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ASTR 1020 - Lab 3: Expansion of the Universe
Unrestricted Use
CC BY
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Edwin Hubble examined the spectra of many galaxies, looking for the red (longer wavelengths) or blue (shorter wavelengths) shifts in the spectra, indicating relative motion. To his surprise, not only did all of the galaxies appear to be moving, but all were moving away from us, no matter the direction of the galaxy. In addition, he found most galaxies exhibited a redshift, and the redshift was larger the further it was from our galaxy.Distant Nature: Astronomy Exercises 2016 by Stephen Tuttle under license "Creative Commons Attribution Non-Commercial Share Alike".

Subject:
Astronomy
Material Type:
Activity/Lab
Author:
Hollyanna White
Date Added:
03/04/2022
Astrophysics II
Conditional Remix & Share Permitted
CC BY-NC-SA
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This is the second course in a two-semester sequence on astrophysics. Topics include galactic dynamics, groups and clusters on galaxies, phenomenological cosmology, Newtonian cosmology, Roberston-Walker models, and galaxy formation.

Subject:
Physical Science
Physics
Material Type:
Full Course
Provider Set:
MIT OpenCourseWare
Author:
Schechter, Paul
Date Added:
09/01/2004
Beyond the Milky Way
Read the Fine Print
Educational Use
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When we look at the night sky, we see stars and the nearby planets of our own solar system. Many of those stars are actually distant galaxies and glowing clouds of dust and gases called nebulae. The universe is an immense space with distances measured in light years. The more we learn about the universe beyond our solar system, the more we realize we do not know. Students are introduced to the basic known facts about the universe, and how engineers help us explore the many mysteries of space.

Subject:
Applied Science
Astronomy
Engineering
Physical Science
Material Type:
Activity/Lab
Lesson Plan
Provider:
TeachEngineering
Provider Set:
TeachEngineering
Author:
Denise W. Carlson
Jane Evenson
Jessica Butterfield
Jessica Todd
Malinda Schaefer Zarske
Sam Semakula
Date Added:
09/18/2014
What the Doppler Effect Tells Us About Distant Stars and Planets
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Some Rights Reserved
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In this demonstration, students experience the Doppler effect for sound. Students can compute the frequency change for motion along the line of sight (LOS) and determine the vector LOS component for motions not exactly on it. A buzzer, battery, bicycle wheel, string and a rubber ball and a timer are needed for the demonstration. The resource is from PUMAS - Practical Uses of Math and Science - a collection of brief examples created by scientists and engineers showing how math and science topics taught in K-12 classes have real world applications.

Subject:
Geoscience
Physical Science
Physics
Material Type:
Simulation
Provider:
NASA
Provider Set:
NASA Wavelength
Date Added:
11/05/2014