) t 2 = 1 2 ( 12 + 0 ) ( 4 ) = 24 m s_2 = \frac{1}{2}(u + v)t_2 = \frac{1}{2}(12 + 0)(4) = 24\;\mathrm{m} s 2 = 2 1 ( u + v ) t 2 = 2 1 ( 12 + 0 ) ( 4 ) = 24 m
s t o t a l = 36 + 24 = 60 m s_{\mathrm{total}} = 36 + 24 = 60\;\mathrm{m} s total = 36 + 24 = 60 m
Common Pitfall
When a problem has multiple stages, the final velocity of one stage becomes the initial velocity
of the next . Forgetting this connection is the most frequent error in multi-stage kinematics
problems.
2. Free Fall Under Gravity
2.1 The acceleration due to gravity
Near the Earth's surface, all objects in free fall (neglecting air resistance) experience the same
acceleration g g g . The standard value is:
g ≈ 9.8 m s − 2 ( o r 9.81 m s − 2 f o r g r e a t e r p r e c i s i o n ) g \approx 9.8\;\mathrm{m\,s^{-2}} \quad (\mathrm{or}\ 9.81\;\mathrm{m\,s^{-2}}\ \mathrm{for\ greater\ precision}) g ≈ 9.8 m s − 2 ( or 9.81 m s − 2 for greater precision )
The direction of g g g is always downward . The sign convention must be established at the start
of every problem.
2.2 Sign conventions
Convention A (upward positive): Displacement upward is positive, so a = − g a = -g a = − g .
Convention B (downward positive): Displacement downward is positive, so a = + g a = +g a = + g .
Both conventions are valid, but you must be consistent throughout a single problem.
2.3 Worked example: object thrown upward
Problem. A ball is thrown vertically upward at 15 m s − 1 15\;\mathrm{m\,s^{-1}} 15 m s − 1 from a height of
2 m 2\;\mathrm{m} 2 m above the ground. Taking g = 9.8 m s − 2 g = 9.8\;\mathrm{m\,s^{-2}} g = 9.8 m s − 2 and upward as positive, find
the speed with which it hits the ground.
At the highest point, v = 0 v = 0 v = 0 :
t m a x = v − u a = 0 − 15 − 9.8 = 15 9.8 ≈ 1.531 s t_{\mathrm{max}} = \frac{v - u}{a} = \frac{0 - 15}{-9.8} = \frac{15}{9.8} \approx 1.531\;\mathrm{s} t max = a v − u = − 9.8 0 − 15 = 9.8 15 ≈ 1.531 s
Maximum height above the throw point:
s u p = v 2 − u 2 2 a = 0 − 225 2 ( − 9.8 ) = 225 19.6 ≈ 11.48 m s_{\mathrm{up}} = \frac{v^2 - u^2}{2a} = \frac{0 - 225}{2(-9.8)} = \frac{225}{19.6} \approx 11.48\;\mathrm{m} s up = 2 a v 2 − u 2 = 2 ( − 9.8 ) 0 − 225 = 19.6 225 ≈ 11.48 m
Total height above ground: 11.48 + 2 = 13.48 m 11.48 + 2 = 13.48\;\mathrm{m} 11.48 + 2 = 13.48 m .
On the way down: u = 0 u = 0 u = 0 , a = − 9.8 a = -9.8 a = − 9.8 (still upward positive), s = − 13.48 m s = -13.48\;\mathrm{m} s = − 13.48 m .
v 2 = 0 + 2 ( − 9.8 ) ( − 13.48 ) = 264.21 v^2 = 0 + 2(-9.8)(-13.48) = 264.21 v 2 = 0 + 2 ( − 9.8 ) ( − 13.48 ) = 264.21
v = − 264.21 ≈ − 16.26 m s − 1 v = -\sqrt{264.21} \approx -16.26\;\mathrm{m\,s^{-1}} v = − 264.21 ≈ − 16.26 m s − 1
The negative sign confirms downward motion. Speed = 16.3 m s − 1 = 16.3\;\mathrm{m\,s^{-1}} = 16.3 m s − 1 (3 s.f.).
Note that the total time of flight can also be found directly: s = − 2 s = -2 s = − 2 , u = 15 u = 15 u = 15 , a = − 9.8 a = -9.8 a = − 9.8 :
− 2 = 15 t − 4.9 t 2 -2 = 15t - 4.9t^2 − 2 = 15 t − 4.9 t 2 , giving t ≈ 3.15 s t \approx 3.15\;\mathrm{s} t ≈ 3.15 s . This is not 2 × t m a x 2 \times t_{\mathrm{max}} 2 × t max
because the ball was thrown from a height, not from ground level.
3. Projectile Motion
3.1 Resolving into horizontal and vertical components
For a projectile launched with speed u u u at angle θ \theta θ above the horizontal:
u x = u cos θ , u y = u sin θ u_x = u\cos\theta, \qquad u_y = u\sin\theta u x = u cos θ , u y = u sin θ
The key principle is that horizontal and vertical motion are independent :
Horizontal: constant velocity (no acceleration, neglecting air resistance).
Vertical: uniform acceleration g g g downward.
3.2 Position as a function of time
Taking the launch point as the origin, with upward as positive:
x = u\cos\theta \cdot t \tag{horizontal}
y = u\sin\theta \cdot t - \frac{1}{2}gt^2 \tag{vertical}
3.3 The trajectory equation
Eliminating t t t from the parametric equations:
t = ◆ L B ◆ x ◆ R B ◆◆ L B ◆ u cos θ ◆ R B ◆ t = \frac◆LB◆x◆RB◆◆LB◆u\cos\theta◆RB◆ t = L ◆ B ◆ x ◆ R B ◆◆ L B ◆ u cos θ ◆ R B ◆
y = u sin θ ⋅ ◆ L B ◆ x ◆ R B ◆◆ L B ◆ u cos θ ◆ R B ◆ − 1 2 g ( ◆ L B ◆ x ◆ R B ◆◆ L B ◆ u cos θ ◆ R B ◆ ) 2 y = u\sin\theta \cdot \frac◆LB◆x◆RB◆◆LB◆u\cos\theta◆RB◆ - \frac{1}{2}g\!\left(\frac◆LB◆x◆RB◆◆LB◆u\cos\theta◆RB◆\right)^{\!2} y = u sin θ ⋅ L ◆ B ◆ x ◆ R B ◆◆ L B ◆ u cos θ ◆ R B ◆ − 2 1 g ( L ◆ B ◆ x ◆ R B ◆◆ L B ◆ u cos θ ◆ R B ◆ ) 2
y = x tan θ − ◆ L B ◆ g x 2 ◆ R B ◆◆ L B ◆ 2 u 2 cos 2 θ ◆ R B ◆ \boxed{y = x\tan\theta - \frac◆LB◆gx^2◆RB◆◆LB◆2u^2\cos^2\theta◆RB◆} y = x tan θ − L ◆ B ◆ g x 2 ◆ R B ◆◆ L B ◆2 u 2 cos 2 θ ◆ R B ◆
This is the equation of a parabola , confirming that the trajectory of a projectile (under
constant gravity with no air resistance) is parabolic.
3.4 Key results
Time of flight (landing at the same height): Setting y = 0 y = 0 y = 0 :
t = ◆ L B ◆ 2 u sin θ ◆ R B ◆◆ L B ◆ g ◆ R B ◆ t = \frac◆LB◆2u\sin\theta◆RB◆◆LB◆g◆RB◆ t = L ◆ B ◆2 u sin θ ◆ R B ◆◆ L B ◆ g ◆ R B ◆
Maximum height:
H = ◆ L B ◆ u 2 sin 2 θ ◆ R B ◆◆ L B ◆ 2 g ◆ R B ◆ H = \frac◆LB◆u^2\sin^2\theta◆RB◆◆LB◆2g◆RB◆ H = L ◆ B ◆ u 2 sin 2 θ ◆ R B ◆◆ L B ◆2 g ◆ R B ◆
Range:
R = ◆ L B ◆ u 2 sin 2 θ ◆ R B ◆◆ L B ◆ g ◆ R B ◆ R = \frac◆LB◆u^2\sin 2\theta◆RB◆◆LB◆g◆RB◆ R = L ◆ B ◆ u 2 sin 2 θ ◆ R B ◆◆ L B ◆ g ◆ R B ◆
Maximum range occurs when sin 2 θ = 1 \sin 2\theta = 1 sin 2 θ = 1 , i.e. θ = 45 ∘ \theta = 45^\circ θ = 4 5 ∘ , giving R max = u 2 g R_{\max} = \dfrac{u^2}{g} R m a x = g u 2 .
3.5 Proof that complementary angles give the same range
If θ 1 + θ 2 = 90 ∘ \theta_1 + \theta_2 = 90^\circ θ 1 + θ 2 = 9 0 ∘ , then sin 2 θ 1 = sin ( 180 ∘ − 2 θ 2 ) = sin 2 θ 2 \sin 2\theta_1 = \sin(180^\circ - 2\theta_2) = \sin 2\theta_2 sin 2 θ 1 = sin ( 18 0 ∘ − 2 θ 2 ) = sin 2 θ 2 .
Therefore R ( θ 1 ) = R ( θ 2 ) R(\theta_1) = R(\theta_2) R ( θ 1 ) = R ( θ 2 ) .
3.6 Worked example
Problem. A cricketer hits a ball at 25 m s − 1 25\;\mathrm{m\,s^{-1}} 25 m s − 1 at 35 ∘ 35^\circ 3 5 ∘ above the horizontal
from a height of 1.5 m 1.5\;\mathrm{m} 1.5 m . Taking g = 9.8 m s − 2 g = 9.8\;\mathrm{m\,s^{-2}} g = 9.8 m s − 2 , find the horizontal distance
travelled before the ball hits the ground.
u x = 25 cos 35 ∘ ≈ 20.48 m s − 1 u_x = 25\cos 35^\circ \approx 20.48\;\mathrm{m\,s^{-1}} u x = 25 cos 3 5 ∘ ≈ 20.48 m s − 1
u y = 25 sin 35 ∘ ≈ 14.34 m s − 1 u_y = 25\sin 35^\circ \approx 14.34\;\mathrm{m\,s^{-1}} u y = 25 sin 3 5 ∘ ≈ 14.34 m s − 1
When the ball hits the ground, y = − 1.5 m y = -1.5\;\mathrm{m} y = − 1.5 m :
− 1.5 = 14.34 t − 4.9 t 2 -1.5 = 14.34t - 4.9t^2 − 1.5 = 14.34 t − 4.9 t 2
4.9 t 2 − 14.34 t − 1.5 = 0 4.9t^2 - 14.34t - 1.5 = 0 4.9 t 2 − 14.34 t − 1.5 = 0
t = ◆ L B ◆ 14.34 ± 14.34 2 + 4 ( 4.9 ) ( 1.5 ) ◆ R B ◆◆ L B ◆ 2 ( 4.9 ) ◆ R B ◆ = ◆ L B ◆ 14.34 ± 205.64 + 29.4 ◆ R B ◆◆ L B ◆ 9.8 ◆ R B ◆ t = \frac◆LB◆14.34 \pm \sqrt{14.34^2 + 4(4.9)(1.5)}◆RB◆◆LB◆2(4.9)◆RB◆ = \frac◆LB◆14.34 \pm \sqrt{205.64 + 29.4}◆RB◆◆LB◆9.8◆RB◆ t = L ◆ B ◆14.34 ± 14.3 4 2 + 4 ( 4.9 ) ( 1.5 ) ◆ R B ◆◆ L B ◆2 ( 4.9 ) ◆ R B ◆ = L ◆ B ◆14.34 ± 205.64 + 29.4 ◆ R B ◆◆ L B ◆9.8◆ R B ◆
t = 14.34 + 15.38 9.8 ≈ 3.025 s ( t a k i n g t h e p o s i t i v e r o o t ) t = \frac{14.34 + 15.38}{9.8} \approx 3.025\;\mathrm{s} \quad (\mathrm{taking\ the\ positive\ root}) t = 9.8 14.34 + 15.38 ≈ 3.025 s ( taking the positive root )
x = 20.48 × 3.025 ≈ 61.95 m x = 20.48 \times 3.025 \approx 61.95\;\mathrm{m} x = 20.48 × 3.025 ≈ 61.95 m
The ball travels approximately 62.0 m 62.0\;\mathrm{m} 62.0 m horizontally.
warning
When a projectile is launched from a height above the landing level, the trajectory is not
symmetric. The time of ascent is less than the time of descent, and the landing angle is steeper
than the launch angle.
4. Two-Dimensional Motion with Non-Perpendicular Components
4.1 Resolving along arbitrary directions
Sometimes it is convenient to resolve velocity or acceleration along non-horizontal/vertical
directions, such as parallel and perpendicular to an inclined plane.
For an inclined plane at angle α \alpha α to the horizontal:
Parallel to the plane: a ∥ = g sin α a_{\parallel} = g\sin\alpha a ∥ = g sin α (down the plane)
Perpendicular to the plane: a ⊥ = g cos α a_{\perp} = g\cos\alpha a ⊥ = g cos α (into the plane)
4.2 Worked example: projectile on an inclined plane
Problem. A particle is projected up a plane inclined at 30 ∘ 30^\circ 3 0 ∘ to the horizontal with
speed 20 m s − 1 20\;\mathrm{m\,s^{-1}} 20 m s − 1 at an angle of 50 ∘ 50^\circ 5 0 ∘ to the horizontal. Taking g = 9.8 m s − 1 g = 9.8\;\mathrm{m\,s^{-1}} g = 9.8 m s − 1 ,
find the distance travelled up the plane before the particle lands on it.
Resolve parallel and perpendicular to the plane. The angle of projection relative to the plane is
50 ∘ − 30 ∘ = 20 ∘ 50^\circ - 30^\circ = 20^\circ 5 0 ∘ − 3 0 ∘ = 2 0 ∘ .
Parallel to plane: u ∥ = 20 cos 20 ∘ ≈ 18.79 m s − 1 u_{\parallel} = 20\cos 20^\circ \approx 18.79\;\mathrm{m\,s^{-1}} u ∥ = 20 cos 2 0 ∘ ≈ 18.79 m s − 1
a ∥ = − g sin 30 ∘ = − 4.9 m s − 2 a_{\parallel} = -g\sin 30^\circ = -4.9\;\mathrm{m\,s^{-2}} a ∥ = − g sin 3 0 ∘ = − 4.9 m s − 2
Perpendicular to plane: u ⊥ = 20 sin 20 ∘ ≈ 6.84 m s − 1 u_{\perp} = 20\sin 20^\circ \approx 6.84\;\mathrm{m\,s^{-1}} u ⊥ = 20 sin 2 0 ∘ ≈ 6.84 m s − 1
a ⊥ = − g cos 30 ∘ = − 8.49 m s − 2 a_{\perp} = -g\cos 30^\circ = -8.49\;\mathrm{m\,s^{-2}} a ⊥ = − g cos 3 0 ∘ = − 8.49 m s − 2
Time of flight: the particle lands when its perpendicular displacement returns to zero.
s ⊥ = u ⊥ t + 1 2 a ⊥ t 2 = 0 s_{\perp} = u_{\perp}t + \tfrac{1}{2}a_{\perp}t^2 = 0 s ⊥ = u ⊥ t + 2 1 a ⊥ t 2 = 0
t ( 6.84 − 4.245 t ) = 0 ⟹ t = 6.84 4.245 ≈ 1.611 s t\!\left(6.84 - 4.245t\right) = 0 \implies t = \frac{6.84}{4.245} \approx 1.611\;\mathrm{s} t ( 6.84 − 4.245 t ) = 0 ⟹ t = 4.245 6.84 ≈ 1.611 s
Distance up the plane:
s ∥ = 18.79 ( 1.611 ) + 1 2 ( − 4.9 ) ( 1.611 ) 2 = 30.27 − 6.36 ≈ 23.9 m s_{\parallel} = 18.79(1.611) + \tfrac{1}{2}(-4.9)(1.611)^2 = 30.27 - 6.36 \approx 23.9\;\mathrm{m} s ∥ = 18.79 ( 1.611 ) + 2 1 ( − 4.9 ) ( 1.611 ) 2 = 30.27 − 6.36 ≈ 23.9 m
5. Variable Acceleration
5.1 Using calculus for non-constant acceleration
When acceleration is not constant, the SUVAT equations do not apply. Instead, we use the calculus
relationships:
v = d s d t , a = d v d t = d 2 s d t 2 = v d v d s v = \frac{ds}{dt}, \qquad a = \frac{dv}{dt} = \frac{d^2s}{dt^2} = v\frac{dv}{ds} v = d t d s , a = d t d v = d t 2 d 2 s = v d s d v
s = ∫ v d t , v = ∫ a d t s = \int v\,dt, \qquad v = \int a\,dt s = ∫ v d t , v = ∫ a d t
The chain rule form a = v d v d s a = v\,\dfrac{dv}{ds} a = v d s d v is particularly useful when acceleration is given as a
function of displacement rather than time.
5.2 Derivation of a = v d v d s a = v\,\dfrac{dv}{ds} a = v d s d v
By the chain rule:
a = d v d t = d v d s ⋅ d s d t = d v d s ⋅ v a = \frac{dv}{dt} = \frac{dv}{ds} \cdot \frac{ds}{dt} = \frac{dv}{ds} \cdot v a = d t d v = d s d v ⋅ d t d s = d s d v ⋅ v
This allows us to solve problems where a = f ( s ) a = f(s) a = f ( s ) by separating variables:
v d v = a d s ⟹ ∫ v d v = ∫ a d s ⟹ 1 2 v 2 = ∫ a d s + C v\,dv = a\,ds \implies \int v\,dv = \int a\,ds \implies \frac{1}{2}v^2 = \int a\,ds + C v d v = a d s ⟹ ∫ v d v = ∫ a d s ⟹ 2 1 v 2 = ∫ a d s + C
5.3 Worked example: a = f ( t ) a = f(t) a = f ( t )
Problem. A particle moves in a straight line with acceleration a = 6 t − 2 t 2 m s − 2 a = 6t - 2t^2\;\mathrm{m\,s^{-2}} a = 6 t − 2 t 2 m s − 2 .
At t = 0 t = 0 t = 0 , v = 3 m s − 1 v = 3\;\mathrm{m\,s^{-1}} v = 3 m s − 1 and s = 0 s = 0 s = 0 . Find the distance travelled in the first
4 4 4 seconds.
v = ∫ ( 6 t − 2 t 2 ) d t = 3 t 2 − 2 3 t 3 + C v = \int (6t - 2t^2)\,dt = 3t^2 - \frac{2}{3}t^3 + C v = ∫ ( 6 t − 2 t 2 ) d t = 3 t 2 − 3 2 t 3 + C
When t = 0 t = 0 t = 0 , v = 3 v = 3 v = 3 : C = 3 C = 3 C = 3 .
v = 3 t 2 − 2 3 t 3 + 3 v = 3t^2 - \frac{2}{3}t^3 + 3 v = 3 t 2 − 3 2 t 3 + 3
Check if the particle changes direction (i.e. v = 0 v = 0 v = 0 ):
3 t 2 − 2 3 t 3 + 3 = 0 ⟹ 9 t 2 − 2 t 3 + 9 = 0 3t^2 - \frac{2}{3}t^3 + 3 = 0 \implies 9t^2 - 2t^3 + 9 = 0 3 t 2 − 3 2 t 3 + 3 = 0 ⟹ 9 t 2 − 2 t 3 + 9 = 0
By inspection or numerical methods, v > 0 v \gt 0 v > 0 for all t ≥ 0 t \geq 0 t ≥ 0 (since 9 t 2 + 9 > 2 t 3 9t^2 + 9 \gt 2t^3 9 t 2 + 9 > 2 t 3 for
0 ≤ t ≤ 4 0 \leq t \leq 4 0 ≤ t ≤ 4 ).
s = ∫ 0 4 ( 3 t 2 − 2 3 t 3 + 3 ) d t = [ t 3 − 1 6 t 4 + 3 t ] 0 4 s = \int_0^4 \!\left(3t^2 - \frac{2}{3}t^3 + 3\right)dt = \left[t^3 - \frac{1}{6}t^4 + 3t\right]_0^4 s = ∫ 0 4 ( 3 t 2 − 3 2 t 3 + 3 ) d t = [ t 3 − 6 1 t 4 + 3 t ] 0 4
s = 64 − 256 6 + 12 = 64 − 42.67 + 12 = 33.33 m s = 64 - \frac{256}{6} + 12 = 64 - 42.67 + 12 = 33.33\;\mathrm{m} s = 64 − 6 256 + 12 = 64 − 42.67 + 12 = 33.33 m
5.4 Worked example: a = f ( v ) a = f(v) a = f ( v )
Problem. A particle moves with acceleration a = − 0.1 v 2 m s − 2 a = -0.1v^2\;\mathrm{m\,s^{-2}} a = − 0.1 v 2 m s − 2 . Initially
v = 10 m s − 1 v = 10\;\mathrm{m\,s^{-1}} v = 10 m s − 1 . Find an expression for v v v in terms of t t t .
Since a = d v d t a = \dfrac{dv}{dt} a = d t d v :
d v d t = − 0.1 v 2 \frac{dv}{dt} = -0.1v^2 d t d v = − 0.1 v 2
Separating variables:
∫ 1 v 2 d v = ∫ − 0.1 d t \int \frac{1}{v^2}\,dv = \int -0.1\,dt ∫ v 2 1 d v = ∫ − 0.1 d t
− 1 v = − 0.1 t + C -\frac{1}{v} = -0.1t + C − v 1 = − 0.1 t + C
When t = 0 t = 0 t = 0 , v = 10 v = 10 v = 10 : − 1 10 = C -\dfrac{1}{10} = C − 10 1 = C .
− 1 v = − 0.1 t − 1 10 -\frac{1}{v} = -0.1t - \frac{1}{10} − v 1 = − 0.1 t − 10 1
1 v = 0.1 t + 0.1 = 0.1 ( t + 1 ) \frac{1}{v} = 0.1t + 0.1 = 0.1(t + 1) v 1 = 0.1 t + 0.1 = 0.1 ( t + 1 )
v = 10 t + 1 m s − 1 v = \frac{10}{t + 1}\;\mathrm{m\,s^{-1}} v = t + 1 10 m s − 1
warning
For variable acceleration problems, always include the constant of integration and use the
initial conditions to find it. Also check whether the particle changes direction by finding when
v = 0 v = 0 v = 0 -- the total distance is not the same as the displacement if there is a change of
direction.
6. Practice Problems
Problem 1
A train decelerates uniformly from 40 m s − 1 40\;\mathrm{m\,s^{-1}} 40 m s − 1 to rest over a distance of 800 m 800\;\mathrm{m} 800 m .
Find the deceleration and the time taken.
Solution Using v 2 = u 2 + 2 a s v^2 = u^2 + 2as v 2 = u 2 + 2 a s :
0 = 1600 + 2 a ( 800 ) ⟹ a = − 1 m s − 2 0 = 1600 + 2a(800) \implies a = -1\;\mathrm{m\,s^{-2}} 0 = 1600 + 2 a ( 800 ) ⟹ a = − 1 m s − 2
t = v − u a = − 40 − 1 = 40 s t = \frac{v - u}{a} = \frac{-40}{-1} = 40\;\mathrm{s} t = a v − u = − 1 − 40 = 40 s
Problem 2
A projectile is launched from ground level at 30 m s − 1 30\;\mathrm{m\,s^{-1}} 30 m s − 1 at 60 ∘ 60^\circ 6 0 ∘ to the horizontal.
Taking g = 9.8 m s − 2 g = 9.8\;\mathrm{m\,s^{-2}} g = 9.8 m s − 2 , find the maximum height and the range.
Solution H = ◆ L B ◆ u 2 sin 2 θ ◆ R B ◆◆ L B ◆ 2 g ◆ R B ◆ = ◆ L B ◆ 900 × 0.75 ◆ R B ◆◆ L B ◆ 19.6 ◆ R B ◆ = 675 19.6 ≈ 34.4 m H = \frac◆LB◆u^2\sin^2\theta◆RB◆◆LB◆2g◆RB◆ = \frac◆LB◆900 \times 0.75◆RB◆◆LB◆19.6◆RB◆ = \frac{675}{19.6} \approx 34.4\;\mathrm{m} H = L ◆ B ◆ u 2 sin 2 θ ◆ R B ◆◆ L B ◆2 g ◆ R B ◆ = L ◆ B ◆900 × 0.75◆ R B ◆◆ L B ◆19.6◆ R B ◆ = 19.6 675 ≈ 34.4 m
R = ◆ L B ◆ u 2 sin 2 θ ◆ R B ◆◆ L B ◆ g ◆ R B ◆ = ◆ L B ◆ 900 × sin 120 ∘ ◆ R B ◆◆ L B ◆ 9.8 ◆ R B ◆ = ◆ L B ◆ 900 × 0.866 ◆ R B ◆◆ L B ◆ 9.8 ◆ R B ◆ ≈ 79.6 m R = \frac◆LB◆u^2\sin 2\theta◆RB◆◆LB◆g◆RB◆ = \frac◆LB◆900 \times \sin 120^\circ◆RB◆◆LB◆9.8◆RB◆ = \frac◆LB◆900 \times 0.866◆RB◆◆LB◆9.8◆RB◆ \approx 79.6\;\mathrm{m} R = L ◆ B ◆ u 2 sin 2 θ ◆ R B ◆◆ L B ◆ g ◆ R B ◆ = L ◆ B ◆900 × sin 12 0 ∘ ◆ R B ◆◆ L B ◆9.8◆ R B ◆ = L ◆ B ◆900 × 0.866◆ R B ◆◆ L B ◆9.8◆ R B ◆ ≈ 79.6 m
Problem 3
A particle moves with acceleration a = 12 t m s − 2 a = 12t\;\mathrm{m\,s^{-2}} a = 12 t m s − 2 . At t = 0 t = 0 t = 0 , it is at rest at the
origin. Find its displacement when t = 3 s t = 3\;\mathrm{s} t = 3 s .
Solution v = ∫ 12 t d t = 6 t 2 + C 1 v = \int 12t\,dt = 6t^2 + C_1 v = ∫ 12 t d t = 6 t 2 + C 1
When t = 0 t = 0 t = 0 , v = 0 v = 0 v = 0 : C 1 = 0 C_1 = 0 C 1 = 0 , so v = 6 t 2 v = 6t^2 v = 6 t 2 .
s = ∫ 6 t 2 d t = 2 t 3 + C 2 s = \int 6t^2\,dt = 2t^3 + C_2 s = ∫ 6 t 2 d t = 2 t 3 + C 2
When t = 0 t = 0 t = 0 , s = 0 s = 0 s = 0 : C 2 = 0 C_2 = 0 C 2 = 0 , so s = 2 t 3 s = 2t^3 s = 2 t 3 .
At t = 3 t = 3 t = 3 : s = 2 ( 27 ) = 54 m s = 2(27) = 54\;\mathrm{m} s = 2 ( 27 ) = 54 m .
Problem 4
A stone is thrown horizontally at 8 m s − 1 8\;\mathrm{m\,s^{-1}} 8 m s − 1 from the top of a cliff 60 m 60\;\mathrm{m} 60 m high.
Taking g = 9.8 m s − 2 g = 9.8\;\mathrm{m\,s^{-2}} g = 9.8 m s − 2 , find the horizontal distance from the base of the cliff where the
stone lands, and the velocity (magnitude and direction) at impact.
Solution Vertical: s = − 60 s = -60 s = − 60 , u y = 0 u_y = 0 u y = 0 , a = − 9.8 a = -9.8 a = − 9.8 .
− 60 = 0 − 1 2 ( 9.8 ) t 2 ⟹ t = ◆ L B ◆ 120 9.8 ◆ R B ◆ ≈ 3.50 s -60 = 0 - \frac{1}{2}(9.8)t^2 \implies t = \sqrt◆LB◆\frac{120}{9.8}◆RB◆ \approx 3.50\;\mathrm{s} − 60 = 0 − 2 1 ( 9.8 ) t 2 ⟹ t = ◆ L B ◆ 9.8 120 ◆ R B ◆ ≈ 3.50 s
Horizontal: x = 8 × 3.50 = 28.0 m x = 8 \times 3.50 = 28.0\;\mathrm{m} x = 8 × 3.50 = 28.0 m .
At impact: v y = − 9.8 × 3.50 = − 34.3 m s − 1 v_y = -9.8 \times 3.50 = -34.3\;\mathrm{m\,s^{-1}} v y = − 9.8 × 3.50 = − 34.3 m s − 1 , v x = 8 m s − 1 v_x = 8\;\mathrm{m\,s^{-1}} v x = 8 m s − 1 .
∣ v ∣ = 8 2 + 34.3 2 = 64 + 1176.5 ≈ 35.2 m s − 1 |\mathbf{v}| = \sqrt{8^2 + 34.3^2} = \sqrt{64 + 1176.5} \approx 35.2\;\mathrm{m\,s^{-1}} ∣ v ∣ = 8 2 + 34. 3 2 = 64 + 1176.5 ≈ 35.2 m s − 1
Angle below horizontal: θ = arctan ( 34.3 8 ) ≈ 76.9 ∘ \theta = \arctan\!\left(\dfrac{34.3}{8}\right) \approx 76.9^\circ θ = arctan ( 8 34.3 ) ≈ 76. 9 ∘ .
Problem 5
A particle moves in a straight line so that its acceleration is given by a = 4 − 2 s m s − 2 a = 4 - 2s\;\mathrm{m\,s^{-2}} a = 4 − 2 s m s − 2 ,
where s s s is the displacement from a fixed point. When s = 0 s = 0 s = 0 , v = 2 m s − 1 v = 2\;\mathrm{m\,s^{-1}} v = 2 m s − 1 . Find the
maximum displacement.
Solution Using a = v d v d s a = v\,\dfrac{dv}{ds} a = v d s d v :
v d v d s = 4 − 2 s v\,\frac{dv}{ds} = 4 - 2s v d s d v = 4 − 2 s
Integrating:
∫ v d v = ∫ ( 4 − 2 s ) d s \int v\,dv = \int (4 - 2s)\,ds ∫ v d v = ∫ ( 4 − 2 s ) d s
1 2 v 2 = 4 s − s 2 + C \frac{1}{2}v^2 = 4s - s^2 + C 2 1 v 2 = 4 s − s 2 + C
When s = 0 s = 0 s = 0 , v = 2 v = 2 v = 2 : 1 2 ( 4 ) = 0 + C ⟹ C = 2 \dfrac{1}{2}(4) = 0 + C \implies C = 2 2 1 ( 4 ) = 0 + C ⟹ C = 2 .
1 2 v 2 = 4 s − s 2 + 2 \frac{1}{2}v^2 = 4s - s^2 + 2 2 1 v 2 = 4 s − s 2 + 2
Maximum displacement when v = 0 v = 0 v = 0 :
0 = 4 s − s 2 + 2 ⟹ s 2 − 4 s − 2 = 0 0 = 4s - s^2 + 2 \implies s^2 - 4s - 2 = 0 0 = 4 s − s 2 + 2 ⟹ s 2 − 4 s − 2 = 0
s = ◆ L B ◆ 4 ± 16 + 8 ◆ R B ◆◆ L B ◆ 2 ◆ R B ◆ = ◆ L B ◆ 4 ± 24 ◆ R B ◆◆ L B ◆ 2 ◆ R B ◆ = 2 ± 6 s = \frac◆LB◆4 \pm \sqrt{16 + 8}◆RB◆◆LB◆2◆RB◆ = \frac◆LB◆4 \pm \sqrt{24}◆RB◆◆LB◆2◆RB◆ = 2 \pm \sqrt{6} s = L ◆ B ◆4 ± 16 + 8 ◆ R B ◆◆ L B ◆2◆ R B ◆ = L ◆ B ◆4 ± 24 ◆ R B ◆◆ L B ◆2◆ R B ◆ = 2 ± 6
Taking the positive root: s max = 2 + 6 ≈ 4.45 m s_{\max} = 2 + \sqrt{6} \approx 4.45\;\mathrm{m} s m a x = 2 + 6 ≈ 4.45 m .