Kinematics is the study of motion, that is, the relationship between an object's position, time, and the rate at which those change. The simplest descriptions and predictions of motion are for objects that don't move at all or only move back and forth along one dimension.
By the end of this unit, a successful student will be able to:
1. Define displacement, position, distance (2-1), speed, velocity (2-2, 2-3) and acceleration (2-4) (MSTE: Phys 1.2)
2. Recognize the algebraic relationships between the above quantities when acceleration is constant and use them to solve one-dimensional problems (2) (MSTE: Phys 1.2)
3. Distinguish between vector quantities (velocity, acceleration) and scalar quantities (speed) (2-1, 2-2) (MSTE: Phys 1.1)
4. Recognize the gravitational field strength near the Earth’s surface as being constant and resulting in a constant acceleration of 9.8 m/s2. (2-7)
5. Create and interpret graphs of motion (position vs. time, speed vs. time, velocity vs. time, acceleration vs. time) including recognizing the role that slope and area under the function play in those interpretations. (2-8) (MSTE: Phys 1.3)
All assignments are due on the date listed. That is not the date they are assigned.
Due date Day Assignment
? Day 1 Read: 2-1 à 2-6
Do: Questions: 1-10 (Problem Set 5)
? Day 3 Do: Problems: 2, 6, 7, 10, 11, 14, 16, 19, 21, 22 (PS 6)
? Day 4 Read: 2-7, 2-8
Do: Questions: 11 – 20 (PS 7)
? Day 5 Do: Problems: 27, 30, 32, 37 (PS 8)
? Day 7 Do: Problems 39, 42, 47, 50, 52 ,55, 58, 63 (PS 9)
? Day 8 Write: Acceleration lab (Cart&Ramp lab #2)
? Day 9 Do: Problems 64, 68, 69,73, 75, 77, 82 (PS 10)
? Day 10 Test: Unit 2
Missed a class? Forgot what we did last week? Follow the link to Physics Unit 2 Daily Plans
Classical Mechanics is the branch of physics first codified by Isaac Newton, built on a foundation laid by Galileo. It works out quite well so long as the velocities involved are much less than the speed of light in a vacuum, when relativity kicks in, or if you try to specify the momentum and position or energy and time of an object so closely that quantum uncertainty becomes important. Most everyday situations involving forces, mass, and energy, can be adequately described using classical mechanics.
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For more on kinematics you may be interested in:
The Cartoon Guide to Physics by Larry Gonick and Art Huffman