Chapters 4-6 Exam Sheet
What to include when solving problems
Reference frame
Picture
List given variables
List what you need to find
Pure equations (no substitutions)
Step by step solutions
Units
Show unit cancelations
New Variables
Variable | Meaning | Vector or Scalar | Units |
---|---|---|---|
F | Force | Vector | N |
ΣF | Net force | Vector | N |
FN | Normal force | Vector | N |
N | Newton | Vector | 1 N = s2kg⋅m |
r | Distance | Scalar | m |
G | Universal gravity constant | Scalar | 6.673×10−11kg2Nm2 |
W | Weight | Vector | N |
fsMAX | Maximum static friction | Vector | N |
fs | Static friction | Vector | N |
μs | Coefficient of static friction | Scalar | None |
fk | Kinetic friction | Vector | N |
μs | Coefficient of kinetic friction | Scalar | None |
T | Tension | Vector | N |
vc | Uniform circular motion velocity | Vector | m/s |
T | Period | Scalar | s |
ac | Centripetal acceleration | Vector | m/s² |
Fc | Centripetal force | Vector | N |
W | Work | Scalar | J |
KE | Kinetic energy | Scalar | J |
PE | Potential energy | Scalar | J |
Wc | Conservative work | Scalar | J |
Wnc | Nonconservative work | Scalar | J |
P | Average Power | Scalar | W |
N = Newton, J = joule, W = watt
Chapter 4: Forces and Newton’s Laws of Motion
Newton’s Three Laws of Motion
Newton’s 1st Law - An object in motion stays in motion or an object at rest stays at rest unless an external force is applied.
Newton’s 2nd Law - The net force on an object is equal to the object's mass multiplied by its acceleration: F=ma (F=max or F=may)
Newton’s 3rd Law - For action action there is an equal and opposite reaction.
Forces
Force (N) - a push or pull required to change the state of motion of an object
SI unit for force = Newton (N)
Newton = s2kg⋅m
kgN=s2m
Net force - vector sum of all forces acting on an object.
If no net force acts on an object, the object’s velocity can not change and the object can not accelerate.
Inertia - The natural tendency of an object to remain at rest or in motion at a constant speed along a straight line. Resistance to a change in velocity.
Inertial reference frame - non-accelerating frames of reference.
All accelerating reference reference frames are non-inertial.
Free Body Diagrams
Free body diagrams - represents the object and the forces that act on it, object is usually represented by a dot.
Weight
Weight: W=mg
Always acts downwards towards center of body.
Newton’s Law of Universal Gravitation
Every particle in the universe exerts an attractive force on every other particle.
For two particles, which have masses m1 and m2 and are separated by a distance r, the force that the particles, and has a magnitude given by:
F=Gr2m1m2
Universal gravitational constant: G = 6.67259× 10-11 kg2Nm2
Inverse square law: The inverse square law states that a physical quantity decreases as the square of the distance ( r ) from a source increases.
Mass of the earth: W=Gr2MEm
Normal Force
Normal force - the component of a contact force that is perpendicular to the surface that an object contacts, magnitude of the normal force indicates how hard the two objects press against each other.
If an object is resting on a surface, there are no vertical forces acting on them. The magnitudes of these two forces are equal.
Apparent Weight
Apparent weight of an object is the reading of a scale.
FN=mg+ma
Static and Kinetic Friction
Friction is always the opposite direction of motion and is parallel to the surface.
Static friction - frictional force resists force that is applied to an object, object remains at rest until the force of static friction is overcome.
Maximum static friction - the force just before breakaway (right before object starts moving).
fsMAX=μs⋅FN
Kinetic friction - force that acted between moving surfaces.
fk=μk⋅FN
0≤μk is the coefficient of kinetic friction.
Three Main Characteristics of Kinetic Frictional Force
It is independent of the apparent area of contact between the surfaces
It is independent of the speed of the sliding motion, if the speed is small.
The magnitude of the kinetic frictional force is proportional to the magnitude of the normal force.
Tension
Cables and ropes transmit forces through tension.
Equilibrium and Nonequilibrium
Equilibrium - the lack of change in the velocity of an object (the object is not accelerating).
ZERO ACCELERATION (∑Fx=0 or ∑Fy=0)
Velocity will not change.
Accelerating object = NOT in equilibrium. (∑Fx=max or ∑Fy=may)
When ΣF=0 , the net F will make the system accelerate, so its velocity WILL change. It will speed up, slow down, or stop.
Newton’s laws apply to objects whether or not they are in equilibrium.
The forces acting on an object in equilibrium must balance.
An object can be moving and still be in equilibrium if there is no acceleration.
Equilibrium
Parked car, objects moving at constant speed and not changing directions.
Non-Equilibrium
A car starting from a stop and moving straight through an intersection.
Accelerating.
A car making a right turn at constant speed.
There is a change in direction.
Chapter 5: Uniform Circular Motion
Uniform circular motion - the motion of an object traveling at a constant speed on a circular path (constant speed = uniform).
Equation for circular velocity: vc=T2πr
Speed (magnitude) is constant, direction is not constant, so velocity is not constant.
Revolution - a singular circular orbit of one body around a point.
Period - time it takes an object to travel once around a circle (to make one revolution).
Period(T)=frequency1
Frequency is the number of revolutions.
Circumference of a circle: 2πr (in meters)
Centripetal Acceleration
In uniform circular motion, speed is constant, but direction of the velocity vector is not constant.
Centripetal acceleration - directed towards the center of the circle; the same direction as the change is velocity
ac=rv2
Spinning an object in circular motion:
When the object is released, it will move along a straight path (Newton’s 1st law).
Once the object is released, there is no net force acting on it.
Centripetal Force
Centripetal force - the net force required to produce centripetal acceleration to keep an object moving in a circular path (newton’s second law).
Direction: ALWAYS towards the center of the circle, continually changes direction as the object moves.
There are two ways to write this equation:
Fc=mac or Fc=rmv2
The second equation inserts the centripetal acceleration equation.
Satellites in Circular Motion
There is only one speed and period that a satellite can have if the satellite is to remain in an orbit with a fixed radius. When something is in orbit, gravity is the centripetal force.
The speed of a satellite: v=rGME
The period of a satellite:T=GME2πr23
Universal gravitation constant: G = 6.67×10−11kg2Nm2
Apparent Weightlessness and Artificial Gravity
Apparent Weightlessness - occurs when an object is falling freely under the influence of gravity, giving the sensation of weightlessness.
Artificial Gravity - a concept of simulating gravity through centrifugal force or acceleration to create a gravitational effect in space or other environments.
Chapter 6: Work and Energy
Work is a force applied over a distance (force x displacement)
W=Fs
W=Fcosθs
The Joule: 1N⋅m=1joule(J)
When a force is PARALLEL to the displacement, the work by the force is POSITIVE.
When a force is OPPOSITE to the displacement, the work done by the force is NEGATIVE.
When the force is PERPENDICULAR to the displacement, the work done by the force is ZERO.
Work Energy Theorem
Kinetic energy (KE) of an object with mass m and speed v. Energy in motion.
KE=21mv2
KE will always be positive because mass can not be negative and v² is always positive.
Work-energy theorem - the net work done by the forces on an object equals the change in its kinetic energy. When a net external force does work on an object, the kinetic energy of the object changes by the amount of work done on it:
W=KEf−KE0
Gravitational Potential Energy
Potential energy (PE) - stored energy
PE=mgh
Gravitational potential energy - the energy that an object of mass m has by virtue of its position relative to the surface of the earth.
Wgravity=mg(h0−hf)
Potential and Kinetic energy
When your PE is at maximum, your KE is zero.
When your PE is zero, your KE is at maximum.
Conservative vs Nonconservative Forces
The gravitational force is called a conservative force and occurs when:
The work it does on a moving object is independent of the path between the object’s initial and final positions.
It does no work on an object moving around a closed path, starting and finishing at the same point.
The total mechanical energy of the system remains constant if only conservative forces are acting on it.
When a path has the same starting and ending point, it is called a closed path.
For a closed path, the work done by gravity will equal zero joules.
Wgravity = 0 J for a closed path.
Working Together
When conservative forces and nonconservative forces act simultaneously on an object, we can write work as:
W=Wc+Wnc
Conservative vs Nonconservative Table
The gravitational force is called a conservative force and occurs when:
The work it does on a moving object is independent of the path between the object’s initial and final positions.
It does no work on an object moving around a closed path, starting and finishing at the same point.
The total mechanical energy (kinetic energy + potential energy) of the system remains constant if only conservative forces are acting on it.
Closed path - when a path has the same starting and ending point
Work done by gravity => Wgravity = 0 J for a closed path.
Working Together
When conservative forces and nonconservative forces act simultaneously on an object, we can write work as: W=Wc+Wnc
Conservative vs Nonconservative Table
Conservative | Nonconservative |
---|---|
Work done is independent of path. | Work done is path dependent. |
Mechanical energy is conserved. | Mechanical energy is not conserved. |
The work done in a closed path is zero. | The work done in a closed loop may not be zero. |
PE can be identified. | PE can not be defined. |
The force is independent of the velocity of an object. | The force depends on the positions and velocities of the objects. |
Examples: gravity (does no work on an object), spring | Examples: friction, tension, air resistance, normal force |
The Conservation of Mechanical Energy
If the net work on an object by nonconservative forces is zero, then its energy does not change.
Conservation of energy: Ef=E0 OR 21mvf2+mghf=21mv02+mgh0
Total mechanical energy: E=KE+PE
The total mechanical energy of an object remains constant as the object moves, provided that the net work done by external nonconservative forces is zero.
Nonconservative Forces and the Work-Energy Theorem
Most moving objects experience nonconservative forces, such as friction, air resistance, and propulsive forces, and the work Wnc done by the net external nonconservative force is not zero. In these situations, the difference between the final and initial total mechanical energies is equal Wnc. Can be written in two ways:
Wnc=Ef−E0
Wnc=(mghf+21mvf2)−(mgh0+21mv02)
Power
Average power (P) is the time rate at which work is done.
P=tW
W is also equal Fs, s/t is equal to v, can be written asP=Fv
SI Unit: watt (W) aka joule/s
The work–energy theorem relates the work done by a net external force to the change in the energy of the object.
We can also define average power as the rate at which the energy is changing, or as the change in energy/time during which the change occurs.
1 horsepower = 550ft⋅lbs/sec = 745.7 watts
The Principle of Conservation of Energy
Energy can neither be created nor destroyed, but can only be converted from one form to another.
Extra
Average speed - how fast something travels over a certain distance: distance/elapsed time
Average velocity - how fast an object’s position changes over time: v=ΔtΔx
Average acceleration - rate at which an object’s velocity changes over a period of time: a=ΔtΔv
Speed vs. Velocity vs. Acceleration
Speed: How fast you're going, like on a speedometer. It's just a number, no direction.
Velocity: Speed with direction. It's how fast you're going and in which direction.
Acceleration: Changes in velocity. Speeding up, slowing down, or changing direction.
Velocity and Acceleration
Velocity, no acceleration = constant velocity
Velocity with acceleration = speeds up as it moves
When acceleration and velocity have opposite directions, the object slows down and decelerates.
Kinematic Equations
v=v0+at
x=21(v+v0)t
x=v0t+21at2
v2=v02+2ax
Chapters 4-6 Exam Sheet
What to include when solving problems
Reference frame
Picture
List given variables
List what you need to find
Pure equations (no substitutions)
Step by step solutions
Units
Show unit cancelations
New Variables
Variable | Meaning | Vector or Scalar | Units |
---|---|---|---|
F | Force | Vector | N |
ΣF | Net force | Vector | N |
FN | Normal force | Vector | N |
N | Newton | Vector | 1 N = s2kg⋅m |
r | Distance | Scalar | m |
G | Universal gravity constant | Scalar | 6.673×10−11kg2Nm2 |
W | Weight | Vector | N |
fsMAX | Maximum static friction | Vector | N |
fs | Static friction | Vector | N |
μs | Coefficient of static friction | Scalar | None |
fk | Kinetic friction | Vector | N |
μs | Coefficient of kinetic friction | Scalar | None |
T | Tension | Vector | N |
vc | Uniform circular motion velocity | Vector | m/s |
T | Period | Scalar | s |
ac | Centripetal acceleration | Vector | m/s² |
Fc | Centripetal force | Vector | N |
W | Work | Scalar | J |
KE | Kinetic energy | Scalar | J |
PE | Potential energy | Scalar | J |
Wc | Conservative work | Scalar | J |
Wnc | Nonconservative work | Scalar | J |
P | Average Power | Scalar | W |
N = Newton, J = joule, W = watt
Chapter 4: Forces and Newton’s Laws of Motion
Newton’s Three Laws of Motion
Newton’s 1st Law - An object in motion stays in motion or an object at rest stays at rest unless an external force is applied.
Newton’s 2nd Law - The net force on an object is equal to the object's mass multiplied by its acceleration: F=ma (F=max or F=may)
Newton’s 3rd Law - For action action there is an equal and opposite reaction.
Forces
Force (N) - a push or pull required to change the state of motion of an object
SI unit for force = Newton (N)
Newton = s2kg⋅m
kgN=s2m
Net force - vector sum of all forces acting on an object.
If no net force acts on an object, the object’s velocity can not change and the object can not accelerate.
Inertia - The natural tendency of an object to remain at rest or in motion at a constant speed along a straight line. Resistance to a change in velocity.
Inertial reference frame - non-accelerating frames of reference.
All accelerating reference reference frames are non-inertial.
Free Body Diagrams
Free body diagrams - represents the object and the forces that act on it, object is usually represented by a dot.
Weight
Weight: W=mg
Always acts downwards towards center of body.
Newton’s Law of Universal Gravitation
Every particle in the universe exerts an attractive force on every other particle.
For two particles, which have masses m1 and m2 and are separated by a distance r, the force that the particles, and has a magnitude given by:
F=Gr2m1m2
Universal gravitational constant: G = 6.67259× 10-11 kg2Nm2
Inverse square law: The inverse square law states that a physical quantity decreases as the square of the distance ( r ) from a source increases.
Mass of the earth: W=Gr2MEm
Normal Force
Normal force - the component of a contact force that is perpendicular to the surface that an object contacts, magnitude of the normal force indicates how hard the two objects press against each other.
If an object is resting on a surface, there are no vertical forces acting on them. The magnitudes of these two forces are equal.
Apparent Weight
Apparent weight of an object is the reading of a scale.
FN=mg+ma
Static and Kinetic Friction
Friction is always the opposite direction of motion and is parallel to the surface.
Static friction - frictional force resists force that is applied to an object, object remains at rest until the force of static friction is overcome.
Maximum static friction - the force just before breakaway (right before object starts moving).
fsMAX=μs⋅FN
Kinetic friction - force that acted between moving surfaces.
fk=μk⋅FN
0≤μk is the coefficient of kinetic friction.
Three Main Characteristics of Kinetic Frictional Force
It is independent of the apparent area of contact between the surfaces
It is independent of the speed of the sliding motion, if the speed is small.
The magnitude of the kinetic frictional force is proportional to the magnitude of the normal force.
Tension
Cables and ropes transmit forces through tension.
Equilibrium and Nonequilibrium
Equilibrium - the lack of change in the velocity of an object (the object is not accelerating).
ZERO ACCELERATION (∑Fx=0 or ∑Fy=0)
Velocity will not change.
Accelerating object = NOT in equilibrium. (∑Fx=max or ∑Fy=may)
When ΣF=0 , the net F will make the system accelerate, so its velocity WILL change. It will speed up, slow down, or stop.
Newton’s laws apply to objects whether or not they are in equilibrium.
The forces acting on an object in equilibrium must balance.
An object can be moving and still be in equilibrium if there is no acceleration.
Equilibrium
Parked car, objects moving at constant speed and not changing directions.
Non-Equilibrium
A car starting from a stop and moving straight through an intersection.
Accelerating.
A car making a right turn at constant speed.
There is a change in direction.
Chapter 5: Uniform Circular Motion
Uniform circular motion - the motion of an object traveling at a constant speed on a circular path (constant speed = uniform).
Equation for circular velocity: vc=T2πr
Speed (magnitude) is constant, direction is not constant, so velocity is not constant.
Revolution - a singular circular orbit of one body around a point.
Period - time it takes an object to travel once around a circle (to make one revolution).
Period(T)=frequency1
Frequency is the number of revolutions.
Circumference of a circle: 2πr (in meters)
Centripetal Acceleration
In uniform circular motion, speed is constant, but direction of the velocity vector is not constant.
Centripetal acceleration - directed towards the center of the circle; the same direction as the change is velocity
ac=rv2
Spinning an object in circular motion:
When the object is released, it will move along a straight path (Newton’s 1st law).
Once the object is released, there is no net force acting on it.
Centripetal Force
Centripetal force - the net force required to produce centripetal acceleration to keep an object moving in a circular path (newton’s second law).
Direction: ALWAYS towards the center of the circle, continually changes direction as the object moves.
There are two ways to write this equation:
Fc=mac or Fc=rmv2
The second equation inserts the centripetal acceleration equation.
Satellites in Circular Motion
There is only one speed and period that a satellite can have if the satellite is to remain in an orbit with a fixed radius. When something is in orbit, gravity is the centripetal force.
The speed of a satellite: v=rGME
The period of a satellite:T=GME2πr23
Universal gravitation constant: G = 6.67×10−11kg2Nm2
Apparent Weightlessness and Artificial Gravity
Apparent Weightlessness - occurs when an object is falling freely under the influence of gravity, giving the sensation of weightlessness.
Artificial Gravity - a concept of simulating gravity through centrifugal force or acceleration to create a gravitational effect in space or other environments.
Chapter 6: Work and Energy
Work is a force applied over a distance (force x displacement)
W=Fs
W=Fcosθs
The Joule: 1N⋅m=1joule(J)
When a force is PARALLEL to the displacement, the work by the force is POSITIVE.
When a force is OPPOSITE to the displacement, the work done by the force is NEGATIVE.
When the force is PERPENDICULAR to the displacement, the work done by the force is ZERO.
Work Energy Theorem
Kinetic energy (KE) of an object with mass m and speed v. Energy in motion.
KE=21mv2
KE will always be positive because mass can not be negative and v² is always positive.
Work-energy theorem - the net work done by the forces on an object equals the change in its kinetic energy. When a net external force does work on an object, the kinetic energy of the object changes by the amount of work done on it:
W=KEf−KE0
Gravitational Potential Energy
Potential energy (PE) - stored energy
PE=mgh
Gravitational potential energy - the energy that an object of mass m has by virtue of its position relative to the surface of the earth.
Wgravity=mg(h0−hf)
Potential and Kinetic energy
When your PE is at maximum, your KE is zero.
When your PE is zero, your KE is at maximum.
Conservative vs Nonconservative Forces
The gravitational force is called a conservative force and occurs when:
The work it does on a moving object is independent of the path between the object’s initial and final positions.
It does no work on an object moving around a closed path, starting and finishing at the same point.
The total mechanical energy of the system remains constant if only conservative forces are acting on it.
When a path has the same starting and ending point, it is called a closed path.
For a closed path, the work done by gravity will equal zero joules.
Wgravity = 0 J for a closed path.
Working Together
When conservative forces and nonconservative forces act simultaneously on an object, we can write work as:
W=Wc+Wnc
Conservative vs Nonconservative Table
The gravitational force is called a conservative force and occurs when:
The work it does on a moving object is independent of the path between the object’s initial and final positions.
It does no work on an object moving around a closed path, starting and finishing at the same point.
The total mechanical energy (kinetic energy + potential energy) of the system remains constant if only conservative forces are acting on it.
Closed path - when a path has the same starting and ending point
Work done by gravity => Wgravity = 0 J for a closed path.
Working Together
When conservative forces and nonconservative forces act simultaneously on an object, we can write work as: W=Wc+Wnc
Conservative vs Nonconservative Table
Conservative | Nonconservative |
---|---|
Work done is independent of path. | Work done is path dependent. |
Mechanical energy is conserved. | Mechanical energy is not conserved. |
The work done in a closed path is zero. | The work done in a closed loop may not be zero. |
PE can be identified. | PE can not be defined. |
The force is independent of the velocity of an object. | The force depends on the positions and velocities of the objects. |
Examples: gravity (does no work on an object), spring | Examples: friction, tension, air resistance, normal force |
The Conservation of Mechanical Energy
If the net work on an object by nonconservative forces is zero, then its energy does not change.
Conservation of energy: Ef=E0 OR 21mvf2+mghf=21mv02+mgh0
Total mechanical energy: E=KE+PE
The total mechanical energy of an object remains constant as the object moves, provided that the net work done by external nonconservative forces is zero.
Nonconservative Forces and the Work-Energy Theorem
Most moving objects experience nonconservative forces, such as friction, air resistance, and propulsive forces, and the work Wnc done by the net external nonconservative force is not zero. In these situations, the difference between the final and initial total mechanical energies is equal Wnc. Can be written in two ways:
Wnc=Ef−E0
Wnc=(mghf+21mvf2)−(mgh0+21mv02)
Power
Average power (P) is the time rate at which work is done.
P=tW
W is also equal Fs, s/t is equal to v, can be written asP=Fv
SI Unit: watt (W) aka joule/s
The work–energy theorem relates the work done by a net external force to the change in the energy of the object.
We can also define average power as the rate at which the energy is changing, or as the change in energy/time during which the change occurs.
1 horsepower = 550ft⋅lbs/sec = 745.7 watts
The Principle of Conservation of Energy
Energy can neither be created nor destroyed, but can only be converted from one form to another.
Extra
Average speed - how fast something travels over a certain distance: distance/elapsed time
Average velocity - how fast an object’s position changes over time: v=ΔtΔx
Average acceleration - rate at which an object’s velocity changes over a period of time: a=ΔtΔv
Speed vs. Velocity vs. Acceleration
Speed: How fast you're going, like on a speedometer. It's just a number, no direction.
Velocity: Speed with direction. It's how fast you're going and in which direction.
Acceleration: Changes in velocity. Speeding up, slowing down, or changing direction.
Velocity and Acceleration
Velocity, no acceleration = constant velocity
Velocity with acceleration = speeds up as it moves
When acceleration and velocity have opposite directions, the object slows down and decelerates.
Kinematic Equations
v=v0+at
x=21(v+v0)t
x=v0t+21at2
v2=v02+2ax