Transcript Newton

How Newton Unified the Motions
of the Moon, Sun, and Apples
Review of Renaissance
Heliocentric Model of Copernicus
Review of Renaissance
Galileo
Saw Venus go through phases like the
moon
Saw objects orbiting Jupiter
Review of Renaissance
Makes the first measurements of how quickly objects pick up speed as they fall – finds all
objects fall at the same rate regardless of size or how heavy they are
The first measurement of gravity. Although he doesn't call it that.
How long does it take the ball to fall ½ way down the ramp?
About ¾ of the total time it takes to fall all the way to the bottom:
Using ratios he discovers d = 1/2at2
Review of Renaissance
He also studied horizontal
motion and the concept of
forces acting to move
objects or stop them
moving. He surmised that
without something to
change the motion of an
object it should keep
going.
Newton
Born in 1642, the same year Galileo died.
He died in 1727, at the age of 85.
Newton discovered the origin of color.
He used his knowledge of optics to invent the
first reflecting telescope - a major
breakthrough because this will eventually
allow larger, more sensitive telescopes to
be built.
Newton
Discovered the nature of gravity as an
attractive force.
Created a unified view of force and motion
in which motion in the heavens, and on
Earth, the known universe at the time
could be explained by the same few rules.
Before he's through, he invents calculus as
the mathematical language necessary to
understand how gravity works.
Calculus
For example, how do I compute the area of a circle.
Using calculus you take a line of some radius and rotate it around
3600 or 2 radians.
In calculus this operation looks like this :
Language should evolve so that communication becomes more
efficient; i.e. the above graphic shows how to derive the area of
a circle in using the least amount of characters and symbols
Principia (1687)
Provided a detailed explanation of the laws of gravity and
motion, particularly as they applied to astronomy.
Principia is still considered by many to be the greatest scientific
book ever written. It contains the fundamentals for all of modern
science.
So What did he do?
Remember Galileo was studying laws of
motion, the concepts of inertia, and forces.
But he did not formalize all of them.
Newton takes what Galileo did and expands
on it until he has a new mathematical
model of forces. We call this Newton's
laws of motion.
First Some Definitions
Newton describes the concepts of
Momentum which equals mass times velocity.
p=mv
The law of the conservation of momentum.
The total momentum of a system is
conserved. Meaning for example you can
transfer momentum between objects in a
collision the total amount of momentum
stays the same.
Force causes changes in momentum.
Newton's 1st Law
The momentum law :
A body remains at rest or moves
in a straight line of constant
velocity as long as no external
forces acts on it
Newton's 2nd Law
The force law :
A body acted on by a force will
accelerate such that force
equals mass times
acceleration
F=ma
Impulse
More accurately, a force is the
time rate of change of the
momentum.
Resistance
Newton's 3rd Law
Law of Reaction :
For every action there is an
equal and opposite reaction.
Means whenever one thing
exerts a force on another, an
equal amount of force is
exerted back on it.
Gravity
Things near the earth fall to the
ground unless something
holds them up.
Earth's gravity pulls any object
toward it - even without
touching it.
It is also the force that holds the
Universe together: planets to
stars, stars to galaxies,
galaxies to each other.
Universal Gravity
ALL objects attract each other with a force of gravitational
attraction.
Gravity
Newton also showed when we
deal with spherical bodies,
the force of gravity acts as if
all the mass is concentrated
at the center of the spheres
Makes math much easier for
us now
But he had to develop modern
calculus to do this
Gravity
The force of gravity
between you and the
Earth acts as though all
the mass of the Earth is
concentrated at a point
at its center and all your
mass is concentrated at
your center of mass
In this case, masses are
said to be Point Masses
A Concern for Newton
How come the Moon doesn't fall into the Earth?
Or the Earth into the Sun...
An orbit is the balance between inertial (Newton's First Law) and
gravitational forces (Newton's second law).
That is, the earth is continually falling toward the sun, but inertia
also wants the earth to keep moving in a straight line. When these
two forces are in balance a stable orbit results:
A Stable Orbit
Well, Is the Universe Stable?
Is gravity there at large distances?
If so, How is it the universe avoids collapsing in on itself?
Are there orbits in the Universe?
It seems to me that if the matter of our sun and planets and all the matter
of the Universe were evenly scattered throughout all of the heavens,
and every particle had and innate gravity towards all the rest … some
of it would convene into one mass and some into another so as to
make an infinite number of great masses, scattered at great distances
from one another throughout all that infinite space.
Newton's Convinced
Newton
Newton was the integrator, the unifier, the
organizer, of all the scientific knowledge
available at the time. He established a
solid platform on which all modern
science could be built.
For centuries, Newton's physics was
accepted without major changes because
it explained so many different phenomena,
could be used to predict many physical
events (such as the return of Halley's
comet), was mathematically sound, and
had many practical applications.