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Determining Satellite Speed, Forces, Frames, and Newton's Laws, Study notes of Physics

Various concepts related to the laws of motion, including the preparation of an astronaut docking with a satellite, the definition and classes of forces, inertial frames, and newton's first, second, and third laws. It includes examples and formulas for calculating satellite speed, time, and resultant forces.

Typology: Study notes

Pre 2010

Uploaded on 08/18/2009

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Chapter 5
The Laws of Motion
The astronaut orbiting the Earth in the Figure is
preparing to dock with a Westar VI satellite. The
satellite is in a circular orbit 700 km above the
Earth's surface, where the free-fall acceleration is
8.21 m/s2. Take the radius of the Earth as 6400
km. Determine the speed of the satellite.
Determine the time interval required to complete
one orbit around the Earth
answer: V =7630 m/s
time= 97.4 min
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Chapter 5

The Laws of Motion

The astronaut orbiting the Earth in the Figure is preparing to dock with a Westar VI satellite. The satellite is in a circular orbit 700 km above the Earth's surface, where the free-fall acceleration is 8.21 m/s^2. Take the radius of the Earth as 6400 km. Determine the speed of the satellite. Determine the time interval required to complete one orbit around the Earth

answer: V =7630 m/s time= 97.4 min

Force

l Forces are what cause any change in the

velocity of an object

l A force is that which causes an acceleration

l The net force is the vector sum of all the

forces acting on an object

l Also called total force, resultant force, or unbalanced force

Zero Net Force

l When the net force is equal to zero:

l The acceleration is equal to zero l The velocity is constant

l Equilibrium occurs when the net force is

equal to zero

l The object, if at rest, will remain at rest l If the object is moving, it will continue to move at a constant velocity

Inertial Frames

l Any reference frame that moves with constant velocity relative to an inertial frame is itself an inertial frame

l A reference frame that moves with constant velocity relative to the distant stars is the best approximation of an inertial frame l We can consider the Earth to be such an inertial frame although it has a small centripetal acceleration associated with its motion

Newton’s First Law –

Alternative Statement

l In the absence of external forces, when viewed from an inertial reference frame, an object at rest remains at rest and an object in motion continues in motion with a constant velocity l Newton’s First Law describes what happens in the absence of a force l Also tells us that when no force acts on an object, the acceleration of the object is zero

Inertia and Mass

l The tendency of an object to resist any

attempt to change its velocity is called inertia

l Mass is that property of an object that

specifies how much resistance an object

exhibits to changes in its velocity

More About Mass

l Mass is an inherent property of an object

l Mass is a scalar quantity

l The SI unit of mass is kg

Newton’s Second Law

l When viewed from an inertial frame, the

acceleration of an object is directly

proportional to the net force acting on it and

inversely proportional to its mass

l Force is the cause of change in motion, as measured by the acceleration

l Algebraically, Σ F = m a

  1. A 7.00 kg object undergoes an acceleration given by a = (2.00 i + 7.00 j ) m/s^2. Find the resultant force acting on it and the magnitude of the resultant force. answer: 14i + 49j N , |F|=51 N.

Force Examples

  1. An electron of mass 9.11x10-31^ kg has an initial speed of 4.00x10^5 m/s. It travels in a straight line, and its speed increases to 6.00x10^5 m/s in a distance of 4.00 cm. Assuming its acceleration is constant, determine the force exerted on the electron.

answer: 2.28x10-18^ N in the direction of motion.

More About Newton’s Second

Law

l Σ F is the net force

l This is the vector sum of all the forces acting on the object

l Newton’s Second Law can be expressed in

terms of components:

l Σ Fx = m ax l Σ Fy = m ay l Σ Fz = m az

Gravitational Force

l The gravitational force, F g , is the force that

the earth exerts on an object

l This force is directed toward the center of the

earth

l Its magnitude is called the weight of the

object

l Weight = | F g |= mg

Newton’s Third Law

l If two objects interact, the force F 12 exerted

by object 1 on object 2 is equal in magnitude

and opposite in direction to the force F 21

exerted by object 2 on object 1

l F 12 = - F 21

l Note on notation: F AB is the force exerted by A on B

Newton’s Third Law,

Alternative Statements

l Forces always occur in pairs

l A single isolated force cannot exist

l The action force is equal in magnitude to the reaction force and opposite in direction l One of the forces is the action force, the other is the reaction force l It doesn’t matter which is considered the action and which the reaction l The action and reaction forces must act on different objects and be of the same type

Action-Reaction Example

l The force F 12 exerted by object 1 on object 2 is equal in magnitude and opposite in direction to F 21 exerted by object 2 on object 1

l F 12 = - F 21

Free Body Diagram

l In a free body diagram, you want the forces acting on a particular object

l The normal force and the force of gravity are the forces that act on the monitor

Equilibrium, Example 1a

l A lamp is suspended from a chain of negligible mass l The forces acting on the lamp are l the force of gravity ( F g ) l the tension in the chain ( T ) l Equilibrium gives

Fy^ =^0 →^ T^ −^ Fg =^0^ T^ = Fg

Equilibrium, Example 1b

l The forces acting on the chain are T ’ and T ” l T ” is the force exerted by the ceiling l T ’ is the force exerted by the lamp l T ’ is the reaction force to T l Only T is in the free body diagram of the lamp, since T ’ and T ” do not act on the lamp

Equilibrium, Example 2a

l Example 5.

l Conceptualize the traffic light

l Categorize as an equilibrium problem l No movement, so acceleration is zero

Equilibrium, Example 2b

l Analyze l Need two free-body diagrams l Apply equilibrium equation to the light and find T 3 l Apply equilibrium equations to the knot and find T 1 and T 2