ODU(part 2) Flashcards

1
Q

What is a projectile

A

A projectile is any object which freely accelerates due to gravity whilst moving forward at the same time.

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2
Q

What are the 2 main types of projectiles

A

horizontal and angled

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3
Q

What 2 componenets are projectiles made up of

A

projectiles are made up of horizontal and vertical components which act independently.

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4
Q

Describe the horizontal component of a projectile

A

Constant velocity, no acceleration

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5
Q

Describe the vertical component of a projectile

A

constant downwards acceleration due to gravity, where a = 9.8 ms^-2

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6
Q

What is the formula for the horizontal component of velocity in an angled projectile

A

uh = ucos0

uh = initial horizontal speed
0 = angle of projectile
u = initial speed of projectile

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7
Q

What is the formula for the vertical component of velocity in an angled projectile

A

Uv = usin0

uv = initial vertical velocity
0 = angle of projectile
u = initial speed of projectile

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8
Q

The moon is a …

A

natural satellite

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9
Q

The ISS is an…

A

artificial satellite

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10
Q

What does gravitiation force between two objects depend on

A

the two masses

distance between their centres

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11
Q

State newtons law of gravitation

A

F = Gm1m2/r^2

m1 and m2 are masses of the two objects in kg
r is the distance between the centres of the objects.
G is the universal constant of gravitation.

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12
Q

State the universal constant of gravitation

A

G = 6.67*10^-11 Nm^2kg^-2 (given on data sheet)

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13
Q

the gravitational force between an object and a planet is its []

A

weight

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14
Q

What is a frame of reference

A

How you describe the motion of an object depends on how you observe it

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15
Q

What is an inertial reference frame

A

Simply two places that are moving at constant speeds relative to one another.

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16
Q

What is an absolute reference frame

A

A unique, universal frame of reference from which everything could be defined or measured. Einstein proved no such reference frame exists.

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17
Q

What are einsteins 2 postulates (assumptions)

A

1) observers moving at constant speed relative to one another (inertial frames) will observe the same laws of physics.

2) the speed of light in a vacuum is the same for all observers regardless of their motion relative to the light source.

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18
Q

What is time dilation

A

Time dilation is the difference in a time interval as measured by a stationary observer and a moving observer.

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19
Q

State the dilated time formula

A

t’ = t/ (√(1-(v/c)^2))

where t is proper time
t’ is dilated time
v is the velocity of the object relative to a rest frame
c is the speed of light in a vacuum

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20
Q

Define proper time

A

Proper time is the time measured in the frame in which the clock is at rest relative to the event. The time will always be shorter in the rest frame.

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21
Q

Define dilated time

A

Dilated time is the time measured on a clock that is moving with a constant velocity relative to you. The time will be longer so the clock is seen to be running slow.

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22
Q

What is length contraction

A

Length contraction is a difference in the length of an object as measured (parallel to the direction of travel) by a stationary observer and a moving observer.

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23
Q

What is the formula for length contraction

A

l’ = l(√(1-(v/c)^2))

24
Q

Define proper length

A

Length measured by the observer at rest with respect to the moving object

25
Q

Define contracted length

A

Contracted length of the object as measured by another observer.

26
Q

What is the lorentz factor

A

The lorentz factor is a way of taking into account the speed of a moving object.

27
Q

State the lorentz factor

A

Y = 1/(√(1-(v/c)^2))

28
Q

At what point relative to c are relativistic effect neglible at

A

Relativistic effects are neglegible when speed are below about 0.1c

29
Q

At what speed relative to c does length contraction become significant

30
Q

Dilated time is measured by

A

an observer who is not in the frame of reference that the event is taking place.

31
Q

Length contraction only occurs in

A

the direction parallel to the motion.

32
Q

What is the doppler effect

A

The doppler effect is the change in observed frequency when a sound source is moving relative to a stationary observer

33
Q

What happens when a sound source is moving towards a stationary observer

A

more waves reach you per second so the frequency of the sound is increased (wavelength is decreased)

34
Q

What happens when a sound source is moving away from a stationary observer

A

Less waves reach you per second so the frequency of the sound is decreased (wavelength is increased)

35
Q

State the doppler equation

A

fo = fs(v/(v+/-vs)
where v is the velocity of sound
fo is frequency heard by the observer
fs is the frequency emmited by the source
vs is of the moving source

36
Q

State 2 applications of the doppler effect

A

Ultrasound in medicine
Radar speed guns

37
Q

Define redshift

A

When a lightsource is moving away from you, the frequency decreases, so the spectrum shifts to longer wavelengths. This is called redshift.This is the doppler effect applied to light.

38
Q

State the redshift formula

A

z = (λo - λr)/ λr
where z is redshift (no units)
λo is the observed wavelength in metres
λr is the rest wavelength in metres

39
Q

z is positive for _______ and negative for _________

A

Redshift, Blueshift

40
Q

State the formula for redshift provided that stars and galaxies are moving at non relativistic speeds

A

z = v/c

where:
z is redshift with no units
v is recessional velocity of the star in metres per second
c is the speed of light in metres per second

41
Q

What were Hubbles two conclusions (Hubble Lemaitre’s law)

A

1) The bigger the magnitude of the shift the greater the speed the galaxy was moving away from the earth.
2) The further away a galaxy is the greater the speed it is travelling

42
Q

State 2 things known about the expansion of the universe

A

The galaxies do not expand (they are gavitationally bound)

Space between the galaxies expands carrying the galaxies with it.

43
Q

State the hubble lemaitre’s law formula

A

V = Hod
where:
Ho is hubbles constant with units per second
d is distance to the galaxy from earth in metres, m
v is the recessional velocity of the galaxy in metres per second

44
Q

Plotting a graph of recessional velocity of galaxies against their distnace from earth gives a straight line of best fit through the origin, the gradient of this graph gives….

A

the value for hubbles constant.

45
Q

State hubbles constant

A

2.3x10^-18 s^-1

46
Q

Explain how the age of the universe can be found using hubbles law

A

Hubbles law suggests that galaxies further away from us are moving away faster than galaxies closer to us.

Therefore the universe is expanding

If we asusume the rate of expansion is fixed then most galaxies have been moving apart at a constant rate.

So time taken for them to reach their relative positions (ie age of the universe) must be t = d/v

Since Ho = v/d, then the age of the universe = 1/Ho = 4.35x10^17 s

47
Q

What is dark matter and how do we know it exists

A

We can determine the mass of galaxies from their orbital speed, but the total masses measured are bigger than the mass accounted for by the observable stars in a galaxy.
The unaccounted mass is called dark matter.

48
Q

Why is the universe still expanding despite the existence of dark matter, what is opposing the additional gravitational effects caused by the increase of matter

A

Dark energy

49
Q

Define dark energy

A

Dark energy is a source of energy capable of producing a force which acts against the gravitational force of attraction, pushing matter apart.

50
Q

Ordinary matter and energy make up what % of the universe

51
Q

Dark energy makes up what % of the universe

52
Q

Dark matter makes up what % of the universe

53
Q

A hot star will appear what colours

54
Q

A cooler star will appear what colour

55
Q

How does peak wavelength relate with temperature

A

Peak wavelength is shorter for hotter objects than for cooler objects

56
Q

How does radiation relate with temperature of objects

A

Hotter objects emmit more radiation per units surface area per unit time than cooler objects.