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A Level Physics

4. Circular Motion, Gravitation & SHM

4.1 Motion in a Circle
4.2 Centripetal Force
4.3 Kepler's Laws
4.4 Law of Universal Gravitation
4.5 Earth's Gravitational Field
4.6 Artificial Satellites
4.7 Escape Velocity
4.8 Weightlessness
4.9 Simple Harmonic Motion
4.10 Equations of SHM
4.11 Mass on a Spring
4.12 Simple Pendulum
4.13 Energy of SHM
4.14 Damped Oscillations
4.15 Forced Oscillations and Resonance


4.1 Motion in a Circle ( examples )

(a) Angles in radians :______s = rq______s - arc length, r - radius, q - angle (radians). 1

__________________________arc length = radius x theta

(b) Angular velocity : ____w = angular velocity____ velocity, v = velocity (at a tangent) ____as s = rq____then v = rw
(c) centripetal acceleration:____a = acceleration due to change in direction - from vector diagram = w2r
__________diagrams - showing angular acceleration

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4.2 Centripetal Force ( examples )

This force causes the circular motion to change direction. It is directed towards the centre.

_____F = ma = centripetal force_____as v = rw_______F = mw2r

Rounding a bend

car over a mound mg - R = centripetal force_____ car banking around corner - no friction ___ (normal=mg)/centripetal force => tan q = angle of banking

Bucket of water

A bucket of water is swung in verticle circle

___normal force keeps water in bucket___ mg < centripetal force Þ water stays in bucket.

Pendulum

A pendulum made to move in a horizontal circle, with tension T in the string.

___horizontal motion of pendulum ___Tsinq = centripetal force ___Tcosq = mg ___Þ tanq = angle of banking

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4.3 Kepler's Laws ( examples )

From prolonged observations of planets Kepler produced 3 laws

1. Earth moves in an ellipse which has the sun as one focus.
2. The line joining the sun to a moving planet sweeps out equal areas in equal times.
3. r3 µ T2, _r - radius of planet-sun, T - period of planet around sun.

planet - equal areas in equal times
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4.4 Law of Universal Gravitation ( examples )

"Every particle of matter in the universe attracts every other particle with a force which is directly proportional to the product of their masses and inversely proportional to the square of their distance apart. "

Law of Universal Gravitation

______________Deriving kepler's laws ________ r - radius; m, M - masses; v - velocity
Table 4.4.1 Astronomical data

Body Equatorial radius, m Mass, kg Density, kgm-3 Distance to sun, m Surface gravity, ms-2 Number of satellites Sidereal period, days Rotational period, days, hours
Sun 6.960 x 108 1.989 x 1030 1409 - - - - 274 - - - - - - - - 25.38 d
Moon 1.738 x 106 7.353 x 1022 33340 1.496 x 1011 1.62 - - - - 27.32 d 27.32 d
Mercury 2.42 x 106 3.301 x 1023 5420 5.791 x 1010 3.76 0 87.97 d 58.7 d
Venus 6.85 x 106 4.869 x 1024 5250 1.082 x 1011 8.77 0 224.7 d 243 d
Earth 6.378 x 106 5.978 x 1024 5510 1.496 x 1011 9.81 1 365.3 d 23.9 h
Mars 3.375 x 106 6.420 x 1023 3960 2.279 x 1011 3.80 2 687 d 24.6 h
Jupiter 7.14 x 107 1.899 x 1027 1330 7.783 x 1011 24.9 13 11.86 yr 9.9 h
Saturn 6.04 x 107 5.685 x 1026 680 1.427 x 1012 10.4 10 29.46 yr 10.2 h
Uranus 2.36 x 107 8.686 x 1025 1600 2.869 x 1012 10.4 5 84.02 yr 10.7 h
Neptune 2.23 x 107 1.025 x 1026 1650 4.498 x 1012 13.8 2 164.8 yr 15.8 h
Pluto 3 x 105 5 x 1023 3000 5.900 x 1012 4 0 248 yr 6.3 d
1 sidereal year (yr) = 365.256 mean solar days (=>earth day = 23.9 hr)

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4.5 Earth's Gravitational Field ( examples )

Action at a distance, effect of a body A exerting a force on another body B. Due to a gravitational field around A.

Gravitational field strength, ____g = g => force acting on unit mass placed in the field = units: N/kg or m/s^2 _______due to density, g1 increases slightly at 1st, g1 = GM1/b^2
g' = GM/r^2, where r > r0
___Variation of g with height.

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4.6 Artificial Satellites ( examples )

circular orit _______centripetal = force of gravity, KE, PE - satellites

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4.7 Escape Speed ( examples )

escape speed -> KE(max) = PE (earth to infinity) ___ escape speed

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4.8 Weightlessness In Orbit ( examples )

When Fc = Fg \ no net force experienced in ship, no net acceleration relative to ship

__________________________ centripetal force = force of gravity (same force)

For a body in a lift descending___ mg - S = ma___ if S = mg Þ weightlessness ( S is normal reaction )

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4.9 Simple Harmonic Motion ( examples )

In oscillatory motion the acceleration, displacement & velocities change periodically (in magnitude & direction).

Definition of SHM - If the acceleration of a body is directly proportional to its distance from a fixed point and is always directed towards that point, the motion is simple harmonic.

__________________________ circluar motion analogy to SHM

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4.10 Equations of SHM ( examples )

Time peiod , T - time to complete one cycle or oscillation.
Frequency, f - number of oscillations per second.
Amplitude, A or r - maximum displacement from mean position.
Phase, f - the initial angular state of the system, usually as a fraction of the time period.
Phase difference, Df degree to which oscillations are out of step, in relation to the time interval between maximum displacements._______Df = (time difference at maximas) / (time period)

acceleration,_a µ - x,_______a = - k x = - w x2 = - w2A sin wt,____ velocity,_v = - vm cos wt = w ± ( A2 - x2 )½
max. velocity, vm = ± wA____displacement,_x = A sin wt = A sin ( wt + f )__if x = 0 at t = 0 then f = 0,
(q = wt, vm = wA ), __T = period = 1/frequency = ang.vel./one cycle

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4.11 Mass on a Spring ( examples )

_______________________________SHM of mass on a spring

Hooke's law :________T = ke, \ T0 = mg = ke0 ( equilibrium )
When displaced, x : ___F = mg - T = mg - k ( e0 + x ) = mg - mg - kx
Newton's 2nd law : ___.F = ma, \ ma = - kx \ a = acceleration = - spring constant x displacement / mass \ period T = 2p Period, also T = 1/f = 2.PI/omega

SHM Experiment to find 'g' using mass on a spring
_____SHM experiment to find 'g'
From (4.11): T2 = 4p2extension/gravity and extension/gravity

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4.12 Simple Pendulum ( examples )

simple pendulum
for x & q small ® sin q = sin theta = displacement / length
Force towards centre ( perpendicular to to tension ), F = - mg displacement / length _____ T = Time Period of oscillations - over 2PI
SHM Experiment to find 'g' using a pendulum

F = mg displacement / length ____ acc. = - wx2 = g displacement / length ____ Þ w2 = gravity / length ____\ w = (gravity / length)^0.5
As T = Time Period of oscillations - over 2PI____then T2 = Time Period squared
Period squared vs. pendulum length
If g = 9.8 ms- 2 then the experiment has accurately been measured for SHM where acc. = - wx2 .

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4.13 Energy of SHM ( examples )

Variation of KE & PE with time - SHM system with amplitude 'a'
PE = ½ F x____( F = k x )____\ PE = ½ k x2 = ½ m w2y2 ____(amplitude a2 = x2 + y2, y can be incorporated into diagram 4.9)
KE = ½ m v2 = ½ m w2x2____E = KE + PE__ (conservation of mechanical energy)

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4.14 Damped Oscillations ( examples )

Damping :
degrees of damping

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4.15 Forced Oscillations and Resonance ( examples )

The graph relates to the experiment with 'Bartons pendulum' & also other SHM systems.
amplitudes / driving frequency / resonance____
Examples of resonance Þ air column in musical instrument, radio tuned to natural frequency = radio signal (electrical resonance), Tacoma Narrows Bridge disaster - wind caused oscillating force in resonance with natural frequency of the bridge.

Experiment to find resonant amplitude - Barton's pendulums
Barton's pendulums - resonant pendulum => A = Z
Frequency, f, found from time exposure photographs. Resonant pendulum = 1/4 oscillation behind diver pendulum.

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Reference

1. If s = r then q = 1 radian ( rad ) - 1 rad is the angle subtended at the centre of a circle by an arc = in length to the radius. The circumference is s = 2pr where q = 2p rad. ( or 360° )

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