| |
| |
|
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.) |
|
|
Back to top |
|
| Materials |
| For each student |
- Copy of the Student Texts One through Nine, “Tracing
the Origins of Quarks”
- Copy of the Glossaries that accompany the Student
Texts, “Tracing the Origins of Quarks”
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

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:
- Student Texts One through Nine, Tracing the Origins of Quarks”
- 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.
|
Back to top |
|
| 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.
|
Back to top |
|
Procedure |
Distribute
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
their
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.
- What is the
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.]
- 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.]
- 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.]
- 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?
- What kind of force holds electrons in atoms?
[electromagnetic]
- During what epochs were electrons found
as free particles? [from Epoch 2 to Epoch 7]
- What kind of force holds quarks in protons
and neutrons? [strong nuclear forces (gluons)]
During
what epochs were quarks found as free particles? [from Epoch
2 to Epoch 4]
- 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]
- 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]
- 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.]
- 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?]
- 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.
- 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 examine
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.] |
Back to top |
|
Back to top
Back to Evolving Universe Overview
|
| |