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History and Structure of the Universe

Eric Linder - Matter and Antimatter
Dr. Linder discussed how cosmology encompasses the entire range of physics. Topics included early conditions of the universe, how inflation created topological defects, and that "freezeout" occurred sooner for weakly interacting matter. The question remains as to why there is any matter left in the universe. Lecture summary.

 

PDF of Powerpoint Presentation

Video clip: Pre-inflation
Video clip: Inflation
Video clip: Inflation as an example of a phase transition
Video clip: Post-inflation - The radiation era
Video clip: Universe freezeout
Video clip: Antimatter

 

Nao Suzuki - Tour of the Universe
Dr. Suzuki delivered a presentation about the entire universe - starting from the smallest objects to the largest. He explored the mechanisms for structure formation such as inflation, dark matter, and dark energy as they relate to the infant and current universe.

 

PDF of Powerpoint Presentation

 

Teacher Resources:

Representation of Eras - classroom lesson

Orders of Magnitude pdf
These two activities examine the immensity of the universe and the speed of light. Included are ways to review calculations involving powers of ten, unit conversions, and the concepts of speed, distance, and time.

 

Inverse Square Law - Rich Lohman

Students learned about astronomical units (arc- seconds and arc-minutes) and also explored parsec measurements by doing angle measurements of their fists. To understand parallax, students see how objects appear when viewed from different angles.

Inverse Law Powerpoint pdf

 

Light and Distance Discovery Station: Vernier Logger Pro

Dick Damian

Lights were pulled away from the light probes that were attached to a computer using the Vernier Logger Pro program.  This demonstrated the inverse square law by which the intensity of the light decreases rapidly with the distance, forming an inverse square graph.

 

Hands on Universe - Supernova Discovery

Rich Lohman used the Hands-On Universe website to guide students through astronomy concepts such as parallax, expansion of the universe, asteroid & supernovae discovery, periodic measurements, and Kepler's laws. The students processed real telescope images and made physics calculations based on the theory presented.

 

Distance - Supernovae

Type Ia supernovae are brighter than entire galaxies. The measurement of their red shift as the universe expands led to the discovery of dark energy.

 

Discovery Station: Electromagnetic Spectrum

 

Each student and teacher was given a diffraction grating slide and a handout that showed the emission spectra for various elements. They then studied the spectra of different gases emitted from arc lamps and were shown the physics behind how the lamp works. The students examined and discussed the differences they saw in the spectral lines as well as the atomic physics behind the emission and absorption of light. Many astrophysics examples were explored as practical uses for spectroscopy.

 

 

Team Media Project


 

Take a concept from cosmology and explain it in terms that a high school or middle school student would understand. Using an analogy and/or a demonstration, act out a short skit, create a rap, or design a comic book to explain the concept. Be creative. These should be two-three minutes long and everyone in the team is involved. Videos will be made of each project.

 


Final student video projects

 

 

 

Rubric for Concept Map

Students were given components of cosmology that would be used to create individual concept maps.

Concept Map Terms pdf

 

 

 

 

Day one: Cosmology for the 21st Century

Day three: History and Structure of the Universe

Day four: Standard Model of Particles and Interactions

Day five: Beyond the Standard Model of Particles and Interactions

Day six: Cosmologists for the 21st Century

 

Workshop homepage