gravitation ch 9: hasbun ch 5: thornton & marion
TRANSCRIPT
GravitationCh 9: HasbunCh 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.
Cavendish Experiment
Henry Cavendish (1731-1810) verified law and measured G
G=6.67 x 10-11 N m2 / kg2
video
Extended Objects
Gravitational Field
Gravitational field = force per unit mass
For point masses:
For extended objects:
White Boards
Is gravity a conservative forces?
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:
Potential from Continuous Mass
Distributions
Prime denotes integration element
Gravitational Potential
Once we know Φ, we can determine the gravitational force and the gravitational potential energy.
Example
What is the gravitational potential both inside and outside a spherical shell of inner radius b and outer radius a?
Poisson’s Equation
Gauss’s Law for the electric field
Gauss’s Law for gravity
Poisson’s Equation
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
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
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.
Lagrange Points
Solved by Euler & Lagrange
Sun is M1
Earth-Moon is M2
Stable equilibriumL4 , L5
WMAP satellite in L2
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