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The Ordered Universe Chapter 2 Great Idea: Newton’s laws of motion and gravity predict the behavior of objects on Earth and in space
Transcript
Page 1: Ch02

The Ordered Universe

Chapter 2

Great Idea:Newton’s laws of motion and gravity predict the

behavior of objects on Earth and in space

Page 2: Ch02

Chapter Outline

• The Night Sky• The Birth of Modern Astronomy• The Birth of Mechanics• Isaac Newton and the Universal Laws

of Motion• Momentum• The Universal Force of Gravity

Page 3: Ch02

The Night Sky

Page 4: Ch02

The Night Sky

• Movement of stars, planets, sun– Key for survival of ancestors

• Astronomy– First science

• Ancient observers:– Physical events are quantifiable and

therefore predictable

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Stonehenge

• Started in 2800 B.C.– Built over long time– Built by different peoples

• Marks passage of time– Specifically the seasons

• Still functions today

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Stonehenge

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Science in the Making

• The Discovery of the Spread of Disease

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Science by the Numbers

• Ancient Astronauts

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The Birth of Modern Astronomy

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The Historical Background: Ptolemy

• Ptolemy• 2nd century A.D.

• First planetary model• Earth at center, stationary• Stars and planets revolved around earth

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The Historical Background: Ptolemy

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The Historical Background: Copernicus

• Copernicus• 1543: On the Revolutions of the Spheres• Sun at center

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The Historical Background: Copernicus

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Observations: Tycho Brahe and Johannes Kepler

• Tycho– Observed new star

• Showed heavens can change

– Designed and used new instruments• Collected data on planetary movement

• Kepler (Tycho’s colleague)– First Law:

• Planets have elliptical orbits

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Kepler’s First Law

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The Birth of Mechanics

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Galileo Galilei

• Mechanics: motions of material objects

• Galileo (1564–1642)– Mathematics professor– Inventor– First to record observations

with telescope• Supported Copernicus’ view

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Telescopes Used by Galileo Galilei

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Science in the Making

The Heresy Trial of Galileo

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Speed, Velocity, and Acceleration

• Speed=distance traveled over time• Velocity=speed with direction

• Equation for speed:

• Acceleration=rate of change of velocity

• Equation for velocity:

t

dv

t

vva if

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The Founder of Experimental Science

• Galileo– Relationship among distance, time,

velocity and acceleration– Found objects accelerate while falling

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Galileo’s Falling-Ball Apparatus

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Galileo cont.

• Constant acceleration– Balls on a plane: v=at

• Freefall– Constant acceleration at g– g = 9.8 m/s2=32 feet/s2

– Distance traveled (d)=½at2

Page 24: Ch02

Accelerated Motion of a Falling Apple

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Equations Relating d,v,a, and t

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The Science of Life

• Experiencing Extreme Acceleration

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Isaac Newton and the Universal Laws of Motion

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The First Law

• An object will continue moving in a straight line at a constant speed, and a stationary object will remain at rest, unless acted upon by an unbalanced force

• Uniform motion vs. acceleration• Force• Inertia

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Hammer Thrower

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The Second Law

• The acceleration produced on a body by a force is proportional to the magnitude of the force and inversely proportional to the mass of the object

• Equation: F=ma

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The Third Law

• Interacting object exert equal but opposite forces upon each other

• The reactions may not be equal and opposite

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Newton’s Laws of Motion at Work

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Newton’s Laws of Motion at Work

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Newton’s Laws at Work

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Momentum

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Momentum

• Motion depends on mass and speed• Linear momentum:

– p=mv

• Law of conservation of linear momentum

• Angular momentum

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The Law of Conservation of Linear Momentum

Page 38: Ch02

The Conservation of Angular Momentum

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The Universal Force of Gravity

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The Universal Force of Gravity

• Gravity

• Newton’s law of universal gravitation– F=Gm1m2/d2

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The Influence of theForce of Gravity

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The Gravitational Constant, G

• G-constant of direct proportionality– Universal

• Henry Cavendish– G = 6.67 x 10–11m3/s2-kg or

6.67 x 10–11N-m2/kg2

Page 43: Ch02

The Cavendish Balance

Page 44: Ch02

Weight and Gravity

• Weight– Gravity acting on an object’s mass

• Weight depends on gravity– Different on earth vs. moon

• Mass is constant

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Big G and Little g

• Closely related:– Force = (G x mass x ME)/RE

2

– Force = mass x g• Setting equations equal:

– Mass x g = (G x mass x ME)/RE2

• Divide by mass

– g = (G x ME)/RE2

• Plug in values

– 9.8 N-kg = 9.8m/s2

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Halley’s Comet in 1985


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