3.7.2 Gravitational fields Flashcards

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1
Q

Properties of Gravity/Gravitational force

A
  • Acts on objects with mass
  • Always attractive
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2
Q

Newtons’s Laws of gravitation

A
  • Directly proportional to the product masses
  • Inversely proportional to the square of the distance between them
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3
Q

Gravitational Force Equation

A

F = (G * m1 * m2) / r²

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4
Q

Relationship between Mass and gravitational force

A

Larger masses exert greater gravitational force

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5
Q

Relationship between distance and gravitational force

A

Greater distance results in weaker gravitational force

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6
Q

Uniform Field

A
  • Same gravitational force everywhere
  • Represented by parallel, equally spaced field lines
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7
Q

Radial Field

A
  • Force varies with position
  • Field lines spread out as distance increases
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8
Q

Field Lines

A
  • Direction of force on mass
  • Closer lines indicate stronger force
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9
Q

Earth’s Gravitational Field

A
  • Radial in nature
  • Nearly uniform close to the surface
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10
Q

Gravitational Field Strength (g) (definition and variability)

A

Definition
* Force per unit mass exerted by a gravitational field

Variability
* Constant in uniform fields
Varies in radial fields

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11
Q

Formulas for Gravitational Field Strength

A

General Formula
* g = F / m

Radial Field Formula
* g = (G * M) / r²

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12
Q

Gravitational Potential

A
  • Work done per unit mass
  • Moving an object from infinity to a point
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13
Q

Gravitational potential at infinity

A

Zero

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14
Q

Is the Gravitational Potential positive or negative

A

Always negative due to energy release

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15
Q

Gravitational potential formula

A
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16
Q

Gravitational Potential Difference (ΔV)

A

Energy needed to move a unit mass between two points

17
Q

Gravitational Potential Difference (ΔV) equation

A
18
Q

Equipotential Surfaces

A
  • Surfaces of equal gravitational potential
  • Constant potential across the surface
  • No work done when moving along these surfaces
    * since gravitational potential difference = 0
red lines are equipotential surfaces
19
Q

V vs r relationship

A

gravitational potential(V) Inversely proportional to the distance between the centres of the two objects (r)

20
Q

1.

area under g vs r graph

A
  • gravitational potential difference
  • Typically shows a decrease as distance increases.
21
Q

Kepler’s Third Law

A

Square of orbital period (T) is directly proportional to the cube of radius (r)

22
Q

How would you derive the equation

A
  • Centripetal Force = Gravitational Force
  • Rearrangement to find velocity (v)
  • Substitute v² into gravitational equation
  • (4π² / GM) is a constant
23
Q

What is the total energy of a satellite

A
  • Kinetic Energy + Potential Energy
  • Constant total energy in orbit
24
Q

Escape velocity

A

Minimum velocity to escape gravitational field

24
Q

Synchronous Orbit

A

Orbital period equals rotational period of the planet

25
Q

Equation for escape velocity

A
26
Q

Geostationary Satellites

A
  • Specific type of synchronous orbit
  • Always above the same point on Earth
  • Useful for communication (TV, telephone)
26
Q

Calculating Geostationary Orbit

A