Gravitational and Electric Fields (Unit 4) Flashcards

(33 cards)

1
Q

Newton’s Law of Gravity

A

an attractive force between two point masses

proportional to the product of their masses and inversely proportional to their separation squared

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2
Q

Concept of a force field

A

the region in which a body experiences a force

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3
Q

Representation of gravitational field lines (radial and uniform fields)

A

See sheet

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4
Q

Equipotential

A

Line joining points of equal potential

No work is done moving an object along an equipotential

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5
Q

Gravitational field strength, g

A

the force acting per unit mass

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6
Q

Gravitational field strength units

A

N kg-1 VECTOR

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7
Q

Gravitational potential, V, (at a point)

A

work done per unit mass to move a small mass from infinity to that point.

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8
Q

Units of gravitational potential

A

J kg-1 SCALAR

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9
Q

Gravitational potential, V, at infinity

A

zero

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10
Q

Gravitational potential difference, V, between two points

A

work done per unit mass to move a small mass from one point to the other.

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11
Q

Graphical variation of magnitude of g with r

A

See sheet

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12
Q

Graphical variation of V with r

A

See sheet

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13
Q

Area under graph of gravitational field strength against r

A

work done moving a unit mass between the two points

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14
Q

Gradient of graph of gravitational potential against r

A

gradient = -g (gravitational field strength); g= -(deltaV/delta r)

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15
Q

Derivation of Kepler’s Law

A
  1. Gravitational force = centripetal force
  2. GMm/r2 = mv2/r or GMm/r2 = mr(omega)2
  3. substitute for v (v = (2pi x r)/T) or omega( omega = (2pi)/T)
  4. re-arrange to get T2 = ((4pi2)/GM) x r3
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16
Q

Energy considerations of an orbiting satellite

A

Total satellite energy = kinetic energy + grav. potential energy
Total satellite energy = 1/2mv2 - GMm/r

17
Q

Features of a geosynchronous orbit

A
  1. orbits over equator
  2. maintains a fixed position relative to surface of Earth
  3. period is 24 hours (same as the Earth)
  4. offers uninterrupted communication between transmitter and receiver
  5. steerable dish is unnecessary
18
Q

Escape velocity of an object from a planet

A

loss of kinetic energy = gain in grav. potential energy
(to get to infinity, need to provide grav. potential energy)
= 1/2mv(escape)2 - GMm/r
gives v(escape) = Square root of 2GM/r

19
Q

Coulomb’s Law

A

magnitude of force between two point charges
is proportional to the product of their charge and inversely proportional to their separation squared
the force is ATTRACTIVE with un-like charges and REPULSIVE with like charges.

20
Q

Representations of electric field lines

21
Q

Electric field strength, E

A

force acting per unit charge on a positive charge.

22
Q

Electric field strength units

A

N C-1 or V m-1 VECTOR

23
Q

Electric potential, V, (at a point)

A

work done to move a small unit positive charge from infinity to the point

24
Q

Units of electric potential, V

A

J C-1 or V (Volts) SCALAR

25
Electric potential, V, at infinity
Zero
26
Electric potential difference, V, between two points
work done to move a small unit positive charge from one point to the other.
27
Graphical variations of E with r (radial and uniform fields)
See sheet
28
Graphical variations of V with r (radial and uniform fields)
See sheet
29
Area under graph of electric field strength against r
See sheet
30
Path of charged particle in a uniform electric field
Path is parabolic, because, | Magnitude of force is constant and always in the same direction
31
Speed of charged particle accelerated across a potential difference, V
Loss of electrical potential energy = gain in kinetic energy QV = 1/2mv2
32
Similarities between electric and gravitational fields
field strengths are both inversely proportional to separation squared potentials are both inversely proportional to separation (see table on Pg 89 of A2 text book.)
33
Differences between electric and gravitational fields
masses always attract but charges may attract or repel | see table on Pg 89 of A2 text book