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Star Spectroscopy/Electromagnetic Spectrum Lab: Online Simulation Edition

Rated 4.44 out of 5, based on 16 reviews
4.4 (16 ratings)
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Teaching STEAM
89 Followers
Grade Levels
9th - 12th
Resource Type
Standards
Formats Included
  • Google Docs™
  • Internet Activities
Pages
14 pages
$4.00
$4.00
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Teaching STEAM
89 Followers
Made for Google Drive™
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What educators are saying

Great resource to help Earth Science students learn these concepts and skills. Students enjoyed this activity and it helped bring them to a better understanding of the content.
I have been trying to find something like this for awhile that is easy for my students to manipulate! This did the trick!

Description

Spectroscopy is how we know what elements are in stars. This lab is awesome connecting students to how star science works. It also makes spectroscopy real in chemistry class, physics, astronomy, and general science about the electromagnetic spectrum. My students loved this activity solo and over Zoom. They felt that they learned how we use spectroscopy and have a deeper understanding of the electromagnetic spectrum.

This activity is an online simulation version of Star Spectroscopy/Electromagnetic Spectrum Lab and is perfect for remote learners or if your school does not have the equipment.

I also like to go through the development of telescopes and begin with Build a Telescope Lab: Reflection and Refraction Fun!

You may also be interested in Modeling Fusion Activity.

Total Pages
14 pages
Answer Key
N/A
Teaching Duration
90 minutes
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Standards

to see state-specific standards (only available in the US).
NGSSHS-ESS1-3
Communicate scientific ideas about the way stars, over their life cycle, produce elements. Emphasis is on the way nucleosynthesis, and therefore the different elements created, varies as a function of the mass of a star and the stage of its lifetime. Details of the many different nucleosynthesis pathways for stars of differing masses are not assessed.
NGSSHS-ESS1-1
Develop a model based on evidence to illustrate the life span of the sun and the role of nuclear fusion in the sun’s core to release energy that eventually reaches Earth in the form of radiation. Emphasis is on the energy transfer mechanisms that allow energy from nuclear fusion in the sun’s core to reach Earth. Examples of evidence for the model include observations of the masses and lifetimes of other stars, as well as the ways that the sun’s radiation varies due to sudden solar flares (“space weather”), the 11-year sunspot cycle, and non-cyclic variations over centuries. Assessment does not include details of the atomic and sub-atomic processes involved with the sun’s nuclear fusion.
NGSSHS-ESS1-2
Construct an explanation of the Big Bang theory based on astronomical evidence of light spectra, motion of distant galaxies, and composition of matter in the universe. Emphasis is on the astronomical evidence of the red shift of light from galaxies as an indication that the universe is currently expanding, the cosmic microwave background as the remnant radiation from the Big Bang, and the observed composition of ordinary matter of the universe, primarily found in stars and interstellar gases (from the spectra of electromagnetic radiation from stars), which matches that predicted by the Big Bang theory (3/4 hydrogen and 1/4 helium).
NGSSHS-PS4-1
Use mathematical representations to support a claim regarding relationships among the frequency, wavelength, and speed of waves traveling in various media. Examples of data could include electromagnetic radiation traveling in a vacuum and glass, sound waves traveling through air and water, and seismic waves traveling through the earth. Assessment is limited to algebraic relationships and describing those relationships qualitatively.

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89 Followers