Mr. Rogers' Honors Physics

Syllabus 1st Quarter 2nd Quarter 3rd Quarter 4th Quarter
2D Force(5)
2D Motion(6)
Gravitation(7)
Rotation(8)
 

Gravitation-- Chapter 7
SC Standards :

Indicators

P-2.1 Represent vector quantities (including displacement, velocity, acceleration, and force) and use vector addition.

P-2.7 Use a free-body diagram to determine the net force and component forces acting upon an object

P-2.5 Explain the factors that influence the dynamics of falling objects and projectiles.


   

Practice Test Study Guide

Objectives

Essential Question: What is a force field field?

Newton's Law of Universal Gravitation

  1. Define the term gravity field.
  2. (gravity field) =

     (gravity force)

    (unit of mass)

  3. Explain why gravity field is a vector.

  4. Define Newton's Law of Universal Gravitation in mathematical form and evaluate the nature of the forces involved.

  5. mathematical form: F = (G∙M∙m) / r2

    M and m represent 2 point sources of mass that are being pull together by an action/reaction pair of gravity forces. While the forces are opposite in direction, each has a magnitude of F as calculated above even though one of the masses could be much larger than the other.

  6. Explain the assumptions and limitations of Newton's Law of Universal Gravitation

    assumes planets act as point sources of mass. The variable r in the equation is the distance between the center of mass of the 2 masses.

  7. only works at or above the surface of a planet. If the equation worked inside the planet, then at the center, the gravitational attraction force would be infinity. However, at the center the force = 0.

  8. Draw and compare the gravity fields for 2 different mathematical models using rays.
  9. Flat Earth (useful near the surface) : F = mg

    Spherical planet: F = (GMm) / r2

  10. Describe the gravity field inside a hollow planet. g = zero

 

Essential Question: How does gravity field vary with distance?

Applications of Newton's Law of Universal Gravitation

 

  1. Solve inverse square law type problems using Newton's Law of Universal Gravitation.

  2. Combine F = mg with the Universal Gravitation Equation to find an expression for g.

    Formative assessment: Evaluate the effects on g for a planet if the mass and/or radius are altered by various factors.

    radius = 6.371 x 106meters

    mass = 5.9736 x 1024 kg

    G = 6.754 x 10-11 m3/kg/s2

     

Homefun (formative/summative assessment): Read sections 7.1

 

Formative Assessment: Physics Investigation

Title Simulation of Gravity Field Using a Light Source
Research Question Does light intensity of the beam from a projector follow an inverse square law relationship?
Background

Light intensity = (amount of light) / (unit of area)

Note: the division operator or / can be verbalized as "per". Hence, Light intensity is the amount of light per unit of area.

Hypothesis Form a hypothesis.
Data, Calculations Calculate the relative light intensity falling on the screen at a distance from the projector. Double the distance and repeat the process.
Conclusions Draw a conclusion
Deliverables Hypothesis, Data, Calculations, Conclusion
Resources/Materials Projector and tape measure.

 

 

Essential Question: What is the fastest way to get from one side of the Earth to the other?

Graphing a Planet's Gravity Force

  1. Graph the gravity force vs. distance from the center of a planet assuming that a tunnel exists that would allow an object to pass from one side of a planet to the other through the center of the Earth.

  2. Describe the motion that would occur if an object were dropped in the tunnel, assuming no air resistance and explain how theoretically this would be an incredibly good form of transportation.

     

Homefun (formative/summative assessment): Read section 7.2, do Section Review Problems 7, 11 p. 178.

 

 
Essential Question: What is a geostationary orbit and how is it used?

Orbits of Satellites

  1. Calculate the weight force acting on an object in orbit. F = (GMm)/r2

    Formative assessment: What is the weight of a 150 lb object 1.6 x 106meters or roughly 1000 miles above the surface of the Earth?

  2. Explain why a person in orbit actually has a significant amount of weight even though they feel weightless.

  3. Derive an expression for the velocity required to maintain a given circular orbit using the following models:

  4. Starting Information
    Final Product

    F = ma

    F = (GMm) / r2

    a = v2/ r

    v = (GM/r)1/2

     

  5. Derive an expression for the period of a circular orbit given the orbital velocity and radius from the center of a planet. Use the following:
  6. S = d / t

    period: (the time it takes to complete 1 orbit) = T

    distance traveled in one orbit: (the circumference) = 2πr

    Final Product

    T = 2π[ r3/ (GM) ]1/2

     

  7. Define what a geostationary orbit is and why it is of significant usefulness to humans.

  8. Neglecting air resistance, explain why heavier masses do not fall at a greater rate of acceleration than lighter weight masses and why the mass of an orbiting object does not affect the conditions required for orbit.

 

Homefun (formative/summative assessment): problems 15, 17 p. 185; 31, 33, 37, 51, 71 p. 190 to 193

 

Essential Question: How can you best prepare for the test?

Review of Objectives 1- 13 (1-3 days)

Formative Assessments:

  1. Work review problems at the board

  2. Work practice problems.

Metacognition Problem Solving Question: Can I still work the problems done in class, several hours or days later? Some amount of repetition on the exact same problems is necessary to lock in learning. It is often better to thoroughly understand a single example of a problem type than to work example after example understanding none of them completely.

Relevance: Good test preparation is essential to performance in physics class.

Homefun (formative/summative assessment): problems 81, 89, 91, 59 pages 193-194; problems turn in on the day stapled to the back of the test.

Summative Assessment: Unit exam objectives 1-16

 
Mr

SAM Team--Southside High School's STEM and Computer Science extra-curricular club (Mr. Rogers Sponsor)

Mr. Rogers' Twitter Site

Mr. Rogers Teacher's Blog

Mr. Rogers T-shirts

Mr. Rogers Information for Teachers

Mr. Rogers Science Fair Information

Check out other web sites created by Mr. R:

Check out Articles by Mr. Rogers:

 
Insultingly Stupid Movie Physics is one of the most humorous, entertaining, and readable physics books available, yet is filled with all kinds of useful content and clear explanations for high school, 1st semester college physics students, and film buffs.

It explains all 3 of Newton's laws, the 1st and 2nd laws of thermodynamics, momentum, energy, gravity, circular motion and a host of other topics all through the lens of Hollywood movies using Star Trek and numerous other films.

If you want to learn how to think physics and have a lot of fun in the process, this is the book for you!

 

First the web site,

now the book!


Mr. Rogers Home | Common Sylabus | AP Comp Sci I | AP Comp Sci II | AP Physics Mech | AP Physics E&M | AP Statistics | Honors Physics|IB Design Tech | Southside

[ Intuitor Home | Physics | Movie Physics | Chess | Forchess | Hex | Intuitor Store |

Copyright 1996-2011 T. K. Rogers, all rights reserved. Forchess is a registered trademark of T. K. Rogers.
No part of this website may be reproduced in any form, electronic or otherwise, without express written approval.