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Complete Astronomy Unit I "Introduction to Astronomy"

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AstronomyDad
516 Followers
Grade Levels
8th - 12th
Standards
Formats Included
  • Zip
Pages
n/a
$35.00
$35.00
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AstronomyDad
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Easel Assessment Included
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Description

Zip file of the complete intro Unit I to Astronomy A (first semester). Assessments (quizz and a unit test) with answer keys included. Assessments in this unit have been converted and can now (also) be given online and auto-graded through Easel. Graphics were added to each assessment to help with student understanding. Many student activities and worksheets are also included on Word and PDF files.

Files include three comprehensive PowerPoint lessons with up-to-date information and instructor slide sorter notes; graphics and short video links and a kahoot.it interactive quiz/review for each lesson as well as a Quizizz.com review for better individual student data analyses. Four supporting review programs with separate PDF files for printable color student guides; student outline note/guidelines for each PPT lesson; study guides including a new webquest review activity; suggested textbook assignments using the "Astronomy Today" textbook Chaisson/McMillan 8th edition (texts not included); activator questions/syllabus and other activities for beginning astronomy students.

A video worksheet folder is also included which provides the video link to youtube in the title if the DVD is not available. Worksheets include the Universe TV series "Constellations and Ancient Civilizations" and Michio Kaku's "The Physics of Everything."

All lessons/programs (not assessments) can also be found separately in the astronomydad store.

Unit I terms and concepts include:

Hubble Space Telescope, Sun, Earth, Solar system, Milky Way, galaxies, Local Group, Universe, superclusters, celestial sphere, celestial coordinates , altitude, azimuth, zenith, N / S celestial pole, celestial equator, Polaris, North Star, circumpolar stars, ecliptic, zodiac, axial tilt, solstice, equinox, seasons, precession, declination, right ascension, Astronomical Unit (AU), light year , hour angle, astrology , solar day, sidereal day, Stonehenge, Caracol, Supernova 1054 A.D., Crab Nebula, Betelgeuse , celestial sphere , geocentric model, Ptolemaic model, heliocentric model, heliocentricity, deferent, epicycle, eccentricity , retrograde motion, Mars , ellipse, focus , Aristarchus, Ptolemy , Copernicus, Tycho Brahe , Johannes Kepler, Galileo Galilei , Isaac Newton, Copernican principle, telescope, Catholic Church, Laws of Planetary Motion, Newton's Laws of Motion, action-reaction pairs, gravity, Law of Gravity

astronomydad

Complete Astronomy Unit I "Introduction to Astronomy" Zip File Updated by astronomydad is licensed under a Creative Commons Attribution 3.0 Unported License.

Total Pages
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Answer Key
Included
Teaching Duration
3 Weeks
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Standards

to see state-specific standards (only available in the US).
Follow precisely a complex multistep procedure when carrying out experiments, taking measurements, or performing technical tasks, attending to special cases or exceptions defined in the text.
Determine the meaning of symbols, key terms, and other domain-specific words and phrases as they are used in a specific scientific or technical context relevant to grades 9–10 texts and topics.
Translate quantitative or technical information expressed in words in a text into visual form (e.g., a table or chart) and translate information expressed visually or mathematically (e.g., in an equation) into words.
NGSSHS-ESS1-4
Use mathematical or computational representations to predict the motion of orbiting objects in the solar system. Emphasis is on Newtonian gravitational laws governing orbital motions, which apply to human-made satellites as well as planets and moons. Mathematical representations for the gravitational attraction of bodies and Kepler’s Laws of orbital motions should not deal with more than two bodies, nor involve calculus.
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.

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