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Force Forces, Fields,Potential and Energy
Objective: TSW understand and apply the concepts gravitational force, fields, potential and energy.
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Gravitational Field: A property of space around a mass that causes forces on other masses. The Gravitational field strength at a point is the force per unit mass on a small mass placed at that point. F F F F g = the gravitational field The gravitational force is always in the same direction as the gravitational field The gravitational field is a vector. (Magnitude and direction)
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Equipotential lines: Lines along which the potential is the same.
Spacing between equipotential lines increases as the distance from the mass increases.
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Equipotential lines are like a topographical map
Click to view the Spin and tilt video
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The units for a gravitational field are N/kg
The gravitational Force = (The mass) x (The Gravitational Field) The units for a gravitational field are N/kg
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Let’s zoom in to our physics room:
Fg Constant Field
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Equipotential line Constant Field
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Example 1: Calculate the gravitational field 10000km from the earth, which has a mass of 6x1024kg and a radius of 6400km 10000km
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Example 2: Find the final velocity of a 4kg object starting from rest if it is accelerated 25meters through a constant gravitational field of 22N/kg? 4kg 25m Fg = mg = (4)(22) = 88N
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Example 2: Solving with energy
Find the final velocity of a 4kg object starting from rest if it is accelerated 25meters through a constant gravitational field of 22N/kg? 4kg 25m V = gh V = 0 J/kg
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The gravitational potential of a position r is given by:
Gravitational potential at a point in a gravitational field is the work done per unit mass in moving a small mass from infinity to that point r R The gravitational potential of a position r is given by: Notice r is not squared The gravitational potential at infinity is zero
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Gravitational potential energy at a point is the work done to move a mass from infinity to that point
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Graphically V (J/kg) r (m)
r (m) The slope (gradient) of the tangent line gives the field strength g. R 2R 3R R = The radius of the mass
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Example: With what velocity must a rocket be fired in order to escape the earth’s gravitational field? (Neglect air resistance)
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