Phy 211: General Physics I Chapter 5: Force & Motion I Lecture Notes.

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Phy 211: General Physics I Chapter 5: Force & Motion I Lecture Notes

Sir Isaac Newton ( ) Co-invented the “calculus” (along with Gottfried Wilhelm Leibnitz) Among his accomplishments included theories of: –Light & Optics –Heat & Cooling Established 3 Laws of Motion Proposed the Law of Universal Gravitation (to settle a parlor bet) –The bet was actually between Edward Haley & Robert Hooke –This theory successfully explained planetary motion and elliptical orbits

Newton’s 1 st Law Every object continues in its state of rest, or of motion unless compelled to change that state by forces impressed upon it. Also known as the “Law of Inertia” Key Points: –When an object is moving in uniform motion it has no net force acting on it –When there is no force acting on an object, it will stay at rest or maintain its constant speed in a straight line –Or simply put, Nature is lazy!

Newton’s 2 nd Law When a net force is exerted on an object its velocity will change: The time rate of change of motion (acceleration) is related to: –Proportional to the size of the net force –Inversely proportional to the mass of the object (i.e. its inertia) The relationship between them is or The direction of will always correspond to the direction of

Free-Body Diagrams Simplified drawing of a body with only the forces acting on it specified The forces are drawn as vectors Free-Body diagrams facilitate the application of Newton’s 2 nd Law Examples: Joey Joey in “Free Fall” Joey Joey standing on a floor Joey Joey getting slapped while standing on a floor

Types of Forces Non-Contact: Gravitational Electric Magnetic Contact: Normal Frictional Tension In our world, forces can be categorized as one of 2 types: Non-Contact: force is exerted over a distance of space with out direct contact (a.k.a. “action-at-a-distance” forces) Contact: forces is exerted due to direct contact (Note: at the microscopic level, ALL forces are non-contact) In either case, Newton’s 3 rd law still applies to the forces present Examples of each type of force:

Weight The “weight” of an object is the gravitational force exerted on it by the gravitational attraction between the object and its environment: On the surface of the Earth, the gravitational force is referred to as weight: Mass is a measure of an object’s inertia (measured in kg) –Independent of object location Weight is the effect of gravity on an object’s mass (measured in N) –Determined by the local gravitational acceleration surrounding the object Notes: Mass is a measure of an object’s inertia (measured in kg) –Independent of object location Weight is the effect of gravity on an object’s mass (measured in N) –Determined by the local gravitational acceleration surrounding the object

Normal Force The “support” force between 2 surfaces in contact Direction is always perpendicular (or normal) to the plane of the area of contact Example: the force of floor that supports your weight Consider standing on a scale on the floor of an elevator. The reading of the scale is equal to the normal force it exerts on you: Construct free body diagrams for the scale: –At rest –Constant velocity –Accelerating upward –Accelerating downward

Examples of Normal Force

Tension Force Force applied through a rope or cable When the rope or cable is massless (negligible compared to the bodies it is attached to) it can be treated as a connection between 2 bodies –No mass means no force needed to accelerate rope –Force of pull transfers unchanged along the rope –Action force at one end is the same as the Reaction force at the other end When attached to a pulley the tension force can be used to change the direction of force acting on a body Calculation of a tension force is usually an intermediate step to connecting the free-body diagrams between 2 attached objects

Tension Applications With Pulley (flat surface): Inclined Plane: Atwood Machine: M1M1 M2M2 M1M1 M2M2  M1M1 M2M2

Newton’s 3 rd Law When an object exerts a force on a second object, the second object exerts an equal but oppositely directed force on the first object where: Consequences: Forces always occur in action-reaction pairs (never by themselves) Each force in an action-reaction pair acts on a different object Important: Newton’s 3 rd law identifies the forces produced by interactions between bodies Newton’s 2 nd law defines the accelerations that each object undergoes Body 1 Body 2