Mod 5 Flashcards

1
Q

Important equations to remember

A

V=Vx+Vy
Vx=Vcosθ
Vy=Vsinθ
V=(V^2x+V^2y)^1/2
θ=tan^-1Vy/Vx

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2
Q

Theory behind projectile motion

A

A projectile is the name given to an object which is unpowered and the only force acting on the object is force due to the gravity.
Assumptions:
There is no such thing as air, If there was air, then the projectile would also experience a changing air resistance force. In the absence of this air resistance force, we will see that an object undergoing projectile motion will trace out a parabolic path.
The acceleration due to gravity is a constant value and has a constant direction (this way we can use our existing equations of uniform acceleration for analysis). This is a reasonably safe assumption if the height the projectile reaches is relatively low. We will see in a separate focus area how acceleration due to gravity changes as height changes.
We ignore the impact of the curvature of the Earth. Another relatively safe assumption (#FES for life). The range of our projectiles are usually small enough to assume that the Earth is relatively flat over the distance.
We also ignore any impact that the rotational motion of the Earth may have on velocity and/or acceleration

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3
Q

Describe the trajectory of an ideal projectile accounting air resistance

A

It has a decreased max height and range as well as a loss of symmetry. This is due to the Initial air force opposing the motion of the object and acts both horizontally and vertically. The maximum vertical displacement is lower as the air force opposes the upwards vertical motion. The range will decrease as the air force will cause the initial horizontal velocity to decrease.
Vy^2=uy^2+2aysy
sy=-uy^2/2ay

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4
Q

What affects the components of projectile motion

A

Projectile motion is two dimensional motion and can be analysed by considering its horizontal (Vx) and vertical (Vy) components of velocity.
The vertical component of velocity is affected by acceleration due to gravity and hence undergoes a constant acceleration due to this gravity (ay=-9.8 ms^-2)
The horizontal component of velocity isn’t affected by any external forces hence maintaining a constant value throughout the entire time of flight. Provided air resistance and the curvature of earth are ignored, it maintains a parabolic path. Since these components of velocity are perpendicular to each other, one has no impact on the other, they can therefore be considered as isolated or independent and hence be solved individually.

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5
Q

Conditions of type 2 projectile motion

A

An object is projected horizontally with a velocity of u from a cliff or some other object at height h.
Initial vertical velocity is 0
Initial horizontal velocity is ux
Overall vertical displacement is -h

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6
Q

Conditions of type 1 projectile motion

A

A projectile launched with an initial velocity at an angle θ above the horizontal. This projectile then strikes another point such that the change in vertical displacement from the beginning to the end of its journey = 0
Initial vertical velocity is usinθ
Initial horizontal velocity is ucosθ
Vertical velocity at max height is 0
Horizontal velocity at max height is ucosθ
Total velocity at max height is ucosθ. V=(Vx^2+Vy^2)^1/2. Vy=0
Final vertical displacement is 0
Final vertical velocity is -usinθ
Time to max height is t=(vy-uy)/ay. t=-uy/ay=-usinθ/ay
Time from max height to ground is t=-uy/ay
Total time of flight is T.O.F=-2uy/ay
Sy=max when tmax =T.O.F/2 and vy=o which is at max height
Sy=0 when t=o or t=T.O.F and when vy=+-uy
T.O.F time of flight
Range equation is sx=(u^2sin2θ)/g
Maximum range will always occur when the launch angle is 45°

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7
Q

Derivation of range equation

A

Sx=uxt
Sy=uyt+1/2ayt^2
o=uyt +1/2ayt^2
=uyt-g/2 x t^2
g/2 x t^2=uyt
t=2uy/y=(2usinθ)/g=T.O.F
Sx=uxt =ucosθ x (2usinθ)/g
=u^2x 2sinθ cosθ
(u^2 x sin2θ)/g

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8
Q

Conditions of type 3 projectile motion

A

Type 3 is a projectile launched with an initial velocity at an angle θ above or below the horizontal. This projectile then strikes another point such that there is a change in vertical displacement from the beginning to the end of its journey. The projectile will finish above or below where it started. Sy doesn’t equal 0.
Initial vertical velocity is +- usinθ
Overall vertical displacement is +-h

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9
Q

What is a projectile
What is gravity
Gravitational force effect on projectile

A

An unpowered object and the only force acting on it is gravitational force
A force occurring between two objects with mass.
It is constant force acting vertically downwards

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10
Q

How to do type 4 projectile motion

A

What is the question asking for
Like when sx=25m, is sy>20, want to get one solution before and after sx=25m
Then solve for t or any other variable

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11
Q

How to find time for stroboscopic images

A

Divide the time by the no of gaps
To get time use suvat equation or use frequency or period

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12
Q

How to describe acceleration and net force direction in circular motion

A

Radially inward or outward

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13
Q

Source of centripetal force in
Ball on a string whirled in a circle
Car driving around a corner
Satellite orbiting the Earth

A

Tension
Friction
Gravity
Note: If force is removed, then the object will fly off at a tangent.

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14
Q

Centripetal acceleration formula
Centripetal force formula
How to find velocity in circular motion

A

ac=v^2/r where centripetal acceleration acts radially inwards
Fc=mv^2/r
v=d/t = 2πr/T =2πrf

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15
Q

Angular velocity formula
Angular displacement formula

A

ω=Δθ/Δt = v/r
Δθ: angular displacement
ω: rotational velocity
θ=arc length/radius = s/r
Note: If angular displacement is 360, then the arc length is 2πr. The angular displacement would be 2πr/r=2π

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16
Q

How to find linear velocity from angular displacement equation

A

s/r=θ
s/t=rθ/t
If the time taken to turn a corner is known, then v=rθ/t =ωr

17
Q

In a completely flat horizontal circular pendulum scenario, what is tension
For conical pendulums, how to derive velocity
Sum of all vertical and horizontal forces in this scenario

A

Fc=tension where normal and weight force are opposite to each other whilst tension acts radially inward. |FN|=|FW|
Sum of all Fy=0,
Tcosθ=mg
Tsinθ=mv^2/r
2/1 =Tsinθ/Tcosθ =(mv^2/r)/mg
tanθ=v^2/rg
v=(grtanθ)^1/2
Fnetx=Tsinθ=mv^2/r
Fnety=0

18
Q

How to calculate velocity at banked tracks with friction and without friction when velocity <ideal speed

A

With friction: Vmin<v=(grtanθ)^1/2<Vmax
Without friction
ΣFx=mv^2/r ΣFy=0
Fnsinθ=Ffcosθ=mv^2/r FNcosθ+Ffsinθ=mg
F=μN

FNsinθ-Ffcost=(mv^2)/r Fncosθ+Ffsinθ=mg
FNsinθ-μFncosθ=mv^2/r FNcosθ+μFNsinθ=mg
FN(sinθ-μcosθ)=mv^2/r FN(cosθ+μsinθ)=mg
FN=mg/cosθ+μsinθ

FN(sinθ-μcosθ)=mv^2/r
g/cosθ+μsinθ (sinθ-μcosθ)=v^2/r
Vmin=(gr(sinθ-μcosθ))/cosθ+μsinθ)^1/2
Divide by cosθ/cosθ
Vmin=(gr(tanθ-μ))/1+μtanθ)^1/2
tanθ=(v^2/gr +μ)/1-μv^2/gr
=(v^2 +grμ)/(gr-μv^2)

19
Q

How to calculate velocity when velocity >ideal speed

A

Vmax=gr(tanθ+μ)/1-μtanθ

20
Q

Equation for work
Torque equation

A

W=Fxcosθ
τ=Ia
I: movement of inertia is constant
a: angular acceleration
τ=r⊥F=rFsinθ
r: distance between axis of rotation and the point of application of the force
F: force applied to object
θ: The angle between radius of rotation and the force vector

21
Q

gravity equation

A

g=Fw/mg=N/kg
F=ma=kgms^-2 is field strength
Newton’s law of Universal gravitation
Fg=G m1m2/r^2
FG: force due to gravity
G: Universal Gravitational constant
m1, m2: masses of the 2 objects
r: distance between centre of masses

22
Q

Acceleration due to gravity equation
Derivation of acceleration due to gravity

A

Fg=Fw
Gm1m2/r^2 =m1g
g=Gm/r^2

23
Q

NLUG formula
Kepler’s third law of motion

A

Fg=Gm1m2/r^2
Gm2/4π = r^3/T^2

24
Q

Derive orbital velocity formula

A

Fc=Fg
mv^2/r =Gm1m2/r^2
v=sqrt(Gm2/r)

25
Q

Gravitational potential energy formula
Change in GPE

A

U=-Gm1m2/r
-GMm(1/ri - 1/rf)

26
Q

Kinetic energy formula in orbit
Orbital energy formula

A

K=Gm1m2/2r
Note: kinetic energy is half of gravitational potential energy
E=-GMm/2r

27
Q

Derive escape velocity formula

A

|1/2 mv^2|=|GMm/r|
𝑣^2= 2𝐺𝑀𝐸/𝑟
v=sqrt(2GM/r)

28
Q

Centrifugal vs centripetal force

A

The apparent force, equal and opposite to the centripetal force, drawing a rotating body away from the centre of rotation, caused by the inertia of the body.
The force that causes a moving object to follow a curved path rather than continue on a straight line. The force is directed towards the centre of the curve.

29
Q

Difference in tension values in vertical circular motion

A

Top:
F=mv^2/r = N +mg
mv^2/r= T + mg
T= mv^2/r - mg
Bottom:
F=mv^2/r = N-mg
mv^2/r = T - mg
T= mv^2/r + mg

30
Q

Derivation of v=sqrt(grtanθ)

A

In the vertical direction there is no acceleration, hence Ncosθ = mg
In the horizontal direction Fnet = mg tanθ and
as Fnet = Fc then 𝑚𝑔 𝑡𝑎𝑛𝜃= (𝑚𝑣^2)/𝑟
Rearranging this equation, we get:
𝑣= √𝑔𝑟𝑡𝑎𝑛𝜃

31
Q

Altitude of:
low earth orbit
medium earth orbit
geostationary/geosynchronous

A

160-2000 km
2000-36000 km
35786 km

32
Q

Period of:
low earth orbit
medium earth orbit
geostationary/geosynchronous

A

1.5 – 2
2 – just below 24
24

33
Q

What are keplers laws of motion

A

Kepler’s first law states:Each planet moves, not in a circle, but in an ellipse, with the sun, off centre, at a focus.
Kepler’s second law states: The linear speed and angular speed of a planet are not constant, but the areal speed of each planet is constant. That is, a line joining the sun to a planet sweeps out equal areas in equal times.
Kepler’s third law states: For all planets, the cube of the average radius is proportional to the square of the orbital period; that is, 𝑟^3/𝑇^2 =𝐺𝑀/(4𝜋^2 ) is a constant for all planets going around the Sun.

34
Q

Uses of:
low earth orbit
medium earth orbit
geostationary/geosynchronous

A

They encounter orbital decay due to the low altitude of the satellites. Uses include spying, weather surveying, geotopographic studies.
Useful for GPS, television, global radio communication.
Used in telecommunications and weather prediction.
Geostationary – orbits Earth at the equator.
Geosynchronous – placed in non-equatorial orbits (i.e. moves above / below the equator in a figure 8 pattern)