M5 Advanced Mechanics Flashcards

You may prefer our related Brainscape-certified flashcards:
1
Q

Projectile motion

A
a(x) = 0 
v(x) = ucos(theta) 
x = utcos(theta) 
a(y) = -g 
v(y) = -gt + usin(theta) 
y = -gt2 / 2+utsin(theta)
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
2
Q

Pendulum

A

T = 2pi x sqrt(L/g)

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
3
Q

Centripetal force

A

towards the centre Fc = mv2/r formula sheet.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
4
Q

Centrifugal force

A

reaction force to centripetal force.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
5
Q

Tangential velocity

A

v = 2r x pi / T

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
6
Q

Angular displacement

A

change in theta = s/r where s is length round the circumference, r is radius and theta is in radians.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
7
Q

Angular velocity

A
w = change in theta / change in time
wr = v where r is radius, v is linear/tangential velocity
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
8
Q

Conical Pendulums

A

Fc = T + mg

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
9
Q

Newton’s Universal Law of Gravitation

A

F = GMm/r2 r measured from centre of masses

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
10
Q

Gravitational Field Strength

A

F per unit mass g = Gm/r2

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
11
Q

Kepler’s Three Laws of Planetary Motion

A
    1. The planets move in ellipses with the sun at one focus.
    1. The line between the Sun and the planet sweeps out equal areas in equal time.
    1. T2 is proportional to r3. r3/T2 = GM/4pi2
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
12
Q

Escape velocity

A

let change in U = EK

v = sqrt(2GM/r)

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
13
Q

Orbital Velocity

A
let Fg = Fc
v = sqrt(GM/r)
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
14
Q

Geostationary Orbit

A
  • stays in the same place relative to the earth, T = 1 day
  • Above outer Van Allen, 35 000km
  • wide field of view
  • allows tracking of stationary point on Earth
  • used for communications, mass-media, weather monitoring
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
15
Q

Low Earth Orbit

A
  • 160 to 2000 km (below inner Van Allen belt)
  • small field of view
  • frequent coverage of specific or varied locations
  • difficult to maintain orbit due to satellite drag
  • used for military, earth observation, shuttle missions, Hubble space telescope
How well did you know this?
1
Not at all
2
3
4
5
Perfectly
16
Q

Polar Orbit

A
  • period can be as low as 30 minutes
  • orbits around the poles, almost perpendicular to the equator
  • used for weather, climate, oceans, volcanoes and vegetation patterns
17
Q

Potential energy of a planet/satellite in orbit

A

U = -GMm/r

negative as U approaches 0 as r approaches infinity

18
Q

Kinetic energy of a planet/satellite in orbit

A
EK = mv2/2 where v2 = GM/r
EK = GMm/2r
19
Q

Total energy of a planet/satellite in orbit

A

U + EK = -GMm/2r