u4: fields Flashcards

(40 cards)

1
Q

field

A

region in space around an object where object exerts force on another

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2
Q

examples of forces tht have fields associated w/ them

A
  • gravitational
  • magnetic
  • electric
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3
Q

newtons law of universal gravitation

A

FG=Gm1m2/r^2

  • FG: grav attr’n btwn two objs (N)
  • G: 6.67 x 10^-11
  • m1m2: masses of both objects (kg)
  • r: centre-to-centre distance
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4
Q

you have three asteroids arranged in a line. you need to find the net gravitational force acting on one of them. how do u do this?

A
  1. draw FBD for forces acting on needed asteriod
  2. make directional compass
  3. write F(C) = F(AonC) (+/-) F(BonC)
  4. put direction in answer
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5
Q

gravitational field strength? when is it used?

A
  • used when finding force of gravity of objects on a planet

g= Gm / r^2
- m: mass of planet
- r: radius of planet

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6
Q

relationship btwn field strength and distance from a planet’s centre?

A

inverse square relationship: as distance from planet centre increases, gravitational field strength decreases rapidly

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7
Q

how do u solve satellite questions?

A
  1. draw a diagram. find the distance btwn centre of planet and satellite w/ wtvr info u have
  2. plug into g=Gm/r^2 where m is mass of satellite
  3. if asked for gravitational force of any object at that point: do Fg=mg where g is the value u just calculated in S2
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8
Q

what keeps moon/satellites in orbit around earth?

A

gravity

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9
Q

what shape is orbits

A

circular

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10
Q

what kind of motion do satellites and moon undergo

A

centripetal motion

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11
Q

how do you find the net centripetal force acting on an orbiting object?

A

F(c) = ma(c) = mv^2 / r

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12
Q

formulas for orbital speed

A

v^2 = GM/r
- v is speed in m/s
- M os mass of central body
- r is orbital radius (centre to centre)

v = 2πr/T
- T is orbital period

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13
Q

relationship btwn orbital speed and distance from planet

A

orbital speeds decrease as u move further from the sun

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14
Q

what is orbital period

A

T
- time for orbiting object to complete a rotation

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15
Q

geosynchronous orbits

A
  • geosyn. satellites orbit at same speed as earth turns
  • orbital period is 24 hours
  • if located above earth’s equator, they stay in a fixed spot and are called geostationary
  • used for weather and terrestrial monitoring
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16
Q

electric field strength formula is E=kQ/r^2
units?

A
  • E: electric field strength, N/C
  • Q: charge, C
  • r: distance btwn masses
  • k: coulombs constant
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17
Q

wht is electric field similar to?

A

gravitational field

18
Q

wht does density of field lines show?

A

strength of electric field

19
Q

do electric field lines ever cross?

20
Q

what’s the direction of electric field lines?

A
  • start at positive, end at negative
  • out of +
  • into -
21
Q

are field lines curved or jagged?

22
Q

relationship btwn electric field and plate charge/unit area, q, in parallel plates

A

E is proportional to q
- unless plates attached to battery

23
Q

how would moving parallel plates further apart impact the electric field intensity?

A
  • does nothing
  • only plate charge/unit area impacts intensity
24
Q

how to find electric force when given a known field?

A

F = qE
- if q is negative, it acts in opposite direction. so plug in -‘ves here!

25
nC to C
divide by 10^9
26
µC to C
divide by 10^6
27
work when forces are repulsive vs attractive
- both positive: work brings charges together - opposite charge: work pulls charges apart
28
how is work stored between q1 and q2?
as electrical potential energy
29
what is work equal to?
- change in electric potential energy - W=Kq1q2/r = EE - include charge signs here
30
units of work
J
31
what is voltage?
Q - electric potential due to a single point - potential energy per unit positive charge at any point in space due to single point charge Q
32
formula to find potential bc of voltage at r? what kind of quantity is this? relationship in it?
V=KQ/r - scalar quantity - if Q>0, V>0 - if Q<0, V<0
33
equipotential surfaces
- every surface has same surface potential - electrical potential constant at given radius from Q - creates spherical surfaces where potential is constant - no work is done to move charges around on equipotential surfaces
34
how do u find the total potential at a point where several charges are there?
V(t) = V1 + V2 + V3... - scalar - account for signs
35
electron/proton symbol
e- and e+
36
charge on electron/protons
e = 1.602 x 10^-19
37
formula for finding charge on object based on number of changes gained/lost
q = ne - e: charge - n: number of them
38
when electrons experience uniform force in uniform electric fields, wht happens
uniform acceleration
39
what can uniform electric fields be used for?
- change speed of charged particle - deflect particle
40
charge of electrons/protons
1.6 x 10^-19