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NGSS Scale History of the Universe HS-ESS1-1 MS-ESS1-3 Activity Includes Spanish

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Williams Hands On Science
1.5k Followers
Grade Levels
6th - 12th, Homeschool
Standards
Formats Included
  • Google Slides™
Pages
40 pages
$5.00
$5.00
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Description

After this activity your students will have a much deeper understanding of how our universe started and how the solar system and life evolved into what it is today! It’s interactive, inquiry based, metacognitive and integrated NGSS!!! I highly recommend you purchase The Universe and Its Stars in my store. It’s only $2.99 and it’s a perfect scaffold for this resource. Another great resource to accompany this one is Scale of the Universe. It teaches students how big objects are and their distances from earth. I teach that first and then follow up with this resource, which teaches students how everything formed.


AND! It includes a Spanish version for your ESL/ELL/Newcomer students!


You can do this lesson all online, hard copies, or a combination of both. I also have it formatted to have a notebooking option.

What Students do:
-Students use prior knowledge to guess the events that occurred from the Big Bang till now
-Students sort cards with major events on them
-As students watch a very engaging video, students rearrange the cards in the correct order.
-Students then glue cards on to a timeline that gives them a great perspective as to how the universe, matter, stars, the solar system and life on earth formed. The timeline is great a making students think critically and to recognize patterns in the formation of the universe and its stars.

Concepts Included:
Scale and Patterns
Formation & Age of the Universe
Formation of Matter
Formation of the Stars, Galaxies & Planets
Formation of the Solar System
Formation of the Earth and Life on Earth
Goldilocks Effect

This resource includes the following:
-Student Handout
-Teacher slides with detailed teacher Notes for pacing, classroom discussions and classroom management
-Cards and timeline for notebooking or handouts

-Spanish Version

NGSS Disciplinary Core Idea (DCI) Middle School:
ESS1.A:  The Universe and Its Stars
• Earth and its solar system are part of the Milky Way galaxy, which is one of many galaxies in the universe. (MS-ESS1-2)
ESS1.B:  Earth and the Solar System
• The solar system consists of the sun and a collection of objects, including planets, their moons, and asteroids that are held in orbit around the sun by its gravitational pull on them. (MS-ESS1-2), (MS-ESS1-3)
ESS2.A:  Earth Materials and Systems
• The planet’s systems interact over scales that range from microscopic to global in size, and they operate over fractions of a second to billions of years. These interactions have shaped Earth’s history and will determine its future.  (MS-ESS2-2)

NGSS Disciplinary Core Idea (DCI) High School:
ESS1.A:  The Universe and Its Stars

• The star called the sun is changing and will burn out over a lifespan of approximately 10 billion years. (HS-ESS1-1)
• The study of stars’ light spectra and brightness is used to identify compositional elements of stars, their movements, and their distances from Earth. (HS-ESS1-2), (HS-ESS1-3)
• The Big Bang theory is supported by observations of distant galaxies receding from our own, of the measured composition of stars and non-stellar gases, and of the maps of spectra of the primordial radiation (cosmic microwave background) that still fills the universe. (HS-ESS1-2)
• Other than the hydrogen and helium formed at the time of the Big Bang, nuclear fusion within stars produces all atomic nuclei lighter than and including iron, and the process releases electromagnetic energy. Heavier elements are produced when certain massive stars achieve a supernova stage and explode. (HS-ESS1-2), (HS-ESS1-3)


NGSS Cross Cutting Concepts (CCC):

· Scale, Proportion and Quantity
· Systems and System Models
· Cause and Effect
· Patterns

NGSS Science and Engineering Practices (SEP):
· Analyzing and Interpreting Data
· Obtaining, Evaluating and Communicating Information.

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TERMS OF USE

• All rights reserved by Williams Hands On Science, Inc.

• This product is to be used by the original purchaser only.

• Intended for classroom and personal use only.

• Copying for more than one teacher, classroom, department, school, or school system is prohibited.

• This product may not be distributed or displayed digitally for public view.

• Failure to comply is a copyright infringement and a violation of the Digital Millennium Copyright Act (DMCA).

If there are any errors or questions, please contact me through TpT or email me at:

williamshandsonscience@gmail.com

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Total Pages
40 pages
Answer Key
Included
Teaching Duration
90 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.
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).

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