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Cosmogony
This science module focuses on the origin and evolution of the universe. If you are using Genesis science modules for the first time, read the User's Guide thoroughly before you begin. (View User's Guide as a PDF.)

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Take a look at other science modules available. All technical terms in the science modules are compiled in the Glossary for easy access. Tech Apps

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Cosmogony

Cosmogony
Cosmologists study the present universe, while cosmogonists study the origin of the universe. Observations about our present universe not only allow predictions of the future, but they also provide clues to events that happened long ago when the chemical evolution of the cosmos began. Throughout this module, students study models, especially mathematical models, since many features of the universe are minimally observable or only presumed to exist based on indirect evidence. They develop an understanding of the difficulties of conducting science on the scale of the universe and of the need to escape from our earthbound frame of reference. Classroom activities examine some aspects of the contemporary models of the origin of the universe, the concepts of time and distance, and the strategy of working backward from a known final state to a reasonable initial state.

Student Mission
Students will explore the inferences that can be made from the limited set of cosmological data available, including that from deep space, to gain an appreciation for the enormous difficulties faced by cosmologists as they attempt to define and describe our universe. They will develop an awareness of some of the "missing pieces" in the overall picture.

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Teacher Resources
For a listing of additional resources that includes URLs, books, and periodicals, click here.

 
PDF Icon Module Overview
PDF Icon Module Planning Guide
Module
Briefing
Cosmogony or Cosmology?
PDF Icon Teacher Text

Incorporated
The primary objective of the Genesis mission is to collect samples of solar wind particles and return them to the Earth for detailed analysis. Precise analysis of these particles will provide solar isotopic and elemental abundances, and thus will form a basis for testing models of solar system formation, evolution, and early nebular composition.

These solar system models ultimately must fit in with models of the formation of the universe, as tiny parts of the whole, but ones for which comparatively complete data exists. The information obtained from the Genesis mission pertaining to the primordial solar system should ultimately prove useful to cosmologists and cosmogonists, since the solar system is thought to have originated from a disk-shaped cloud of gas and dust when the universe was about two-thirds its current age. Thus, the Genesis mission becomes a part of the necessary cosmological strategy of working backwards through time toward a beginning.


Curriculum Connections
National Standards Addressed

National Science Education Standards

Grades 5-8

Science as Inquiry

  • Understandings about scientific inquiry
Physical Science
  • Properties and changes of properties in matter
  • Motions and Forces
  • Transfer of Energy
Earth and Space Science
  • Structure of the Earth System
  • Earth in the Solar System
  • Origin and Evolution of the Universe
Science and Technology
  • Understandings about Science and Technology
History and Nature of Science
  • Science as a Human Endeavor
  • Nature of Science
  • History of Science

Curriculum Connections
National Standards Addressed

National Science Education Standards

Grades 9-12

Science as Inquiry

  • Abilities necessary to do scientific inquiry
  • Understandings about scientific inquiry
Physical Science
  • Structure of Atoms
  • Motion and Forces
  • Structure and Properties of Matter
  • Interactions of Energy and Matter
Earth and Space Science
  • The Origin and Evolution of the Earth System
  • The Origin and Evolution of the Universe
Science and Technology
  • Understandings about Science and Technology
History and Nature of Science
  • Science as a Human Endeavor
  • Nature of Scientific Knowledge
  • Historical Perspectives

Module
Exploration
Mathematical Models
PDF Icon Teacher Guide
PDF Icon Student Activity
PDF Icon Anticipation Guide
PDF Icon Appendix A
PDF Icon Appendix B

Density and Gravity-The Push and Pull of the Universe
PDF Icon Teacher Guide
PDF Icon Student Activity
PDF Icon Student Data/Reporting Sheet
PDF Icon Anticipation Guide
PDF Icon Student Text

Doppler Effect-Are You Coming or Going?
PDF Icon Teacher Guide
PDF Icon Student Data/Reporting Sheet
PDF Icon Student Handout
PDF Icon Student Activity
PDF Icon Student Text

Quarks-Getting Down to Fundamentals
PDF Icon Teacher Guide
PDF Icon Teacher Tools
PDF Icon Student Activity, Part I
PDF Icon Student Activity, Part II
PDF Icon Student Activity, Part III
PDF Icon Student Text

Thought Experiments: Tracing Origins
PDF Icon Student Text
PDF Icon Student Handout
In the activities of this module, the teacher's primary role is Socratic. Through effective questioning, students should become aware of the relationship between what scientists observe and the theories and models that they develop from the observations.

The Student Activity, "Mathematical Models," emphasizes the fact that cosmology is, of necessity, a mathematical science, and it illustrates the power of mathematics to organize our thoughts and to direct the course of future investigations. During this activity, students should be guided to an understanding of the various kinds of models used by scientists and how observations are converted into useful logic-based models.

The Student Activity, "Density and Gravity-The Push and the Pull of the Universe," focuses on the importance of a very simple concept (gravity) to cosmological thought while stressing the difficulty of determining the density of something as vast and poorly defined as the universe. The part of this activity dealing with gravity is designed to underline the crucial role that this extremely weak force plays in determining the structure of the universe.

The Student Activity, "Doppler Effect-Are You Coming or Going?" Doppler Effectillustrates the application of a simple technique that has been a mainstay of cosmological science since the early part of the 20th century. After students develop a physical model that simulates the Doppler effect, they proceed to explore some actual cosmic Doppler data and draw conclusions based on these observations.

The Student Activity, "Quarks-Getting Down to Fundamentals," focuses the students' attention on extrapolations into the unknown by inference. The inferred information is used to build models consistent with observable contemporary data about fundamental particles and how this matter relates to the origin of the universe.

Module
Development
A Spongy Universe
PDF Icon Teacher Guide
PDF Icon Student Activity
PDF Icon Student Text

Dark Matter-More Than Meets the Eye
PDF Icon Teacher Guide
PDF Icon Student Activity
PDF Icon Student Text
PDF Icon Appendix C
PowerPoint Power Point
PDF Icon PowerPoint as PDF
PDF Icon Teacher Guide for PowerPoint
PDF Icon Teacher Notes for PowerPoint

Use the Student Activities, "A Spongy Universe" Spongy Universeand "Dark Matter-More Than Meets the Eye" to create interest in learning more about the structure of the universe and the models that are now being considered. The "Spongy Universe" activity emphasizes two things. The first is that how we view things often depends on our perspective, and the second is how our view of the universe from here in the solar system is very limited by our perspective.

StarsThe "Dark Matter" activity encourages students to wrestle with the difficulties faced by scientists when they do not have information on which to base models. The activity also focuses on the intellectual developments that are necessary in order to address these obstacles. Galaxy

Module
Interaction/Synthesis
Incorporated

Students interact with peers to accomplish the tasks assigned in the Rotating GalaxyExploration and Development sections above. Each activity contains work to be done in groups, with the whole class participating in preliminary and summary discussions.


Module
Assessment
Cosmic Tug of War
PDF Icon Teacher Guide
PDF Icon Student Activity
PDF Icon Student Text

In the assessment activity, "Cosmic Tug of War," students are asked to decide which of two cosmic forces (expansion and gravity) will dominate the future of the universe. In addition to their background from the Exploration and Development activities of the module, they will use the more quantitative information in the student text for the Assessment activity and the references for the module to make and defend their decisions. Students may also be required to make physical models of the future universe.


Curriculum Connections
National Standards Addressed

National Science Education Standards

Assessment Standard B

  • Achievement and Opportunity to Learn Science must be Assessed

Assessment Standard C

  • Assessment Tasks Are Authentic

McREL
This education module, Cosmic Chemistry: Cosmogony, was developed by educators at Mid-continent Research for Education and Learning.
Writers:
~Dr. Donna Bogner
~Dr. B.J. McCormick
Contributing Writer:
~John Ristvey, McREL
Graphics:

~Judy Counley, McREL

Layout:

~Susanne Chastain, McREL
~Amy Hoza, McREL

Special thanks to the following reviewers:

~Dr. Gil Yanow, Jet Propulsion Laboratory
~Dr. Monika Kress, NASA Ames Research Center
~Mark Rose, Maplewood Junior & Senior High School, PA
~Alice Krueger, McREL
~Jacinta Behne, McREL
~Deb Jordan, McREL

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