Curved motion
-
Upload
scienceeducationexpert -
Category
Education
-
view
149 -
download
5
description
Transcript of Curved motion
Curved motion
Overview
Curved motion 2
The trajectory and velocity of an object is fully determined byβ¦ 1. Its initial place π 02. Its initial velocity π£0
3. The present overall force field Ξ£ πΉ
π£0
π 0
Ξ£ πΉ π£0
π£0
π 0 Ξ£ πΉ
π£0
π 0
Ξ£ πΉ
Uniform Ξ£ πΉ ON thesame working line as π£0
= Linear motion
Uniform Ξ£ πΉ NOT ON thesame working line as π£0
= Projectile motion
Ξ£ πΉ always directed to ONEsingle point + constant π£ .= Circular motion
Velocity change β π£ as a vector
Curved motion 3
π£0
Ξ£ πΉ
π£0
π£0
Ξ£ πΉ
π£0
Ξ£ πΉ
Ξ π£ = πΞπ‘ =1
πΞ£ πΉΞπ‘ The velocity always changes in the direction of the overall force
Ξ π£
π£1
Ξ π£
π£1
π£1
π£2
Ξ π£
Ξ π£
Ξ π£
π£1
Verify in the pictures that always β π£ ββ Ξ£ πΉ
Difficult because Ξ£ πΉchanges direction
during Ξπ‘So Ξπ‘ must be small
Projectile (ballistic) motion
Curved motion 4
π£0
β1β0
π£1
π£2
πΉπ
Range
Trajectory
Assumption: Ξ£ πΉ = πΉπ (only uniform downwards weight, no air resistance)
Projectile motion, scalar treatment - I
Curved motion 5
π£0
β1β0
π£1
π£2
πΉπ
Use the energy conservation law πΈ0 = πΈ1 = πΈ2
Range
Trajectory
πΈπ0 + πΈπ0 = πΈπ1 + πΈπ1 β1
2ππ£0
2 + ππβ0 =1
2ππ£1
2 + ππβ1 β1
2π£0
2 + πβ0 =1
2π£1
2 + πβ1
To calculate the maximum height, apply πΈ0 = πΈ1
4 unknowns, so 3 must be known
Projectile motion, scalar treatment - II
Curved motion 6
π£0
β1β0
π£1
π£2
πΉπ
Range
Trajectory
πΈπ0 + πΈπ0 = πΈπ2 + πΈπ2 β1
2ππ£0
2 + ππβ0 =1
2ππ£2
2 + ππ β 0 β1
2π£0
2 + πβ0 =1
2π£2
2
To calculate the final velocity, apply πΈ0 = πΈ2
3 unknowns, so 2 must be known
Projectile motion, scalar treatment - III
Curved motion 7
π£0
β1β0
π£1
π£2
πΉπ
Example: β0 = 10.0π, π£0 = 20.0ππ β1, π£1 = 18.0ππ β1
Range
Trajectory
Maximum height: 1
2π£0
2 + πβ0 =1
2π£1
2 + πβ1 β1
220.02 + 9.81 β 10.0 =
1
218.02 + 9.81 β β1 β β1 = 13.9π
Final velocity: 1
2π£0
2 + πβ0 =1
2π£2
2 + πβ2 β1
220.02 + 9.81 β 10.0 =
1
2π£2
2 β π£2 = 24.4ππ 2
Important: Scalar treatment does not solve: time values & angle values & range !
Projectile motion, vector treatment - I
Curved motion 8
πΉπ
π£
π
π π₯
π π¦ π£π₯
π£π¦
start
origin
Resolve π , π£, π, and πΉ in separate π₯ & π¦ direction.1. Make sure π₯-axis is horizontal, π¦-axis is vertical2. Choose origin below the start point on β = 03. Choose β+ directionsβ: to right and upwards
In that case the equations of motion can be written independently for both directions:
π π₯ = π π₯0 + π£π₯0 β π‘ + 1 2ππ₯ β π‘2
π£π₯ = π£π₯0 + ππ₯ β π‘
π π¦ = π π¦0 + π£π¦0 β π‘ + 1 2ππ¦ β π‘2
π£π¦ = π£π¦0 + ππ¦ β π‘
With the correct initial values this becomes easierβ¦
π
Projectile motion, vector treatment - II
Curved motion 9
πΉπ
π£
π
π π₯
π π¦ π£π₯
π£π¦
start
origin
Choose:π π₯0 = 0 & π π¦0 = β0
π£π₯0 = π£0πΆππ π & π£π¦0 = π£0ππππ
ππ₯ = 0 & ππ¦ = βπ
Now the equations reduce to:π π₯ = π£π₯0 β π‘
π π¦ = β0 + π£π¦0 β π‘ β 1 2π β π‘2
π£π¦ = π£π¦0 β π β π‘
And for a horizontal projection (π = 0)π π₯ = π£0 β π‘
π π¦ = β0 β 1 2π β π‘2
π£π¦ = βπ β π‘
π
Projectile motion, vector treatment - III
Curved motion 10
πΉπ
π£ = 20.0ππ β1
origin
Exampleβ0 = 10.0π, π = 0.0Β°, π£0 = 20.0ππ β1
π π₯ = 20.0 β π‘π π¦ = 10 β 4.905 β π‘2
π£π¦ = β9.81 β π‘
Time at the ground: set π π¦ = 0 β 10 β 4.905 β π‘2 = 0 β π‘ = 1.43π
Range: π π₯ 1.43 = 20 β 1.43 = 28.6π
Final velocity: π£π₯ 1.43 = 20ππ β1 π£π¦ 1.43 = β9.81 β 1.43 = β14.0ππ β1
Magnitude: π£ 1.43 = 202 + 142 = 24.4ππ β1
Angle: π 1.43 = π‘ππβ1 π£π¦ π£π₯ = π‘ππβ1 β14.0 20.0 = β35.0Β°
β0
Projectile motion, vector treatment - IV
Curved motion 11
πΉπ
π£ = 20.0ππ β1
π£π₯
π£π¦
origin
Exampleβ0 = 10.0π, π = 30.0Β°, π£0 = 20.0ππ β1
π£0π₯ = 20πΆππ 30Β° = 17.32ππ β1
π£0π¦ = 20πππ 30Β° = 10.0ππ β1π π₯ = 17.32 β π‘
π π¦ = 10 + 10 β π‘ β 4.905 β π‘2
π£π¦ = 10 β 9.81 β π‘
Time at highest point: set π£π¦ = 0 β 10 β 9.81 β π‘ β π‘ = 1.02π
Height of highest point: π π¦ 1.02 = 10 + 10 β 1.02 β 4.905 β 1.022 = 15.1π
Time at the ground: set π π¦ = 0 β 10 + 10 β π‘ β 4.905 β π‘2 = 0
4.905π‘2 β 10π‘ β 10 = 0 β π‘ =10 Β± 102 β 4 β 10 β β4.905
2 β 4.905= 2.77π
Range: π π₯ 2.77 = 17.32 β 2.77 = 48.0πFinal velocity: π£π₯ 2.77 = 17.32ππ β1 π£π¦ 2.77 = 10 β 9.81 β 2.77 = β17.2ππ β1
Magnitude: π£ 2.77 = 17.322 + 17.22 = 24.4ππ β1
Angle: π 2.77 = π‘ππβ1 π£π¦ π£π₯ = π‘ππβ1 β17.2 17.32 = β44.8Β°
β0
30Β°
Projectile motion, vector treatment - V
Curved motion 12
πΉπ
π£ = 20.0ππ β1
β0 = 10.0π
30.0Β°
π£ = 24.4ππ β1
β1 = 15.1π
π = β35.0Β° π = β44.8Β°
28.6π48.0π
RESULTS of the calculation
Acceleration in circular motion
Curved motion 13
π£0
π£1Ξπ
π
π
π£0
π£1
Ξ π£
Ξπ A
BΞ π
In a circle segment: πππ π΄π΅ = π β Ξπ (πππ)If π small: Ξπ = π β Ξπ β Ξπ = βπ π
The 2 triangles are similar, so:
βπ(π ππππ) =Ξπ£
π£=
Ξπ
π
Divide by Ξπ‘:Ξπ£
π£ β βπ‘=
Ξπ
π β βπ‘β π
βπ£
βπ‘= π£
βπ
βπ‘β π β π = π£2
π =π£2
πCentripetal acceleration
Force in circular motion
Curved motion 14
π£0
π£1
A
B
According to Newtonβs 2nd law an acceleration πrequires an overall force Ξ£πΉ = ππ
In other words:An object that orbits around a point at a distance πWith a velocity π£ requires an overall force:
πΉπππ‘ = πππππ‘ =ππ£2
πCentripetal force
πΉπππ‘
Force in circular motion β Example I
Curved motion 15
Moon circles around EarthDistance Earth - Moon π = 384.4 β 106πPeriod π = 27.32πMass π = 7.35 β 1022ππ
π£ =2ππ
π=
2π β 384.4 β 106
27.32 β 24 β 3600= 1023ππ β1
ππππ‘ =π£2
π=
10232
384.4 β 106 = 2.724 β 10β3ππ β2
πΉπππ‘ = πππππ‘ = 2.002 β 1020π
This force is provided by the gravitational pull of the Earth
Force in circular motion β Example IIa
Curved motion 16
Fairground looping β lowest pointRadius π = 14πVelocity π£ = 24ππ β1
Mass (you) π = 65ππ
ππππ‘ =π£2
π=
242
14= 41ππ β2 πΉπππ‘ = πππππ‘ = 2.67 β 103π
Weight πΉπ = 0.64 β 103π works in the wrong direction!
A normal force πΉπ = 2.67 β 103 + 0.64 β 103 = 3.3 β 103πis required to provide the necessary πΉπππ‘
βyou feel the chair pressing you upwardsβ πΉπ
πΉπππ‘ = Ξ£ πΉ
πΉπ
Force in circular motion β Example IIb
Curved motion 17
Fairground looping β highest pointRadius π = 14πVelocity π£ = 5.2ππ β1
Mass (you) π = 65ππ
ππππ‘ =π£2
π=
5.22
14= 1.9ππ β2 πΉπππ‘ = πππππ‘ = 126π
Weight πΉπ = 638π works in the correct direction, but is too much!
An upwards normal force πΉπ = 638 β 126 = 5.1 β 102πis required to compensate weight and provide the necessary πΉπππ‘
βyou are saved by the braces (belts)β
πΉπ
πΉπππ‘ = Ξ£ πΉ
πΉπ
You are 2 Γ 14π higher now and your velocity equals 5.2ππ β2
in stead of 24ππ β1 . Energy conservation law, check it yourself!
Force in circular motion β Example III
Curved motion 18
Short track skatingRadius π = 8.0πVelocity π£ = 10ππ β1
Mass π = 65ππ
ππππ‘ =π£2
π=
102
8.0= 12.5ππ β2
πΉπππ‘ = πππππ‘ = 813π
Weight πΉπ = 638π works downwards!
Construct a free body diagram to find the contact force by the ice on the skates.
With 1cm β 200π this yields πΉπππ = 1.0 β 103πOr calculate it algebraically with Pythagoras.
π‘ππ π =πΉπ
πΉπππ‘=
ππ
ππ£2 π=
ππ
π£2 = 0.785 β π = 38Β°
Or measure it in the free body diagram
Vectors must beon scale! πΉπ
πΉπππ‘
πΉπππ
π
Satellite orbits
Curved motion 19
In case of satellites orbiting a planet (Earth), the πΉπππ‘
Is provided by the gravitational force between to masses:
πΉπ = πΊπ β π
π2
Newtonβs law of gravitation
πTypically large
πTypically small
πΉ
π£
π
Gravitational constant πΊ = 6.67384 β 10β11π3ππβ1π β2
Inverse square law
Keplerβs 3rd law
Curved motion 20
πΉπ = πΉπππ‘ β πΊπ β π
π2=
π β π£2
πβ πΊ β π = π β π£2
β
π π
π
Substitute: π£ =2ππ
π
πΊ β π = π β2ππ
π
2
= 4π2π3
π2 βπ3
π2 =πΊπ
4π2 = ππππ π‘πππ‘
π
Attention: π = π π + β. Always add the planetβs radius to the orbiting altitude to get the correct radius
Keplerβs 3rd law - Example
Curved motion 21
π3
π2 =πΊπ
4π2 =6.67384 β 10β11 β 5.976 β 1024ππ
4π2 = 1.010 β 1013π3π β2
Calculate the altitude above the Earthβs surface of geostationary satellites
π3 = 1010 β 1013 β 23.93 β 3600 2 = 7.4975 β 1022
π =32.355 β 1023 = 42.167 β 106π
β = π β π π = 42.167 β 106 β 6.378 β 106 = 35.79 β 106 πwikimedia
Earth
Mass π = 5.976 β 1024ππ
Radius π π = 6.378 β 106
Siderial rotation period
π = 23.93β
END
Curved motion 22
DisclaimerThis document is meant to be apprehended through professional teacher mediation (βlive in classβ) together with a physics text book, preferably on IB level.