An exposure to Newtonian mechanics

Slides:



Advertisements
Similar presentations
How to Study the Universe
Advertisements

The Beginning of Modern Astronomy
Phys141 Principles of Physical Science Chapter 3 Force and Motion Instructor: Li Ma Office: NBC 126 Phone: (713)
Fall Final Review WKS: WORD PROBLEMS Part II. 1. A car travels at a constant speed of 15 m/s for 10 seconds. How far did it go?
Newton’s Laws of Motion three laws of motion: fundamental laws of mechanics describe the motion of all macroscopic objects (i.e., everyday size objects)
Newton’s Laws.
Classical Mechanics Describes the relationship between the motion of objects in our everyday world and the forces acting on them Conditions when Classical.
FORCE A force is any influence that can change the velocity of a body. Forces can act either through the physical contact of two objects (contact forces:
Chapter 4: Newton and Universal Motion
AMY SHANTA BABOOLAL PHYSICS PROJECT: MECHANICS. ARISTOTLE’S ARGUMENTS One of his well known arguments is: to understand change, a distinction must be.
Mechanics Motion Equations and Graphs Combining and Resolving Vectors Force and Acceleration Gravity and Free-Body Diagrams Projectile Motion Work and.
Newton’s Three Laws Forces and Motion. What Is a Force? Any influence that may change the motion of an object For example: a push, a pull, an attraction,
1 Physics 1100 – Spring 2009 Review for Exam I Friday, February 27 th Chapters
Professional Development Series June 18, 2005 The Physics of Tops presented by Luis A. Martínez-Pérez, Ph.D. Associate Professor Science Education Florida.
ISAAC NEWTON’S PHYSICS PRINCIPLES. WHAT NEWTON DID When it comes to science, Isaac Newton is most famous for his creation of the THREE LAWS OF MOTION.
1 An exposure to Newtonian mechanics Quantities such as velocity, etc. Newtonian spacetime Newton’s laws A smattering of useful equations Motivation In.
Equations of Motion PSC1341 Chapter 2 2 Speed and velocity Speed is the distance traveled in a certain amount of timev = d/t Average speed is determined.
Resistance of an object to a change in its motion inertia.
Chapter 3.2 & 3.3 Forces and Energy!!. Force Force is a push or a pull on an object! Forces can change the shape or motion of an object!
Patterns of Motion. In a moving airplane, you feel forces in many directions when the plane changes its motion. You cannot help but notice the forces.
Chapter 2 MOTION. - one of the more common intangible concepts in science - is the act or process of changing position TWO IMPORTANT ASPECTS OF MOTION.
Chapter 3.2 & 3.3 Forces and Energy!!.
Chapter 5 Newton’s 2 nd Law. We know that in order for an object at rest to move it has to have a force on it. For a moving object to stop it has to have.
MOTION & FORCES VOCABULARY MOTION The process of continual change in the physical position of an object (distance) relative to reference point ; With.
Gravity Gravity is the force that pulls objects toward the center of the earth.
Dynamics: Newton’s Laws of Motion
Last Thoughts on Work Work can be done by friction Friction always opposes motion so the work it does is usually negative. (exceptions are like conveyor.
Chapter 4 The Laws of Motion. Classical Mechanics Describes the relationship between the motion of objects in our everyday world and the forces acting.
Physics 218 Lecture 15: Momentum Alexei Safonov.
The Laws of Motion Newton’s Three Laws. What is a Force? It is something we experience every single day. You are exerting a force on your pencil right.
Newtonian Mechanics Single Particle, Chapter 2 Classical Mechanics: –The science of bodies at rest or in motion + conditions of rest or motion, when the.
Ch. 4, Motion & Force: DYNAMICS
KD3 Linear Mechanics Chapters 4, 5 & 6. Force Force- A push or pull which can change an object’s state of rest or motion (if the force is unbalanced)
1 A Quick Look at the Basics Dr. Harold Geller College of Science School of Physics, Astronomy and Computational Sciences George Mason University.
Notes – Representing Motion. Laws of Motion Isaac Newton – 1686 – English scientist discovered the three laws of motion Motion – The change in position.
What Is interesting about this title?
Chapter 4 The Laws of Motion.
Space-Time Symmetry.
Chapter 8: Forces & Motion
Syll. State.: —due Friday, October 3
Motion and Mechanics Physics.
Chapter Four The Laws of Motion.
How Forces Affect Motion
Newton’s Laws of Motion
FORCE A force is any influence that can change the velocity of a body. Forces can act either through the physical contact of two objects (contact forces:
Physics: Principles with Applications, 6th edition
Bell Work Week of Monday, March 23 – Friday, March 27
Newton, Einstein and Gravity
Physical Science Coach Mynhier
Newton’s Laws of Motion
Force -a push or a pull F = ma.
Universal Gravitation
Chapter 3 Motion in a Plane.
UNIT 2 MECHANICS Chapter 5 Dynamics.
Standards S8P3. Obtain, evaluate, and communicate information about cause and effect relationships between force, mass, and the motion of objects. Construct.
Chapter 4 The Laws of Motion.
Newton’s Laws of Motion
Dynamics: Newton’s Laws of Motion (Ch. 12)
Chapter 4 The Laws of Motion.
Force and Motion Vocabulary
Newton, Einstein, and Gravity
Gravity, Projectiles, and Satellites
Several themes are recurrent
Forces.
Impulse and Momentum Chapter 7.
The Laws of Motion (not including Atwood)
The Science of Motion & Orbits
Force and Motion Vocabulary
Newton’s First Law & Linear Motion
Newton’s 1st and 2nd Laws.
Presentation transcript:

An exposure to Newtonian mechanics Quantities such as velocity, etc. Newtonian spacetime Newton’s laws A smattering of useful equations Motivation In order to understand aspects of more modern physics and astronomy, we must ground it in the context of conventional science.

The 3+1 Newtonian grid of the Universe Space consists of three spatial dimensions. To every point in space, you can assign coordinates (x, y, z). This is your reference frame. Distances between points in this space are given by the Pythagorean theorem, L2=Δx2 + Δy2 + Δz2 Absolute space, in its own nature, without regard to anything external, remains always similar and immovable. – Newton (1687) 7

The 3+1 Newtonian grid of the Universe Time (t) is the beat to which the Universe ages. One can assign the same time value to all points in the grid, thus establishing when things are simultaneous, and when they are not. The rate of time is 1 sec/sec, everywhere. Absolute, true and mathematical time, of itself, and from its own nature flows equably without regard to anything external, and by another name is called duration.... – Newton (1687) 7

Linear Velocity and Acceleration If an object changes (Δ) the value of its spatial coordinate, during a certain interval of time, we call this velocity. vx= Δx/Δt vy= Δy/Δt vz= Δz/Δt Note: velocity is not quite the same as speed. It includes direction information: it is a vector, not a scalar. If an object changes the value of its velocity during a certain interval of time, we call this acceleration. ax= Δvx/Δt ay=Δvy/Δt az=Δvz/Δt 7

Linear Velocity and Acceleration Close your eyes in a luxury car. You cannot feel velocity. You can feel acceleration. The physical laws of the world work if whether we are sitting still, or moving in a straight line. —Or, stated another way… Physical laws work the same whether your reference frame is… — stationary to someone else’s — moving with respect to someone else’s. 7

Linear Velocity and Acceleration Velocities add together quite sensibly. vtotal= v1 + v2 This is called Velocity Addition. Many other vectors and scalars add this way too, such as accelerations, changes in distance, etc. 7

Newton’s Laws of Motion LAW #1: An object at rest stays at rest, unless acted upon by an external, unbalanced force. Similarly, an object in motion continues in motion, unless acted upon by an external, unbalanced force. This law defines a reference frame that is either stationary with respect to the observer (v=0), or moving (v=0). Newton’s laws work within an inertial reference frame. If an object changes its velocity WITHOUT an external force acting on it, you are not in an inertial reference frame. Ex: In an accelerating car. 7

Inertial reference frames A belief in absolute reference frames is so ingrained into our minds, they have become a metaphor for comforting reliability. I have of late,—but wherefore I know not,—lost all my mirth, forgone all custom of exercises; and indeed, it goes so heavily with my disposition that this goodly frame, the earth, seems to me a sterile promontory; this most excellent canopy, the air, look you, this brave o’erhanging firmament, this majestical roof fretted with golden fire,—why, it appears no other thing to me than a foul and pestilent congregation of vapours. —Shakespeare, “Hamlet,” Act II, scene ii 7

Mass, Momentum, and Force Mass is a measure of how much stuff you are dealing with. It is (in Newton’s framework) a sum of the particles that constitute something. It is NOT weight. M, m, etc. is measured in kg. Momentum is a useful concept, p=mv. Force is a measure of how hard one thing pushes or pulls upon something else. F is measured in Newtons or pounds. 7

Newton’s Laws of Motion LAW #2: If an unbalanced force (F) acts upon a mass (m), the mass will respond with an acceleration (a), such that: F = ma This law can be rewritten: Since a= Δv/Δt F = ma = m(Δv/Δt) = (mΔv)/Δt = Δp/Δt 7

Newton’s Laws of Motion LAW #3: For every force, there is a counter force of equal strength but opposite direction: F1 = -F2 m1a1 = -m2a2 This law can be manipulated to: a1 = -(m2/m1)a2 This does not mean that nothing can happen! Ex: Rockets, bullets, or energy dissipation. 7

Newton’s Laws of Motion Law of Gravity: For two objects, of masses m1 and m2, with their centers separated by distance R12, there is a mutually attractive force : F12 = Gm1m2/R122 Notes G=6.67×10-11 N m2/kg2 Gravity never goes away. Gravity is an inverse-square law. 7

Newton’s Action at a Distance For Newton’s law of gravity to work, he required that it be able to affect things at unlimited distances. The effect was instantaneous. This is called a NONLOCAL effect, and Newton despised nonlocality. “I have not been able to discover the cause of those properties of gravity from phenomena, and I frame no hypothesis” Leibnitz: “That means of communication (says he) is invisible, intangible, not mechanical. He might as well have added, inexplicable, unintelligible, precarious, groundless, and unexampled… ‘Tis a chimerical thing, a scholastic occult quantity.” 7

Energy in various forms Kinetic energy (K.E.) 1) K.E.=½mv2 2) Temperature is a measure of KE/particle Potential energy (P.E.) 3) P.E.=mgh (falling under the influence of a uniform gravitational field) More forms of P.E. exist: batteries, springs, etc. 7

Circular Motion Linear motion x, v, a, F, p, E, t Angular motion θ, ω, α, τ, L, E, t Force required to keep an object in circular motion: Fc = mvc2/R 7

Conservation Laws A vast number of problems in physics are solved using principles of conservation. Linear momentum and total energy are conserved. Notes Angular momentum is also a conserved quantity. Energy is conserved, but it may be transferred to/from K.E., P.E., and other things. 7

Things Worth Noting! Newton’s genius is reflected in three insightful assumptions. 1)Action at a distance for the Law of Gravity (violation of locality). 2)Inertial mass (F=ma) is the same thing that causes gravity (F=Gm1m2/R2). 3)Previous to Newton, scientists treated terrestrial physics and cosmic physics differently. Newton uses the same laws for both settings. Showing that both sets of laws are really aspects of a simpler, underlying single set of laws, is called “Unification.” 7