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Chapter 3
 In chapter 2 we studied motion but not its cause.
 In this chapter we will look at both force and
motion – the cause and effect.
 We will consider Newton’s:
◦ Newton’s three laws of motion
◦ Newton’s law of universal gravitation
◦ Buoyancy and momentum
Intro
 Only 25 when he formulated most of his
discoveries in math and physics
 His book Mathematical Principles of Natural
Philosophy is considered to be the most important
publication in the history of Physics.
Intro
 Force – a vector quantity capable of producing
motion or a change in motion
◦ A force is capable of changing an object’s velocity and
thereby producing acceleration.
 A given force may not actually produce a change
in motion because other forces may serve to
balance or cancel the effect.
Section 3.1
Section 3.1
Equal in magnitude but in opposite directions.
Section 3.1
Net force to the right
 Aristotle considered the natural state of most
matter to be at rest.
 Galileo concluded that objects could naturally
remain in motion indefinitely.
 Newton’s 1st
Law of Motion – An object will remain
at rest or in uniform motion in a straight line unless
acted on by an external, unbalance force.
Section 3.2
 An object will remain at rest or in uniform motion
in a straight line unless acted on by an external,
unbalance force.
 Balanced forces have equal magnitude in
opposite directions
 An external force is a force applied to the entire
object or system.
Section 3.2
Photo Source: Copyright © Bobby H. Bammel. All rights reserved.
Section 3.2
Photo Source: Copyright © Bobby H. Bammel. All rights reserved.
Section 3.2
 Inertia - the natural tendency of an object to
remain in a state of rest or in uniform motion in a
straight line (first introduced by Galileo)
 Basically, objects tend to maintain their state of
motion and resist change.
 Newton went one step further and related an
object’s mass to its inertia.
◦ The greater the mass of an object, the greater its
inertia.
◦ The smaller the mass of an object, the less its inertia.
Section 3.2
The large man has more inertia – more force is necessary to
start him swinging and also to stop him – due to his greater
inertia
Section 3.2
Quickly pull the paper and the stack of quarters tend to stay in
place due to inertia.
Section 3.2
 Because of the relationship between motion and
inertia:
 Newton’s First Law of Motion is sometimes called
the Law of Inertia.
 Seatbelts help ‘correct’ for this law during sudden
changes in speed.
Section 3.2
 Acceleration (change in velocity) produced by a
force acting on an object is directly proportional to
the magnitude of the force (the greater the force
the greater the acceleration.)
 Acceleration of an object is inversely proportional
to the mass of the object (the greater the mass of
an object the smaller the acceleration.)
 a = F/m or F = ma
Section 3.3
Force
mass
• Acceleration α
b) If we double the
force we double the
acceleration.
c) If we double the
mass we half the
acceleration.
Section 3.3
a α F
m
a)Original situation
 “F” is the net force (unbalanced), which is likely
the vector sum of two or more forces.
 “m” & “a” are concerning the whole system
 Units
 Force = mass x acceleration = kg x m/s2
= N
 N = kg x m/s2
= newton -- this is a derived unit
and is the metric system (SI) unit of force
Section 3.3
 Forces are applied to blocks connected by a string
(weightless) resting on a frictionless surface. Mass
of each block = 1 kg; F1 = 5.0 N; F2 = 8.0 N
 What is the acceleration of the system?
Section 3.3
 Forces are applied to blocks connected by a string
(weightless) resting on a frictionless surface. Mass
of each block = 1 kg; F1 = 5.0 N; F2 = 8.0 N. What
is the acceleration of the system?
 GIVEN:
◦ m1 = 1 kg; m2 = 1 kg
◦ F1 = -5.0 N; F2 = 8.0 N
 a = ?
• a = = = = 1.5 m/s2
F Fnet 8.0 N – 5.0 N
m m1 + m2 1.0 kg + 1.0 kg
Section 3.3
 Mass = amount of matter present
 Weight = related to the force of gravity
 Earth: weight = mass x acc. due to gravity
 w = mg (special case of F = ma) Weight is a
force due to the pull of gravity.
 Therefore, one’s weight changes due to changing
pull of gravity – like between the earth and moon.
 Moon’s gravity is only 1/6th
that of earth’s.
Section 3.3
What is the weight of a 2.45 kg mass on (a) earth,
and (b) the moon?
Section 3.3
 What is the weight of a 2.45 kg mass on (a) earth,
and (b) the moon?
 Use Equation w =mg
 Earth: w = mg = (2.45 kg) (9.8 m/s2
) = 24.0 N (or
5.4 lb. Since 1 lb = 4.45 N)
 Moon: w = mg = (2.45 kg) [(9.8 m/s2
)/6] = 4.0 N
(or 0.9 lb.)
Section 3.3
Section 3.3
 Friction – resistance to relative motion that occurs
whenever two materials are in contact with each
other.
◦ Ever-present and found in all states (solids, liquids, and
gases) of matter
 In some cases we want to increase friction (sand
on ice), in other cases we want to reduce friction
(motor oil).
Section 3.3
 Static friction occurs when the frictional force is
sufficient to prevent relative motion between
surfaces
 Kinetic (or sliding) friction occurs when there is
relative motion between surfaces in contact.
 Kinetic friction is generally less than static friction
◦ Usually it takes less force to keep something moving
than to start it moving.
Section 3.3
 Coefficients of friction (µ) are dimensionless
quantities used to characterize particular contact
situations.
 Both, coefficients of static friction (µs) and
coefficients of kinetic friction (µk) are determined
experimentally for a wide range of contact
surfaces.
 Usually (µs) > (µk).
Section 3.3
Section 3.3
 For every action there is an equal and opposite
reaction.
or
 Whenever on object exerts a force on a second
object, the second object exerts an equal and
opposite force on the first object.
 action = opposite reaction
 F1 = -F2 or m1a1 = -m2a2
Section 3.4
 F1 = -F2 or m1a1 = -m2a2
 Jet propulsion – exhaust gases in one direction
and the rocket in the other direction
 Gravity – jump from a table and you will accelerate
to earth. In reality BOTH you and the earth are
accelerating towards each other
◦ You – small mass, huge acceleration (m1a1)
◦ Earth – huge mass, very small acceleration (-m2a2)
◦ BUT  m1a1 = -m2a2
Section 3.4
 Friction on the tires provides necessary centripetal acceleration.
 Passengers continue straight ahead in original direction and as car
turns the door comes toward passenger – 1st
Law
 As car turns you push against door and the door equally pushes
against you – 3rd
Law
Section 3.4
 Gravity is a fundamental force of nature
◦ We do not know what causes it
◦ We can only describe it
 Law of Universal Gravitation – Every particle in the
universe attracts every other particle with a force
that is directly proportional to the product of their
masses and inversely proportional to the square
of the distance between them
Section 3.5
 G is the universal gravitational constant
 G = 6.67 x 10-11
N.
m2
/kg2
 G:
◦ is a very small quantity
◦ thought to be valid throughout the universe
◦ was measured by Cavendish 70 years after Newton’s
death
◦ not equal to “g” and not a force
Section 3.5
Gm1m2
r2
• Equation form: F =
 The forces that attract particles together are equal and
opposite
 F1 = -F2 or m1a1 = -m2a2
Section 3.5
 For a homogeneous
sphere the gravitational
force acts as if all the
mass of the sphere were
at its center
Section 3.5
Gm1m2
r2
• F =
 Two objects with masses of 1.0 kg and 2.0 kg are
1.0 m apart. What is the magnitude of the
gravitational force between the masses?
Section 3.5
 Two objects with masses of 1.0 kg and 2.0 kg are
1.0 m apart. What is the magnitude of the
gravitational force between the masses?
Section 3.5
Gm1m2
r2
• F =
• F =
(6.67 x 10-11
N-m2
/kg2
)(1.0 kg)(2.0 kg)
(1.0 m)2
• F = 1.3 x 10-10
N
 ME and RE are the mass and radius of Earth
 This force is just the object’s weight (w = mg)
Section 3.5
GmME
R2
E
• F = [force of gravity on object of mass m]
• ∴ w = mg =
GmME
RE
2
GME
R2
E
• g =
• m cancels out ∴ g is independent of mass
Section 3.5
Photo Source: Standard HMCO copyright line
 Buoyant force – the upward force resulting from
an object being wholly or partially immersed in a
fluid.
 The Archimedes’ Principle – An object immersed
in a fluid experiences a buoyant force equal to the
weight of the volume of fluid displaced.
 Both liquids and gases are considered fluids.
Section 3.6
 The buoyant force depends on the weight of the
fluid displaced.
◦ The weight of the fluid displaced depends on the
density of the fluid and the volume displaced.
 Salt water is more dense than fresh water.
◦ Therefore, one floats higher in salt water, since one
needs to displace less salt water to equal one’s weight.
Section 3.6
 Ships float because the average density of the
ship is less than the water it would displace.
 Oil floats on water, since oil is less dense than
water
 Cream floats on milk, since cream is less dense
than milk.
 By taking in, or pumping out water, submarines
can vary their buoyancy.
Section 3.6
 Linear momentum = mass x velocity
 ρ = mv
 If we have a system of masses, the linear
momentum is the sum of all individual momentum
vectors.
 Pf = Pi (final = initial)
 P = ρ1 + ρ2 + ρ3 + … (sum of the individual
momentum vectors)
Section 3.7
 Law of Conservation of Linear Momentum - the
total linear momentum of an isolated system
remains the same if there is no external,
unbalanced force acting on the system
 Linear Momentum is ‘conserved’ as long as there
are no external unbalance forces.
◦ It does not change with time.
Section 3.7
 Pi = Pf = 0 (for man and boat)
 When the man jumps out of the boat he has momentum
in one direction and, therefore, so does the boat.
 Their momentums must cancel out! (= 0)
Section 3.7
 Two masses at rest on a frictionless surface. When the
string (weightless) is burned the two masses fly apart
due to the release of the compressed (internal) spring (v1
= 1.8 m/s).
Section 3.7
 Two masses at rest on a frictionless surface. When the
string (weightless) is burned the two masses fly apart
due to the release of the compressed (internal) spring (v1
= 1.8 m/s).
GIVEN:
• m1 = 1.0 kg
• m2 = 2.0 kg
• v1 = 1.8 m/s, v2 = ?
•Pf = Pi = 0
• Pf = ρ1 + ρ2 = 0
• ρ1 = -ρ2
•m1v1 = -m2v2
Section 3.7
m1v1
m2
(1.0 kg) (1.8 m/s)
2.0 kg
Section 3.7
m1v1 = -m2v2
 v2 = - = - = -0.90 m/s
 Jet Propulsion can be explained in terms of both
Newton’s 3rd
Law & Linear Momentum
 ρ1 = -ρ2  m1v1 = -m2v2
 The exhaust gas molecules have small m and
large v.
 The rocket has large m and smaller v.
 BUT  m1v1 = -m2v2 (momentum is conserved)
Section 3.7
 Torque – the twisting effect caused by one or
more forces
 As we have learned, the linear momentum of a
system can be changed by the introduction of an
external unbalanced force.
 Similarly, angular momentum can be changed by
an external unbalanced torque.
Section 3.7
 Torque is a
twisting
action that
produces
rotational
motion or a
change in
rotational
motion.
Section 3.7
 Torque varies with
the length of the
lever arm. As the
length of the lever
arm is doubled, the
torque is doubled, for
a given force.
Section 3.7
 Law of Conservation of Angular Momentum - the
angular momentum of an object remains constant
if there is no external, unbalanced torque (a force
about an axis) acting on it
Section 3.7
• Concerns objects that go in paths around a fixed
point, for example a satellite orbiting the earth
 L = mvr
 L = angular momentum, m = mass, v = velocity,
and r = distance to center of motion
 L1 = L2
 m1v1r1 = m2v2r2
Section 3.7
 Mass (m) is constant.
 As r changes so must v. When r decreases, v must
increase so that m1v1r1 = m2v2r2
Section 3.7
 In our solar system the planet’s orbit paths are slightly elliptical,
therefore both r and v will slightly vary during a complete orbit.
Section 3.7
 A comet at its farthest point from the Sun is 900
million miles, traveling at 6000 mi/h. What is its
speed at its closest point of 30 million miles away?
 EQUATION: m1v1r1 = m2v2r2
 GIVEN: v2, r2, r1, and m1 = m2
Section 3.7
• FIND: v1 = =
v2r2
r1
(6.0 x 103
mi/h) (900 x 106
mi)
30 x 106
mi
• 1.8 x 105
mi/h or 180,000 mi/h
Rotors on large helicopters rotate in the opposite direction
Section 3.7
 Figure Skater – she/he starts the spin with arms
out at one angular velocity. Simply by pulling the
arms in the skater spins faster, since the average
radial distance of the mass decreases.
 m1v1r1 = m2v2r2
 m is constant; r decreases;
 Therefore v increases
Section 3.7
 F = ma (2nd
Law) or w = mg (for weight)
 F1 = -F2 (3rd
Law)
 F = (Gm1m2)/r2
(Law of Gravitation)
 G = 6.67 x 10-11
N-m2
/kg2
(gravitational constant)
 g = GM/r2
(acc. of gravity, M=mass of sph. object)
 r = mv (linear momentum)
 Pf = Pi (conservation of linear momentum)
 L = mvr (angular momentum)
 L1= m1v1r1 = L2 = m2v2r2 (Cons. of ang. Mom.)
Review

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Sci 1010 chapter 3

  • 2.  In chapter 2 we studied motion but not its cause.  In this chapter we will look at both force and motion – the cause and effect.  We will consider Newton’s: ◦ Newton’s three laws of motion ◦ Newton’s law of universal gravitation ◦ Buoyancy and momentum Intro
  • 3.  Only 25 when he formulated most of his discoveries in math and physics  His book Mathematical Principles of Natural Philosophy is considered to be the most important publication in the history of Physics. Intro
  • 4.  Force – a vector quantity capable of producing motion or a change in motion ◦ A force is capable of changing an object’s velocity and thereby producing acceleration.  A given force may not actually produce a change in motion because other forces may serve to balance or cancel the effect. Section 3.1
  • 5. Section 3.1 Equal in magnitude but in opposite directions.
  • 6. Section 3.1 Net force to the right
  • 7.  Aristotle considered the natural state of most matter to be at rest.  Galileo concluded that objects could naturally remain in motion indefinitely.  Newton’s 1st Law of Motion – An object will remain at rest or in uniform motion in a straight line unless acted on by an external, unbalance force. Section 3.2
  • 8.  An object will remain at rest or in uniform motion in a straight line unless acted on by an external, unbalance force.  Balanced forces have equal magnitude in opposite directions  An external force is a force applied to the entire object or system. Section 3.2
  • 9. Photo Source: Copyright © Bobby H. Bammel. All rights reserved. Section 3.2
  • 10. Photo Source: Copyright © Bobby H. Bammel. All rights reserved. Section 3.2
  • 11.  Inertia - the natural tendency of an object to remain in a state of rest or in uniform motion in a straight line (first introduced by Galileo)  Basically, objects tend to maintain their state of motion and resist change.  Newton went one step further and related an object’s mass to its inertia. ◦ The greater the mass of an object, the greater its inertia. ◦ The smaller the mass of an object, the less its inertia. Section 3.2
  • 12. The large man has more inertia – more force is necessary to start him swinging and also to stop him – due to his greater inertia Section 3.2
  • 13. Quickly pull the paper and the stack of quarters tend to stay in place due to inertia. Section 3.2
  • 14.  Because of the relationship between motion and inertia:  Newton’s First Law of Motion is sometimes called the Law of Inertia.  Seatbelts help ‘correct’ for this law during sudden changes in speed. Section 3.2
  • 15.  Acceleration (change in velocity) produced by a force acting on an object is directly proportional to the magnitude of the force (the greater the force the greater the acceleration.)  Acceleration of an object is inversely proportional to the mass of the object (the greater the mass of an object the smaller the acceleration.)  a = F/m or F = ma Section 3.3 Force mass • Acceleration α
  • 16. b) If we double the force we double the acceleration. c) If we double the mass we half the acceleration. Section 3.3 a α F m a)Original situation
  • 17.  “F” is the net force (unbalanced), which is likely the vector sum of two or more forces.  “m” & “a” are concerning the whole system  Units  Force = mass x acceleration = kg x m/s2 = N  N = kg x m/s2 = newton -- this is a derived unit and is the metric system (SI) unit of force Section 3.3
  • 18.  Forces are applied to blocks connected by a string (weightless) resting on a frictionless surface. Mass of each block = 1 kg; F1 = 5.0 N; F2 = 8.0 N  What is the acceleration of the system? Section 3.3
  • 19.  Forces are applied to blocks connected by a string (weightless) resting on a frictionless surface. Mass of each block = 1 kg; F1 = 5.0 N; F2 = 8.0 N. What is the acceleration of the system?  GIVEN: ◦ m1 = 1 kg; m2 = 1 kg ◦ F1 = -5.0 N; F2 = 8.0 N  a = ? • a = = = = 1.5 m/s2 F Fnet 8.0 N – 5.0 N m m1 + m2 1.0 kg + 1.0 kg Section 3.3
  • 20.  Mass = amount of matter present  Weight = related to the force of gravity  Earth: weight = mass x acc. due to gravity  w = mg (special case of F = ma) Weight is a force due to the pull of gravity.  Therefore, one’s weight changes due to changing pull of gravity – like between the earth and moon.  Moon’s gravity is only 1/6th that of earth’s. Section 3.3
  • 21. What is the weight of a 2.45 kg mass on (a) earth, and (b) the moon? Section 3.3
  • 22.  What is the weight of a 2.45 kg mass on (a) earth, and (b) the moon?  Use Equation w =mg  Earth: w = mg = (2.45 kg) (9.8 m/s2 ) = 24.0 N (or 5.4 lb. Since 1 lb = 4.45 N)  Moon: w = mg = (2.45 kg) [(9.8 m/s2 )/6] = 4.0 N (or 0.9 lb.) Section 3.3
  • 24.  Friction – resistance to relative motion that occurs whenever two materials are in contact with each other. ◦ Ever-present and found in all states (solids, liquids, and gases) of matter  In some cases we want to increase friction (sand on ice), in other cases we want to reduce friction (motor oil). Section 3.3
  • 25.  Static friction occurs when the frictional force is sufficient to prevent relative motion between surfaces  Kinetic (or sliding) friction occurs when there is relative motion between surfaces in contact.  Kinetic friction is generally less than static friction ◦ Usually it takes less force to keep something moving than to start it moving. Section 3.3
  • 26.  Coefficients of friction (µ) are dimensionless quantities used to characterize particular contact situations.  Both, coefficients of static friction (µs) and coefficients of kinetic friction (µk) are determined experimentally for a wide range of contact surfaces.  Usually (µs) > (µk). Section 3.3
  • 28.  For every action there is an equal and opposite reaction. or  Whenever on object exerts a force on a second object, the second object exerts an equal and opposite force on the first object.  action = opposite reaction  F1 = -F2 or m1a1 = -m2a2 Section 3.4
  • 29.  F1 = -F2 or m1a1 = -m2a2  Jet propulsion – exhaust gases in one direction and the rocket in the other direction  Gravity – jump from a table and you will accelerate to earth. In reality BOTH you and the earth are accelerating towards each other ◦ You – small mass, huge acceleration (m1a1) ◦ Earth – huge mass, very small acceleration (-m2a2) ◦ BUT  m1a1 = -m2a2 Section 3.4
  • 30.  Friction on the tires provides necessary centripetal acceleration.  Passengers continue straight ahead in original direction and as car turns the door comes toward passenger – 1st Law  As car turns you push against door and the door equally pushes against you – 3rd Law Section 3.4
  • 31.  Gravity is a fundamental force of nature ◦ We do not know what causes it ◦ We can only describe it  Law of Universal Gravitation – Every particle in the universe attracts every other particle with a force that is directly proportional to the product of their masses and inversely proportional to the square of the distance between them Section 3.5
  • 32.  G is the universal gravitational constant  G = 6.67 x 10-11 N. m2 /kg2  G: ◦ is a very small quantity ◦ thought to be valid throughout the universe ◦ was measured by Cavendish 70 years after Newton’s death ◦ not equal to “g” and not a force Section 3.5 Gm1m2 r2 • Equation form: F =
  • 33.  The forces that attract particles together are equal and opposite  F1 = -F2 or m1a1 = -m2a2 Section 3.5
  • 34.  For a homogeneous sphere the gravitational force acts as if all the mass of the sphere were at its center Section 3.5 Gm1m2 r2 • F =
  • 35.  Two objects with masses of 1.0 kg and 2.0 kg are 1.0 m apart. What is the magnitude of the gravitational force between the masses? Section 3.5
  • 36.  Two objects with masses of 1.0 kg and 2.0 kg are 1.0 m apart. What is the magnitude of the gravitational force between the masses? Section 3.5 Gm1m2 r2 • F = • F = (6.67 x 10-11 N-m2 /kg2 )(1.0 kg)(2.0 kg) (1.0 m)2 • F = 1.3 x 10-10 N
  • 37.  ME and RE are the mass and radius of Earth  This force is just the object’s weight (w = mg) Section 3.5 GmME R2 E • F = [force of gravity on object of mass m] • ∴ w = mg = GmME RE 2 GME R2 E • g = • m cancels out ∴ g is independent of mass
  • 38. Section 3.5 Photo Source: Standard HMCO copyright line
  • 39.  Buoyant force – the upward force resulting from an object being wholly or partially immersed in a fluid.  The Archimedes’ Principle – An object immersed in a fluid experiences a buoyant force equal to the weight of the volume of fluid displaced.  Both liquids and gases are considered fluids. Section 3.6
  • 40.  The buoyant force depends on the weight of the fluid displaced. ◦ The weight of the fluid displaced depends on the density of the fluid and the volume displaced.  Salt water is more dense than fresh water. ◦ Therefore, one floats higher in salt water, since one needs to displace less salt water to equal one’s weight. Section 3.6
  • 41.  Ships float because the average density of the ship is less than the water it would displace.  Oil floats on water, since oil is less dense than water  Cream floats on milk, since cream is less dense than milk.  By taking in, or pumping out water, submarines can vary their buoyancy. Section 3.6
  • 42.  Linear momentum = mass x velocity  ρ = mv  If we have a system of masses, the linear momentum is the sum of all individual momentum vectors.  Pf = Pi (final = initial)  P = ρ1 + ρ2 + ρ3 + … (sum of the individual momentum vectors) Section 3.7
  • 43.  Law of Conservation of Linear Momentum - the total linear momentum of an isolated system remains the same if there is no external, unbalanced force acting on the system  Linear Momentum is ‘conserved’ as long as there are no external unbalance forces. ◦ It does not change with time. Section 3.7
  • 44.  Pi = Pf = 0 (for man and boat)  When the man jumps out of the boat he has momentum in one direction and, therefore, so does the boat.  Their momentums must cancel out! (= 0) Section 3.7
  • 45.  Two masses at rest on a frictionless surface. When the string (weightless) is burned the two masses fly apart due to the release of the compressed (internal) spring (v1 = 1.8 m/s). Section 3.7
  • 46.  Two masses at rest on a frictionless surface. When the string (weightless) is burned the two masses fly apart due to the release of the compressed (internal) spring (v1 = 1.8 m/s). GIVEN: • m1 = 1.0 kg • m2 = 2.0 kg • v1 = 1.8 m/s, v2 = ? •Pf = Pi = 0 • Pf = ρ1 + ρ2 = 0 • ρ1 = -ρ2 •m1v1 = -m2v2 Section 3.7
  • 47. m1v1 m2 (1.0 kg) (1.8 m/s) 2.0 kg Section 3.7 m1v1 = -m2v2  v2 = - = - = -0.90 m/s
  • 48.  Jet Propulsion can be explained in terms of both Newton’s 3rd Law & Linear Momentum  ρ1 = -ρ2  m1v1 = -m2v2  The exhaust gas molecules have small m and large v.  The rocket has large m and smaller v.  BUT  m1v1 = -m2v2 (momentum is conserved) Section 3.7
  • 49.  Torque – the twisting effect caused by one or more forces  As we have learned, the linear momentum of a system can be changed by the introduction of an external unbalanced force.  Similarly, angular momentum can be changed by an external unbalanced torque. Section 3.7
  • 50.  Torque is a twisting action that produces rotational motion or a change in rotational motion. Section 3.7
  • 51.  Torque varies with the length of the lever arm. As the length of the lever arm is doubled, the torque is doubled, for a given force. Section 3.7
  • 52.  Law of Conservation of Angular Momentum - the angular momentum of an object remains constant if there is no external, unbalanced torque (a force about an axis) acting on it Section 3.7 • Concerns objects that go in paths around a fixed point, for example a satellite orbiting the earth
  • 53.  L = mvr  L = angular momentum, m = mass, v = velocity, and r = distance to center of motion  L1 = L2  m1v1r1 = m2v2r2 Section 3.7
  • 54.  Mass (m) is constant.  As r changes so must v. When r decreases, v must increase so that m1v1r1 = m2v2r2 Section 3.7
  • 55.  In our solar system the planet’s orbit paths are slightly elliptical, therefore both r and v will slightly vary during a complete orbit. Section 3.7
  • 56.  A comet at its farthest point from the Sun is 900 million miles, traveling at 6000 mi/h. What is its speed at its closest point of 30 million miles away?  EQUATION: m1v1r1 = m2v2r2  GIVEN: v2, r2, r1, and m1 = m2 Section 3.7 • FIND: v1 = = v2r2 r1 (6.0 x 103 mi/h) (900 x 106 mi) 30 x 106 mi • 1.8 x 105 mi/h or 180,000 mi/h
  • 57. Rotors on large helicopters rotate in the opposite direction Section 3.7
  • 58.  Figure Skater – she/he starts the spin with arms out at one angular velocity. Simply by pulling the arms in the skater spins faster, since the average radial distance of the mass decreases.  m1v1r1 = m2v2r2  m is constant; r decreases;  Therefore v increases Section 3.7
  • 59.  F = ma (2nd Law) or w = mg (for weight)  F1 = -F2 (3rd Law)  F = (Gm1m2)/r2 (Law of Gravitation)  G = 6.67 x 10-11 N-m2 /kg2 (gravitational constant)  g = GM/r2 (acc. of gravity, M=mass of sph. object)  r = mv (linear momentum)  Pf = Pi (conservation of linear momentum)  L = mvr (angular momentum)  L1= m1v1r1 = L2 = m2v2r2 (Cons. of ang. Mom.) Review