Physics 218: Mechanics Instructor: Dr. Tatiana Erukhimova Lecture 17.

Slides:



Advertisements
Similar presentations
Rotational Equilibrium and Rotational Dynamics
Advertisements

Physics 218: Mechanics Instructor: Dr. Tatiana Erukhimova Lecture 24.
Physics 218: Mechanics Instructor: Dr. Tatiana Erukhimova Lecture 18.
Physics 218: Mechanics Instructor: Dr. Tatiana Erukhimova Lecture 19.
The first exam will be held on Tuesday, September 23, in room 109 Heldenfels from 7 to 9:30 p.m. Section 807 and half of section 808 (students with last.
Physics 218: Mechanics Instructor: Dr. Tatiana Erukhimova Lecture 14.
Physics 218: Mechanics Instructor: Dr. Tatiana Erukhimova Sections 818, 819, 820, 821 Lecture 11.
Physics 218: Mechanics Instructor: Dr. Tatiana Erukhimova Lecture 13.
Physics 218: Mechanics Instructor: Dr. Tatiana Erukhimova Lecture 24.
Physics 218: Mechanics Instructor: Dr. Tatiana Erukhimova Lecture 21.
Physics 218: Mechanics Instructor: Dr. Tatiana Erukhimova Lecture 42.
Instructor: Dr. Tatiana Erukhimova
Physics 218: Mechanics Instructor: Dr. Tatiana Erukhimova Lectures 25, 26.
Physics 218: Mechanics Instructor: Dr. Tatiana Erukhimova Lecture 12.
Physics 218: Mechanics Instructor: Dr. Tatiana Erukhimova Lectures 27, 28.
Physics 218: Mechanics Instructor: Dr. Tatiana Erukhimova Lecture 13.
Instructor: Dr. Tatiana Erukhimova
Physics 218: Mechanics Instructor: Dr. Tatiana Erukhimova Lecture 22.
Physics 218: Mechanics Instructor: Dr. Tatiana Erukhimova Lecture 37 Exam: from 6 pm to 8 pm.
Physics 121 Newtonian Mechanics Instructor: Karine Chesnel Feb 26 th, 2009 Review for Exam 2 Class website:
Physics 218: Mechanics Instructor: Dr. Tatiana Erukhimova Lectures
The first exam will be on Tuesday, September 25, room 109 in Heldenfels building. Section 807 and half of the Section 808 (students with last name starting.
Physics 218: Mechanics Instructor: Dr. Tatiana Erukhimova Sections 818, 819, 820, 821 Lecture 10.
Physics 218: Mechanics Instructor: Dr. Tatiana Erukhimova Lecture 23.
Physics 218: Mechanics Instructor: Dr. Tatiana Erukhimova Lecture 15.
Instructor: Dr. Tatiana Erukhimova
Physics Instructor: Dr. Tatiana Erukhimova Lecture 6.
Physics 218: Mechanics Instructor: Dr. Tatiana Erukhimova Lecture 20.
Physics 218: Mechanics Instructor: Dr. Tatiana Erukhimova Lecture 27.
Physics 218: Mechanics Instructor: Dr. Tatiana Erukhimova Sections 807, 808, 809 Lecture 8.
Physics 218: Mechanics Instructor: Dr. Tatiana Erukhimova Lecture 23.
Physics 218: Mechanics Instructor: Dr. Tatiana Erukhimova Lectures 22, 23 Hw: Chapter 14 problems and exercises.
Physics 218: Mechanics Instructor: Dr. Tatiana Erukhimova Lecture 26.
Wednesday, Oct. 6, 2004PHYS , Fall 2004 Dr. Jaehoon Yu 1 1.Work done by a constant force 2.Scalar Product of Vectors 3.Work done by a varying force.
Central Force Motion Chapter 8
PHYS 1441 – Section 002 Lecture #22 Monday, April 22, 2013 Dr. Jaehoon Yu Work, Power and Energy in Rotation Angular Momentum Angular Momentum Conservation.
Lecture 17: Problem Solving Review For test 2.
Energy Transformations and Conservation of Mechanical Energy 8
REVISION MOMENTUM. the product of an object's mass and its velocity a vector quantity with the same direction as the velocity of the object. MOMENTUM.
Exam 2 Review 8.02 W08D1. Announcements Test Two Next Week Thursday Oct 27 7:30-9:30 Section Room Assignments on Announcements Page Test Two Topics: Circular.
200 Physics Concepts from Delores Gende Website
Chapter 5 Two Dimensional Forces Equilibrium An object either at rest or moving with a constant velocity is said to be in equilibrium The net force acting.
Tuesday June 14, PHYS , Summer I 2005 Dr. Andrew Brandt PHYS 1443 – Section 001 Lecture #8 Tuesday June 14, 2005 Dr. Andrew Brandt Accelerated.
Thursday, Oct. 30, 2014PHYS , Fall 2014 Dr. Jaehoon Yu 1 PHYS 1443 – Section 004 Lecture #19 Thursday, Oct. 30, 2014 Dr. Jaehoon Yu Rolling Kinetic.
Work and Energy. Scalar (Dot) Product When two vectors are multiplied together a scalar is the result:
Work Readings: Chapter 11.
Physics Instructor: Dr. Tatiana Erukhimova Lecture 6.
Tuesday, June 26, 2007PHYS , Summer 2006 Dr. Jaehoon Yu 1 PHYS 1443 – Section 001 Lecture #15 Tuesday, June 26, 2007 Dr. Jaehoon Yu Rotational.
Chapter 1: Survey of Elementary Principles
Instructor: Dr. Tatiana Erukhimova
Instructor: Dr. Tatiana Erukhimova
Instructor: Dr. Tatiana Erukhimova
University Physics: Mechanics
PHYS 1443 – Section 003 Lecture #18
PHYS 1441 – Section 002 Lecture #22
PHYS 1443 – Section 002 Lecture #12
Instructor: Dr. Tatiana Erukhimova
Force Diagrams.
Instructor: Dr. Tatiana Erukhimova
7.3 Forces in Two Dimensions
Instructor: Dr. Tatiana Erukhimova
Newton’s 1st and 2nd Laws of Motion
PHYS 1443 – Section 003 Lecture #12
Instructor: Dr. Tatiana Erukhimova
Instructor: Dr. Tatiana Erukhimova
Instructor: Dr. Tatiana Erukhimova
Instructor: Dr. Tatiana Erukhimova
Instructor: Dr. Tatiana Erukhimova
Work, Energy, Power.
Instructor: Dr. Tatiana Erukhimova
Presentation transcript:

Physics 218: Mechanics Instructor: Dr. Tatiana Erukhimova Lecture 17

Quiz A block of mass m is placed at rest on a plane inclined at angle θ. After moving down L meters, it has velocity V 1. Find the coefficient of friction between the block and the plane.

Second exam Tuesday, October Heldenfels Section 807 and half of 802 start at 7 pm Section 809 and half of 808 start at 8:05 pm

Work Energy Theorem

If a force can be written as the gradient (slope) of some scalar function, that force is conservative. U(x) is called the potential energy function for the force If such a function exists, then the force is conservative 1D case:

does NOT depend on path! 1D case:

does NOT depend on path! If F x (x) is known, you can find the potential energy function as

or

Newton’s 2nd Law

Work does not depend on the choice of coordinates! You can calculate work of each force in the most convenient system of coordinates. Do not forget to work with components!

Usually there are several ways to solve the problem. Indicate the law or the theorem you use!

Center of Mass

Find the position of the center of mass of the system of the sun and Jupiter. (Since Jupiter is more massive than the rest of the planets put together, this is essentially the position of the center of mass of the solar system.) Does the center of mass lie inside or outside the sun?

Motion of the Center of Mass

The center of mass of a system moves as if all of the mass of the system were concentrated at that point and as if all of the forces were acting at that point There is only the external forces that affect the motion of the center of mass ( ) Only external forces affect the motion of the center of mass

Momentum is a vector! Vector equation!

If

Conservation of Momentum If there is no external force on a system, then the total momentum of the system is a constant

True in X and Y directions separately!