Newtons Laws of Motion Newtons Laws Newtons First

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Newton’s Laws of Motion

Newton’s Laws of Motion

Newton’s Laws Ø Newton’s First Law • Law of Inertia Ø Newton’s Second Law

Newton’s Laws Ø Newton’s First Law • Law of Inertia Ø Newton’s Second Law • Ø Newton’s Third Law • Law of Action and Reaction Ø Law of Universal Gravitation •

Mass Ø …is the amount of “stuff” in an object. Ø …is measured in

Mass Ø …is the amount of “stuff” in an object. Ø …is measured in kilograms. Ø …is the measure of the inertia of an object. Ø Inertia is the natural tendency of a body resist changes in motion.

History of Inertia Ø Aristotle (384 -322 BCE): “…a constant force will yield a

History of Inertia Ø Aristotle (384 -322 BCE): “…a constant force will yield a constant speed. ” Ø Jean Buridan (1300 -1358): believed that objects stayed in motion because they possessed “impetus” – something inside that makes them continue to move. Ø Galileo Galilei (1564 -1642): challenged the commonly held belief that an object’s motion was the result of continued force. Instead, he viewed uniform motion as being a state just as natural as rest. OK!

Galileo’s Thought Experiments on Motion Ball drop from leaning tower of Pisa Ø Galileo’s

Galileo’s Thought Experiments on Motion Ball drop from leaning tower of Pisa Ø Galileo’s Inclined Planes Ø

Force Ø …is a push or pull that changes the velocity of an object.

Force Ø …is a push or pull that changes the velocity of an object. Ø …is a vector quantity. Ø. . . measured in Newtons.

Newton’s First Law of Inertia Ø “A body remains at rest or moves in

Newton’s First Law of Inertia Ø “A body remains at rest or moves in a straight line at a constant speed unless acted upon by a force. ” Ø The more massive the object, the greater the tendency to keep doing what it is already doing. Ø

Newton’s First Law Ø No mention of chemical composition Ø No mention of terrestrial

Newton’s First Law Ø No mention of chemical composition Ø No mention of terrestrial or celestial realms Ø Net force required when object changes motion Ø Acceleration is the observable consequence of forces acting

Newton’s Second Law The Sum of the Forces acting on a body is proportional

Newton’s Second Law The Sum of the Forces acting on a body is proportional to the acceleration that the body experiences SF a S F = (mass) a

Net Force

Net Force

Newton’s Third Law Ø Action-Reaction Ø For every action force there is an equal

Newton’s Third Law Ø Action-Reaction Ø For every action force there is an equal and opposite reaction force

The Law of Gravity Every mass exerts a force of attraction on every other

The Law of Gravity Every mass exerts a force of attraction on every other mass. Ø The math… Ø FG = 6. 67 10 -11 N·m 2/kg 2

Gravity Questions Ø Did the Moon exert a gravitational force on the Apollo astronauts?

Gravity Questions Ø Did the Moon exert a gravitational force on the Apollo astronauts? Ø What kind of objects can exert a gravitational force on other objects?

Gravity Questions Ø The constant G is a rather small number. What kind of

Gravity Questions Ø The constant G is a rather small number. What kind of objects can exert strong gravitational forces? Ø If the distance between two objects in space is doubled, then what happens to the gravitational force between them?

Weight Ø The weight of an object Fg is the gravitational force acting downward

Weight Ø The weight of an object Fg is the gravitational force acting downward on the object. Ø Fg = m g

Tension (Tensile Force) Ø Tension is the force in a string, chain or tendon

Tension (Tensile Force) Ø Tension is the force in a string, chain or tendon that is applied tending to stretch it. Ø FT

Normal Force Ø The normal force on an object that is being supported by

Normal Force Ø The normal force on an object that is being supported by a surface is the component of the supporting force that is perpendicular to the surface. Ø FN

Coefficient of Friction F Kinetic Friction • F f = m k. F N

Coefficient of Friction F Kinetic Friction • F f = m k. F N Ø Static Friction • F f m s. F N Ø In most cases, mk < ms.

On to problems. . .

On to problems. . .