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Google Arts & Culture “What is the James Webb Space Telescope?” PDF

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Mrs Glitterski Classroom
7 Followers
Grade Levels
6th - 12th
Standards
Formats Included
  • PDF
  • Internet Activities
Pages
1 page
$1.75
$1.75
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Mrs Glitterski Classroom
7 Followers
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  1. The resources in this bundle are all internet resources with links and the accompanying worksheet.
    Price $5.99Original Price $7.00Save $1.01

Description

This worksheet will walk students through the article. The questions are in the order of the article.

Total Pages
1 page
Answer Key
Not Included
Teaching Duration
30 minutes
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Standards

to see state-specific standards (only available in the US).
NGSSMS-ESS1-2
Develop and use a model to describe the role of gravity in the motions within galaxies and the solar system. Emphasis for the model is on gravity as the force that holds together the solar system and Milky Way galaxy and controls orbital motions within them. Examples of models can be physical (such as the analogy of distance along a football field or computer visualizations of elliptical orbits) or conceptual (such as mathematical proportions relative to the size of familiar objects such as students’ school or state). Assessment does not include Kepler’s Laws of orbital motion or the apparent retrograde motion of the planets as viewed from Earth.
NGSSMS-ESS1-3
Analyze and interpret data to determine scale properties of objects in the solar system. Emphasis is on the analysis of data from Earth-based instruments, space-based telescopes, and spacecraft to determine similarities and differences among solar system objects. Examples of scale properties include the sizes of an object’s layers (such as crust and atmosphere), surface features (such as volcanoes), and orbital radius. Examples of data include statistical information, drawings and photographs, and models. Assessment does not include recalling facts about properties of the planets and other solar system bodies.
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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