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  Teacher Guide: Tracing The Origins of Our Universe
 

Cosmology
Background Information
This Tracing Origins activity is the third in a series of three “Thought Experiments.” Scientists use thought experiments when it is not possible to actually conduct real experiments with real equipment.

In Activity 1, students traced the origins of pizza ingredients back to atoms, the building blocks of matter. But atoms have their own building blocks—protons, neutrons, and electrons. And protons and neutrons have their own “fundamental particles”—quarks.

In Activity 2, students explored the characteristics of quarks. Quarks and electrons may have been among the first stable particles formed in the early universe. Most students know something about the characteristics of electrons, but few of them know about quarks or their characteristics.

If electrons are free, stable particles in today’s universe, why aren’t quarks? This question is the basis for this final activity of the series, “Tracing the Origins of Our Universe.” Students will combine the “tracing process” they used in the first activity to trace quarks and electrons backwards in time to discover what important role these fundamental particles may have played in those early cosmic periods when the universe was in a state of high density and high energy. This activity will engage students in a discussion of the energy (temperature) changes that have occurred from the beginning of the cosmos until now.

National Science Education Standards Addressed
Grades 5–8
Science As Inquiry
  • Understands about scientific inquiry
Physical Science
  • Properties and changes of properties in matter
  • Transfer of energy

Science and Technology

  • Understandings about science and technology
History and Nature of Science
  • Nature of science and scientific knowledge
  • History of science and historical perspective
Grades 9-12 Science As Inquiry
  • Understands about scientific inquiry
Earth and Space Science
  • The origin and evolution of the universe
Physical Science
  • Structure of atoms
  • Motions and forces
  • Interactions of energy and matter
Science and Technology
  • Understandings about science and technology
History and Nature of Science
  • Nature of science and scientific knowledge
  • History of science and historical perspective
(View the full text of the National Science Education Standards.)

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Materials
For each student

The Student Activity and Student Text materials are available for use with audio-amplified computer software, 14-point font print copy for partially sighted students, and in Braille for significantly sight-impaired students. You may select the most appropriate version of these materials by following these directions.

Note that there are two forms of the Student Texts and Student Activity available. One includes the phonetic pronunciation of glossary terms and is written in paragraph form for large print hard copy readers. The other is suitable for screen readers or braille transcription. It does not contain the phonetic pronunciation.

An audio tape that contains the student activity the two student texts, and glossaries is also available.

You may wish to have headsets to use with screen-reading students.

  • One set of Eight Epochs tactile cards
    Text Box: Optional

These can be obtained free of charge by downloading the PDF template at insert URL here. You can then make thermally-enhanced copies for your students. Follow the directions for doing this at or you may request The Eight Epochs Card Set, is available at cost.

  • Prepare a set of “Density Balls” for use in the post-discussion session.

Epoch 8 can be modeled using a beach ball about 30 cm in diameter ( »51 cm in circumference). Inflated it has a mass of » 79 grams.

Epoch 7 can be modeled using a styrofoam ball that is 12 cm in diameter. Open the ball and add enough modeling clay bring mass very close to 79 grams.

Epoch 6 can be modeled with 4-cm ball of modeling clay (or a plastic toy golf ball with enough b-b’s to bring the mass to 79 grams.)

Epoch 5 is a 2.4 cm steel ball bearing. This may have a mass that is slightly less than 79 grams.

  • A set of double pan balances to confirm the masses of the balls.

Getting Ready
  • Before class make copies of the following handout in the form most appropriate for each of your students:
    1. Student Texts One through Nine, Tracing the Origins of Quarks”
    2. Glossaries that accompany the Student Texts, “Tracing the Origins of Quarks”
  • Preview the text material in Braille and using your audio-amplified computer software. Give your visually-impaired students any instructions they need to take advantage of their appropriate learning aids.
  • Prepare (or order) a set of the thermally-enhanced tactile cards for each student.
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Background for Tracing the Origins of our Universe

In the Student Text, “Tracing the Origins of Quarks," we have chosen to trace the origins of quarks by running the movie of the beginning of the universe “in reverse.” During this time the universe is getting smaller and smaller. If you continue this process back in time, you come to a point where the mass of the universe is “crammed” into an infinitely dense point. At this time, matter is thought to have been a mixture of quarks, leptons (particles, including electrons, that are not influenced by the strong nuclear force), and theoretical particles, which may have been the source of quarks (and antiquarks).

Where did the particles in the “primal stew” come from? If we had an answer to this question, we would have insight into the beginning of the universe. They may have been produced from energy during the second, very brief epoch or during the Mysterious Epoch immediately preceding it, when the universe was very compact and temperatures were very high. This is in agreement with a premise of the standard cosmological model that the early universe was in a state of high density and high energy.

If this is the case, then matter is frozen energy. The universe, which began in a high-energy state, has been cooling off ever since and hot energy congealed into cold matter. We continue to study quarks in this activity because they appear to be one the first forms of matter in the universe and they are still present today. Not only are they fundamental particles of matter, but they also played a vital role in the formation of atoms and molecules that form the vast structures of today’s universe.

As your students work with this model, emphasize that it is consistent with observations of chemical constituents in the universe. These observations include studies of young and old stars; planetary nebulae; shells of gas ejected by unstable stars; glowing gas clouds; lunar soil samples that Apollo astronauts brought to Earth; and particles of solar wind gathered by sheets of aluminum foil deployed on the surface of the moon. The observed abundances of hydrogen and helium in space match the abundances of those elements predicted from this model.

This model is also consistent with known physical laws and properties of fundamental forces. Examples include the fact that the temperature of matter decreases as it expands (so the reverse would be true as matter condenses) and that the fundamental attractive forces have different strengths and operate through different distances.

As you guide your students through this activity, continue to use the background material in “The Universe is Expanding” and “Remnants of the Big Bang” sections of Appendix A from the original Cosmic Chemistry: Cosmogony module.

For additional background reading, see Appendix A and Appendix C, Student Texts, “The Invisible Fire” and “ Models in Science” from Cosmic Chemistry: Sun and Solar Wind.

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Procedure

  • Text Box: Clarifying TerminologyDistribute copies of the nine Student Texts, “Tracing the Origins of Quarks” and the accompanying set of tactile cards in the appropriate form for each of the students in your class. You may distribute them one at a time and discuss the contents after each one or give students all of them at one time and make them a reading assignment prior to your next classroom discussion.

Regardless of which method you choose for distributing these materials, the follow-up sessions should concentrate on the critical factors that change as we go backwards in time. These include the time span of epoch; the temperature changes during epoch; the form of matter in the epoch; and the location and relative freedom of quarks and electrons during the epoch.

We have organized these factors into the following table for your reference and convenience.

  • Students should have Student and Tactile cardstheir tactile card sets available and arranged in order on their desks as they answer the classroom discussion questions. You may also wish them to use their student texts for reference during this time.
  • Use questions like the following questions as the basis for your classroom discussion and for student assessment for the Tracing the Origins of Our Universe activity.
    1. What is theStudent and Tactile cards 2 basis of the descriptions of the different epochs of the universe? [Epochs are based on models that incorporate observations of the universe today, descriptive mathematics, and fundamental laws of physics.]
    2. Do we KNOW that these descriptions are accurate? What questions do we have concerning their accuracy? [No, we can only say that that these descriptions are consistent with what we know about the universe today and the physical laws that are in operation today.]
    3. What is the trend in the temperature of the universe from the first to eight epoch? [it decreased] Why do we think that the temperature decreased during this time?

      [We have observed that the universe today is expanding and this expansion is accompanied by a decrease in temperature, consistent with the laws of thermodynamics. We assume that this trend is a continuation of the temperature changes that occurred in the early universe.]

    4. What role do you think decreasing temperatures played in the changes in constituents of the universe from the beginning to the present epoch? [Help students understand the direct relationship between temperature and energy. Have them trace the temperature changes and the constituents of different epochs by answering these specific questions?
      1. What kind of force holds electrons in atoms? [electromagnetic]
      2. During what epochs were electrons found as free particles? [from Epoch 2 to Epoch 7]
      3. What kind of force holds quarks in protons and neutrons? [strong nuclear forces (gluons)]
      4. The Epoch 6 Tactile Card shows a helium nuclei decomposing into two Deuterium ions.  During what epochs were quarks found as free particles? [from Epoch 2 to Epoch 4]
      5. Which kind of force—electromagnetic or strong nuclear force—do you think is the stronger? Why? [strong nuclear force because the temperature had to be higher to overcome strong nuclear forces than it did to overcome electromagnetic force]
    5. What is the trend in the length of time for epochs as you go from Epoch 1 to Epoch 8? [the epochs get longer, but there doesn’t seem to be a mathematical relationship]
    6. What is happening to the size of the universe as we go backward from the current epoch to the first epoch? Why do we think this is correct? [The size decreases. We have observed that the universe today is expanding. This expansion may just be an extension of the original trend.]
    7. Ask students how they “visualize” the size of the universe during the first epoch. [There are models that say that the universe was just a pinpoint of matter. There are others that say that say that the universe was all energy from which matter was formed. What do your students think is the correct model?]
    8. Ask students whether or not they think this epoch model of the universe is plausible or not? They should have reasons for their answers, rather than just “yes” or “no” responses. Accept their answers without bias, asking only questions that help clarify their reasons.
    9. Ask students what other information they might want to have before giving unqualified support to this epoch model.

Changes in density through the Epochs

This would be a good opportunity to have students address the density changes that occurred during the epochs. Have students examinestudents arrange the balls according to their masses a set of “Density Balls” that have the same mass in different volumes.

Have students arrange the balls according their masses. [Students will probably think that the steel ball bearing has the most mass. However, this ball is exerting the most force on the smallest area so it only FEELS like it has the most mass.]

Use double-pan balances to show students that all the balls have the same mass. Then tell them that these balls model the size of Epochs 5, 6, 7, and 8. Emphasize that the mass, the amount of matter in the universe, did not change as it went through the epochs.

Now have students arrange these balls in order of size. Then ask:

  • Which of these balls would model Epoch 8? [Beach ball]
  • Which of these balls would model Epoch 7? [Plastic ball]
  • Which of the balls models Epoch 6? [Clay ball]

That leaves steel ball bearing to model Epoch 5.

Now ask, if the density is the amount of matter in a given volume, in which of the Epochs was matter the least dense? [In Epoch 8, 79 grams are contained in the largest volume.]

In which of these Epochs was matter the most dense? [Matter is the most dense in Epoch 5 because the same amount of matter is compressed into the smallest volume.]

What is trend in density of matter as you go back in time from Epoch 8 to Epoch 5? [The density increases.]

Do you think this trend in density continued through Epochs 4 through 1 when matter was in the physical state of plasma? [Accept student answers without comment.]

Plasma is a gas made of charged particles. Scientists have found that when you compress a gas, the temperature of the gas increases. How does the temperature change as we trace the change in the Universe back through Epochs 4, 3, 2, and to Epoch 1?

Are these changes in the Universe density, temperature, and size through the Epochs consistent with what we know about the physical laws today? [Help students to see that the characteristics they have been studying are consistent with the physical laws that govern matter and energy today.]

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