Measuring the Speed of EMR

Slides:



Advertisements
Similar presentations
27.1 – EARLY CONCEPTS OF LIGHT
Advertisements

LIGHT. Early Concepts Light first thought to consist of particles Socrates, Plato, and Euclid Later thought and proved that Empedocles and Huygens Einstein.
Light and sound are the two major ways that we receive information about the world. Of the two, light provides the greater variety of information. The.
Shadows Today’s learning objective is to:
…and a ray?
Astronomy Picture of the Day. Question The Moon has a(n) ________ orbit meaning ________. A. synchronous, its orbital period is equal to its rotation.
The Solar System Isaac Newton (1642)
1. 2 Objectives To state the SI unit of time as the second To explain the meaning of speed and average speed To use the speed equation for calculation.
Where are we?
Distances in Space Science 9. Using scientific notation Distances in space are very large We use scientific notation to represent very large and very.
Ch The Lunar Cycle.  All moonlight is reflected light.  The different parts of the lighted side of the moon that face the earth are known as the.
1. what moon is this  A) waxing gibbous B) Waning gibbous C) Waning crescent D) New moon.
SPACE SYSTEMS UNIT Chapters 26 & 30.
 Photo-Electric Effect  Light causes a metal to eject electrons  Amount of electron ejected depends on frequency of wave not intensity  Einstein’s.
Astronomy in the News It turns out there is five times more material in clusters of galaxies than we would expect from the galaxies and hot gas we can.
Physics Mrs. Coyle. Electromagnetic Waves: oscillating electric and magnetic fields.
1 PH604 Special Relativity (8 lectures) Books: “Special Relativity, a first encounter”, Domenico Giulini, Oxford “Introduction to the Relativity Principle”,
Electromagnetic Spectrum Electromagnetic Spectrum (EM Spectrum) is the entire range of light radiation from gamma rays to radio waves.
Why does the Moon look that way?.  The Moon is about 240,000 miles from the Earth.  The Moon rotates slowly on its axis once every 28 days & orbits.
Chap 16-1 Light Fundamentals.
The Nature of Light Waves vs. Particles. Particle (Corpuscular) Theory Advocated by Newton ( ) Said energy is carried by tiny particles from source.
Days of the week (always go to 1 st hour every day) Monday Guided Study after 2 nd hour Tuesday 1 st 25 minutes is Quiet Study Wednesday Advisory after.
ASTR 111 – 003 Fall 2007 Lecture 02 Sep. 10, 2007 Introducing Astronomy (chap. 1-6) Introduction To Modern Astronomy I: Solar System Ch1: Astronomy and.
Characteristics of Stars There are millions of stars in the universe, but they are very far apart. Because of this, distances between stars are measured.
Archeo-Measuring the speed of light
Sources of Light. Luminous Body – An object that emits light waves.
Light Light is an electromagnetic wave.. We see things because: Either they EMIT light What emits light? Light bulbs Flames The sun Stars or REFLECT light.
RELATIVITY IN EVERY INERITAL REFERENCE FRAME, THE SPEED OF LIGHT IS A CONSTANT BUT WHAT DOES THIS MEAN?
Light!. General Properties of Light Isaac Newton: believed light was a series of fast moving small particles Now we know: light behaves both as particles.
The Speed of Light: Galileo Galileo (Italian) in early 1600s attempted to determine light’s speed by opening a lantern which would be seen by a person.
INTRODUCTION TO LIGHT & ITS SPEED PW2 - REFLECTION.
Speed of light Chapter 27.2 Notes. The Speed of Light It was not known whether light travels instantaneously or with finite speed until the late 1600s.
Motion. INTRODUCTION It’s 2:26 and school is over! You hurry out of class and into the bright daylight. A light breeze is blowing. A few clouds drift.
Warm-up: How far is an Astronomical Unit? Go over 10 questions Sun – Earth - Moon System Notes Sun – Earth – Moon System Homework: Finish the lab.
PHYS Astronomy Homework Set #2 8/31/16 Due 9/12/16 Chapter 3 Review Questions 1, 2, 9 Problems 1, 7, 9, 11 Using the small angle formula, calculate.
What is light?. Light Light is a form of energy. Light Light travels in a straight line Light Light speed is 3.0 x 10 8 m/s Light Light is an electromagnetic.
Lesson 2 Measuring the Speed of Light
Big Bang Theory The majority of the information in this PowerPoint is used unedited for educational purposes and was taken from
Astronomical distances.
01 – Introduction to Light & its Speed
Please write down all the underlined items. Abbreviate to save time.
Spaced-Out System Review
Light Physics Mrs. Coyle.
Speed, Distance, Time Calculations
Light and Color.
Light Physics Mr. Berman.
Tools That Help Us See Celestial Objects
THE MEASUREMENT OF DISTANCE
Eclipses of Jupiter’s moons
Measuring the Speed of Light
Key Areas covered Hubble’s law shows the relationship between the recession velocity of a galaxy and its distance from us. Hubble’s law allows us to estimate.
Lesson #6 Moon Phases.
MOTION Speed, distance, time, velocity, and acceleration
Topic: Light Years Essential Question: How do scientists use light years to measure distances in our universe?
Key Areas covered Hubble’s law shows the relationship between the recession velocity of a galaxy and its distance from us. Hubble’s law allows us to estimate.
Time Distance Graphs Time (mins) Distance (km) E D B C
Speed, Distance, Time Calculations
Speed, Distance, Time Calculations
Natural Sciences and Technology Grade 6
Measuring the Speed of EMR
Speed, Distance, Time Calculations
Key Areas covered Hubble’s law shows the relationship between the recession velocity of a galaxy and its distance from us. Hubble’s law allows us to estimate.
The Motion of the Moon Unit 0.4.
The Universe Going the distance.
Speed, Distance, Time Calculations
MEASURING ASTRONOMICAL DISTANCES
Observing the Moon.
Time Distance Graphs Time (mins) Distance (km) E D B C
11.3 Measuring Distances in Space
Speed, Distance, Time Calculations
Presentation transcript:

Measuring the Speed of EMR Lesson 2

Objectives You will be able to Describe qualitatively some experiments measuring the speed of light Quantitatively calculate the speed of light using Michelson’s apparatus.

Speed of Sound It was known that the speed of sound was about 330 m/s. Experiment to measure speed: Person A and B are on two hills. Person A fires a cannon and drops flag. Person at B starts clock when flag dropped. Person at B hears sound and stops clock.

Speed of Light Person A and B are on two hills. Person A flashes light and starts clock. Person B sees flash and sends a flash of light back at A. Person A sees flash and stops clock. Suppose the distance from one hill to the other is 20.0 km. Using today’s accepted speed of light (3.00 x 108 m/s), calculate the time that it takes the light to go from A to B and back again.

Calculation: Clearly a time too small to measure centuries ago.

Roemer and Huygens The difficulty in showing that light had a finite speed is apparent from the example. To measure the speed of light a method of measuring very small times, or very large distances was needed. Olaus Roemer was an astronomer in 1676. He studied Io, one of Jupiter’s moons as it orbited Jupiter.

Roemer and Huygens He found that the time that Io would appear from behind Jupiter would vary. He determined that the maximum difference in time would be 22 minutes. This was due to the movement of the Earth away from Jupiter as it moves around the Sun.

Roemer and Huygens This “late” time was the time it took light to cover the extra distance.

Roemer and Huygens Roemer could not calculate the speed of light because the distance from the Earth to the Sun was not known at this time. Huygens estimated the diameter of the Earth's orbit around the Sun and used Roemer's data to calculate the speed of light. His value was about 2.0 x 108 m/s. The error was due to the error in “late time” observed by Roemer. The actual late time is 16 mins and not the 22 mins that Roemer stated.

Albert A. Michelson 1852-1931 The first accurate measurements of the speed of light were performed by A.A. Michelson. In 1926 he measured the time required for light to travel through an evacuated pipe that was constructed between two mountains 35 km apart.

Michelson’s Apparatus

Michelson’s 8 sided mirror – How it works Line everything up while the 8 sided mirror is stationary. Start to rotate the mirrors. The light will be reflected and no longer be seen in the observer’s telescope. The light will return to the same position (observed in telescope) if the mirror rotates fast enough that side B moves to exactly the same position as side C was initially in the time that it takes the light to go to the far mirror and back. (1/8 of a revolution)

Example The octagonal mirror apparatus turns at 30000 RPM and an image is observed through the telescope. Determine the time required for the mirror to go totally around once. Calculate the time for side B to get to side C. Calculate c based on this data.

Calculations

Value of c

Example Using the currently accepted value for c, calculate how far apart the two mirrors would need to be placed if the octagonal mirror is able to turn at 30 000 RPM.

Calculation

Calculation of d

Example How fast (in RPM) would a hexagonal mirror need to turn if the stationary mirror is 20.0 km from the rotating mirror? Calculation: 20.0 km is d between. Light travels 20.0 km • 2 = 40.0 km

Mirror t = 1.33… x 10-4 s is time for mirror to turn 1/6 rotation. t for full rotation = 1.33… x 10-4 s • 6 = 0.0008 s t in min = 1.33… x 10-6 min

Your Turn Read text pages 648-652 Do practice problems p. 650 check and reflect p. 652 #1-6