Unit 1 - Kinematics And Dynamics Flashcards

(43 cards)

1
Q

Horizontal component velocity

A

U(h) = R*cosx°

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2
Q

Vertical component velocity

A

U(v) = R*sin°

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3
Q

Newton’s Universal Law of Gravitation

A

F = Gm(1)m(2)
————
r^2

G = gravitational constant (6.67*10^-11m^3kg^-1s^-2)

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4
Q

Gravitational field strength definition

A

The gravitational force per kilogram or weight per unit mass

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5
Q

Inverse square nature of gravitational force

A

As the distance between two masses increase, the gravitational force decreases

As it doubles, force quarters
As it triples, force is 1/9th etc

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6
Q

Why do satellites orbit?

A

Gravitational force exerted on satellite
Force accelerates the satellite
Orbital speed is constant, but velocity vector changes direction
Satellite follows curved path that follows the curvature of the Earth

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7
Q

Newton’s first law

A

Balanced forces mean the object will be at rest or constant velocity

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8
Q

Newton’s second law

A

Unbalanced forces accelerate masses

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9
Q

Newton’s third law

A

Each force exerts an equal and opposite reaction

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10
Q

If tension force and weight are balanced

A

At rest, constant upwards speed or constant speed downwards

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11
Q

If tension is greater than weight

A

Constant upward acceleration or constant downward acceleration

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12
Q

If weight is greater than tension

A

Constant downward acceleration

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13
Q

What must happen when calculating forces applied at an angle?

A

Get horizontal and vertical components

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14
Q

Equations for weight component

A

W(c) = WsinX°

Or

W(c) = mgsinX°

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15
Q

Equation for gravitational potential energy

A

E(p) = mgh

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16
Q

Equation for kinetic energy

A

E(k) = 1/2mv^2

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17
Q

Equation for work done

A

E(w) = Fd

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18
Q

What is momentum?

A

Product of mass and velocity:

p = mv

19
Q

What is the principle of conservation of linear momentum

A

The total momentum before a collision or explosion is equal to the total momentum after a collision or explosion when there are no external forces like friction

20
Q

What is an elastic collision

A
Total E(k) before 
=
Total E(k) after

Total kinetic energy conserved

21
Q

What is an inelastic collision?

A

More kinetic energy before collision

Most energy lost to heat

22
Q

What happens in an explosion?

A
One mass splits into two
Total E(k) increases
Total energy and momentum conserved
23
Q

Equations for impulse

A

Impulse = F(avg)*t(c)

Impulse = change in momentum

Impulse = mv-mu

F(avg)*t(c) = mv-mu

Impulse = area under graph

24
Q

The effect of hardness of surface on impulse

A

Softer surfaces increase contact time which results in the average force being less if change in momentum is the same

25
Find random uncertainty
``` Random uncertainty = max-min --------- N ```
26
Calculate percentage uncertainty
``` Percentage uncertainty = Random Uncertainty --------------------- * 100 Mean ```
27
What uncertainty do you use when calculating something
Biggest uncertainty in one of the variable Same with percentage
28
Analogue scales for uncertainties
Far apart divisions = 1/5 | Close divisions = 1/2
29
Digital scale for uncertainties
Always +/-1 of the last digit Eg 9.98 would be +/-0.01
30
Systematic uncertainties
Give consistently too high or too low reading Eg scale that isn't reading 0 before you weigh something
31
What happens during the Doppler effect
Sounds waves propagate outwards from the source at 340ms^-1 (in air)
32
Doppler effect when source is moving towards observer
Source is moving towards so waves bunch closer together and therefore the source is heard to be higher pitched
33
Doppler effect when source is moving away from observer
Source is moving away so waves spread further apart and therefore the source is heard to be lower pitched
34
What sign do we use when the source is moving away?
Away = add
35
What sign do we use when the source is moving towards the observer?
Towards = take away
36
Equation for Hubble's constant
v = Hd recession velocity = hubble's constant * distance Hubble's constant = 2.3*10^-18s^-1
37
Redshift equations
z=v/c Redshift = recession velocity / speed of light z = observed wavelength - rest wavelength ------------------------------------- rest wavelength
38
How can the age of the universe be calculated?
Rewinding the expansion process back to a singularity at the start of the universe t = 1 / Hubble's constant
39
Evidence for the Big Bang
Expanding universe Most galaxies redshifted Rewinding expansion leads to singularity that contained everything in universe Cosmic microwave background radiation- the "after glow" of the Big Bang Abundance of hydrogen and helium as these were most likely to form as universe cooled from Big Bang
40
What is dark energy?
Fuels the expansion of the universe
41
What is dark matter?
Not detected easily as it weakly interacts with detectors
42
Evidence for dark matter?
Rotational speeds of galaxies requires a bigger gravitational force than can be accounted for by mass detected Gravitational lensing - light is affected by dark matter which explains some astronomical explanations
43
How do you calculate temperature of stellar objects?
By plotting intensity of radiation against wavelength Peak wavelength * temperature in kelvin = constant (2.9*10^-3)