gravitation ch 9: hasbun ch 5: thornton & marion

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Gravitation Ch 9: Hasbun Ch 5: Thornton & Marion

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Page 1: Gravitation Ch 9: Hasbun Ch 5: Thornton & Marion

GravitationCh 9: HasbunCh 5: Thornton & Marion

Page 2: Gravitation Ch 9: Hasbun Ch 5: Thornton & Marion

Introduction

Newton, 1666Published in Principia, 1687 (needed to develop calculus to prove his assumptions)

Newton’s law of universal gravitationEach mass particle attracts every other particle in the universe with a force that varies directly as the product of the two masses and inversely as the square of the distance between them.

Page 3: Gravitation Ch 9: Hasbun Ch 5: Thornton & Marion

Cavendish Experiment

Henry Cavendish (1731-1810) verified law and measured G

G=6.67 x 10-11 N m2 / kg2

video

Page 4: Gravitation Ch 9: Hasbun Ch 5: Thornton & Marion

Extended Objects

Page 5: Gravitation Ch 9: Hasbun Ch 5: Thornton & Marion

Gravitational Field

Gravitational field = force per unit mass

For point masses:

For extended objects:

Page 6: Gravitation Ch 9: Hasbun Ch 5: Thornton & Marion

White Boards

Is gravity a conservative forces?

Page 7: Gravitation Ch 9: Hasbun Ch 5: Thornton & Marion

Gravitational PotentialGravitational field vector can be written as the gradient of a scalar function:

Φ is the gravitational potentialEnergy/mass

We can obtain Φ by integrating:

Page 8: Gravitation Ch 9: Hasbun Ch 5: Thornton & Marion

Potential from Continuous Mass

Distributions

Prime denotes integration element

Page 9: Gravitation Ch 9: Hasbun Ch 5: Thornton & Marion

Gravitational Potential

Once we know Φ, we can determine the gravitational force and the gravitational potential energy.

Page 10: Gravitation Ch 9: Hasbun Ch 5: Thornton & Marion

Example

What is the gravitational potential both inside and outside a spherical shell of inner radius b and outer radius a?

Page 11: Gravitation Ch 9: Hasbun Ch 5: Thornton & Marion

Poisson’s Equation

Gauss’s Law for the electric field

Gauss’s Law for gravity

Poisson’s Equation

Page 12: Gravitation Ch 9: Hasbun Ch 5: Thornton & Marion

Lines of Force & Equipotential Surfaces

Equipotential lines connect points of constant potential

Force is always perpendicular to the equipotential lines

Like a contour map, lines of equipotential show where an object can move while maintaining constant gravitational potential energy

Page 13: Gravitation Ch 9: Hasbun Ch 5: Thornton & Marion

Using Potential

Potential is a convenient way to calculate the force

Force is physically meaningful

In some cases, it might be easier to calculate the force directly

Potential is a scalar

Page 14: Gravitation Ch 9: Hasbun Ch 5: Thornton & Marion

Example

Consider a thin uniform disk of mass M and radius a. Find the force on a mass m located along the axis of the disk. Solve this using both force and potential.

Page 15: Gravitation Ch 9: Hasbun Ch 5: Thornton & Marion

Lagrange Points

Solved by Euler & Lagrange

Sun is M1

Earth-Moon is M2

Stable equilibriumL4 , L5

WMAP satellite in L2

Page 16: Gravitation Ch 9: Hasbun Ch 5: Thornton & Marion

MATLAB ProblemStart with the following code. Adjust the mass ratios and contour levels until you recreate the plot showing the Lagrange points. Name your file equipotential.m