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Absorption Line Spectra
Absorption Line Spectra
Absorption Line Spectra
Absorption Line Spectra
Absorption Line Spectra
Absorption Line Spectra
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Description

Next Generation Science Standards

Absorption Line Spectra

Different elements absorb energy at different wavelengths. By studying the light from distant stars we can learn about their composition. If a certain wavelength of energy is missing from a star's light, we can determine what elements absorbed that wavelength and therefore what element is present in the star.

This reading and coloring activity introduces the student to the basic structure of an atom. Then how absorption line spectra are created.

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Absorption Line Spectra

Rated 5 out of 5, based on 1 reviews
5.0 (1 rating)
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Digital downloads
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Grades
8th - 12th, Higher Education
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Standards
Pages
2
Teaching Duration
30 minutes

Description

Next Generation Science Standards

Absorption Line Spectra

Different elements absorb energy at different wavelengths. By studying the light from distant stars we can learn about their composition. If a certain wavelength of energy is missing from a star's light, we can determine what elements absorbed that wavelength and therefore what element is present in the star.

This reading and coloring activity introduces the student to the basic structure of an atom. Then how absorption line spectra are created.

Report this resource to TPT
Reported resources will be reviewed by our team. Report this resource to let us know if this resource violates TPT's content guidelines.

Reviews

5.0
Rated 5 out of 5, based on 1 reviews
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rating
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Rated 5 out of 5
October 16, 2022
Great visual to go with my star spectra lab. My students were very intrigued - thanks!
Julia U.
37 reviews
Grades taught: 6th

Questions & Answers

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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-ESS1-2
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).
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