A Field Trip Package for the LIGO Hanford Observatory





Some notes for the teacher
Relationships between Teachers Corner Packages and LIGO Explorer activities
A student field trip handout - the LIGO Explorer (Web copy)
A downloadable MS Word version of the LIGO Explorer
The LIGO Explorer Teachers Guide (Web copy)
A visit evaluation for teachers

LIGO Field Trip Notes for the Teacher

We appreciate your efforts to plan a trip to the LIGO Hanford Observatory . Here is some information that may assist your preparations.



Teachers Corner Classroom PackageRelated LIGO Field Trip ExhibitScience Themes of the Package or ExhibitAdditional LIGO aspects of the exhibit
Scaling the Layers of the Earth's AtmosphereJourney to the StarsScale relationships in the use of modelsLIGO tries to 'listen' to events and processes that may happen millions or billions of light years away
The LIGO Star ChartJourney to the StarsRelative locations of stars & constellations in the night skyThe sky is LIGO's laboratory. Learn your way around the lab.
Build and Use a Simple SpectroscopeScoping the StarsThe nature of light & the spectroscopy of visible light sourcesThe LIGO interferometers are light-based instruments, but LIGO, unlike a spectroscope, is not a light wave detector. LIGO is a gravitational wave detector.
Build and Use Your Own Michelson InterferometerThe Little Michelson Interferometer (similar to the Package model but a bit fancier)Light interference; the nature of laser light; interferometers as measurement instrumentsLIGO interferometers use the basic design of a Michelson, but are very large and very complex instruments
The Scientific Method with A PendulumA Pendulum is One Type of Falling Object; Heavy as a Rock, Lght as a Feather (Free-fall Tube)The nature of gravity & the nature of scienceEinstein's relativity-based model of space and time forms the foundation of LIGO's explorations of the universe
Powers of TwoFilm: Powers of Ten (The film is not part of the LIGO Explorer but we would be happy to show it at the teacher's request)The difference between linear and exponential relationshipsThe extraordinary magnitudes of many LIGO quantities (both large and small) make exponential and logarithmic relations essential for our work.



A HANDOUT FOR STUDENTS


The LIGO Explorer


To the student: This activity sheet will take you through a number of the exhibits at the LIGO Hanford Observatory. Here's what you should do:


Scoping the Stars

Location: In the Auditorium (This exhibit is under construction and may not be ready during your trip)
Procedure: Point the narrow opening of your spectroscope at the various light sources that are in the room and look into the scope through the diffraction grating (the slide on the other end of the box). Look at the patterns inside the box. Compare the patterns of different light sources to each other
Questions
  1. What type of spectral pattern do you see when you look at white light?

  2. How do the patterns from the colored lights differ from the pattern of the white light?

  3. If all you could see was a spectral pattern and you couldn't see the light that produced the pattern, could you figure out the color of the light from the pattern? Explain.


A Shadow - More than Meets the Eye?

Location: In the Auditorium
Procedure: A special set of ceiling lights needs to on for this exhibit. If those lights are on, stand a few feet in front of the front wall of the auditorium so that you cast shadows on the wall. Move from side to side and watch your shadows. Note: Please don't put your hands on the wall itself. The wall is our projector screen and we need to keep it spanking clean. Thank you!
Questions
  1. List all seven colors of shadows you can see at this exhibit.

  2. Explain how you think a blue shadow is produced on the wall.

  3. Explain how you think a magenta (purple) shadow is produced on the wall.

  4. What combinations of colors produce yellow light?


An Antenna That Won't Fit on Your Car

Location: The front of the common area (the large aluminum cylinder)
Procedure: At this station you will read the printed material about Joseph Weber's aluminum bar gravitational wave detector.
Questions
  1. What kind of experiments did Dr. Weber do with this bar? What was he trying to discover?

  2. Why do you think the bar is sometimes referred to as an antenna? (You may need to ask someone how the antenna on your car works)

  3. What does the bar have in common with LIGO?


A Pendulum is One Type of Falling Object

Location: The back of the auditorium
Procedure: Weigh one of the colored sacks on the spring scale, put the sack in the pendulum and measure the time that is needed for ten full swings. Repeat this with process with the other two sacks and fill in the data table.

Color of BagWeight of BagTime needed for 10 swings (seconds)
   
   
   

Questions
  1. Everyone knows that pendulums swing. Why do we say that a pendulum also falls?

  2. Is it important to keep the lid on the pendulum while it swings? Give a reason for your answer

  3. Does a heavy pendulum fall at about the same rate as a light pendulum? What does this tell us about gravity?


The Little Michelson Interferometer

Location: In the front of the common area across from the Weber Bar
Procedure: The laser pen in the interferometer should be on. Look at the poster on the wall behind the display to learn how the light travels through the interferometer. Look at the interference pattern that the light beams create on the white screen. The stripes in the pattern are called fringes. Step hard on the floor and watch the fringes.
Questions
  1. An interferometer such as this can be used as a very sensitive measuring tool. From observing the device can you see why this is true?

  2. Why is an interferometer an important exhibit to have here at LIGO?


Learn More About LIGO

Location: The LIGO posters on display near the auditorium entrance
Procedure: Scan the information on the posters of find answers to these questions
Questions
  1. What are some ways that gravitational waves can be produced?

  2. What contribution did Einstein make to our understanding of gravitational waves?


Heavy as a Rock, Light as a Feather: How Do They Fall?

Location: In the rear corner of the common area next to the window (This exhibit is under construction and may not be ready during your trip)
Procedure: A feather and a heavy little ball are inside the transparent vertical plastic tube. The ball and the feather need to be placed on the shelf at the top of the tube. A power switch on the outside of the exhibit controls the shelf. When you throw the switch, the shelf drops and the ball and feather fall to the bottom of the tube.

Place the ball and feather on the shelf, close the tube and throw the switch. Compare the way the ball and the feather fall to the bottom of the tube. Now place the feather and ball back on the shelf and turn on the vacuum pump that is connected to the tube. The vacuum tube will remove all of the air from the tube. Set the timer for three minutes. Turn off the pump at the end of three minutes. Throw the shelf switch and again compare the way that the feather and ball fall to the bottom of the tube. Finish by venting the tube to let the air return to the inside.


Questions
  1. Based on what you've seen here, why do people often think that heavier objects fall faster than light objects?

  2. What is responsible for making the feather fall so slowly?

  3. What does the display teach us about gravity? Does gravity cause objects to fall at the same rate or different rates?

  4. Is the pull (the force) of gravity the same on light objects as on heavy objects? Explain your thinking.

To Our Galaxy and Beyond

Location: The photographs for this exhibit are mounted on the upper front wall of the common area. Explanations are mounted next to the images.
Procedure: Look at the Hubble Telescope images that are mounted on the upper wall of the common area. Observe the differences between them. Read the explanations that accompany the images.
Questions
  1. What is a Nebula?

  2. How far away is the farthest object that is mentioned in the explanations?

  3. Which images do you like the best? Why?

  4. What thoughts about the universe do you have from looking at the images?


Physics History

Location: The series of posters on the rear wall of the auditorium.
Procedure: Take some time to read the posters that are on the rear wall of the auditorium. These describe many of the important people and events in the physics of the last century. Identify four people whose work is described in the posters. Your list should include both genders, each person should come from a different country and each person should be discussed in a different decade.
Questions
  1. Scientist 1 (name, gender, country of origin, decade, contribution):

  2. Scientist 2:

  3. Scientist 3:

  4. Scientist 4:


Journey To The Stars

Location: The galaxy model is outside the building. The computer tutorial is inside.

First you will learn to locate a star that is expected to supernova within the next 10,000 years!
  1. Log onto the constellation tutorial on the computer in the common area.

  2. Spend a few minutes learning to locate the star Betelgeuse in the constellation Orion.

  3. Please locate and circle Betelgeuse in each of the diagrams below:


 

Now you will determine the distances from the Earth to 6 prominent stars in the Milky Way Galaxy.

Please go to the earth's solar system indicator located outside, at the front corner of the building. We have carefully plotted points on the LIGO grounds to represent 6 stars and their relative distances from the earth. But how are you going to measure these distances?

Starting at the earth's solar system indicator, carefully count the number of steps it takes you to walk out to the star "Merak" located in the Big Dipper. (You are now using each of your step lengths as a unit of measure so make each step as identical in length as possible).

Number of steps = ________

Because the distances to the stars are so huge it is very difficult to measure them using miles or kilometers. For example Merak is 475 trillion miles from the earth! It is much easier to measure these distances in light years. (A light year is the distance a beam of light will travel in one year. This is a significant distance considering light travels 186,000 miles in just one second!)

If Merak is 80 light years away, and it took _______ steps to get from the earth to Merak, then_______light years represents one of your steps.

Now determine the estimated distance to each of the 5 remaining stars by counting the number of steps it takes you to walk from the earth's solar system marker to the stars in each constellation. Complete the table on the next page with your data.

Write your Scaling Ratio here: _____ light years per step

Name of Constellation or "Group of Stars"Name of StarFacts about the Star# of your steps# of light years from earth
MerakHot white star. The light you see from this star took 80 years to reach the earth. 80
DubheIs orbited by another less massive star   
RuchbahAbout four times as big as the sun  
SchedarA very young star, about 200,000,000 years old  
BellatrixWill become an orange giant in a few million years. Then die quietly as a massive white dwarf.  
Betelgeuse("beetle juice")Red super giant. If Betelgeuse replaced our sun, the surface of the star would reach out beyond the asteroid belt. Betelgeuse is 60,000 times brighter than the sun  


Attraction Action

Location: Rear of the common area by the window (This exhibit is under construction and may not be ready during your trip)
Procedure: Roll one of the balls into the bowl. Make careful observations.
Questions
  1. What will happen if you just set the ball near the rim and let it go without propelling it forward?

  2. If you set the ball near the rim and propel it straight forward, what path will it follow? Why?

  3. Why does the ball's orbit shrink as it continues to roll around? Does this factor affect the earth's orbit? Why not?

  4. Now propel the ball towards but not straight at the center hole. Describe the path of the ball.

  5. The poster on the wall behind this exhibit describes some very smart and famous people. What are the possible reasons why these people presented different facts about the nature of gravity?
    1. Famous, smart people tell a lot of lies
    2. Famous, smart people always find stuff to argue over
    3. The way gravity behaves has been changing over the course of history
    4. The facts we think we know change over time as people learn new things or find better ways to explain the way things behave.

When You Are Finished

Your teacher will collect your Explorer packets - he or she will give you instructions on how this is to be done. Someone will tell you where you can leave your clipboard. Please make sure that you take any personal items you may have brought, such as pencils, pens, calculators, hats, etc.

Thank you for coming to LIGO! We hope that you had an enjoyable and educational visit!

Back to Teachers Corner


Last modified January 26, 2005
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