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Seasons Winter Solstice NGSS ESS1.B Claim Evidence Reasoning CER

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Williams Hands On Science
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Grade Levels
5th - 9th, Homeschool
Standards
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Pages
7 pages
$3.99
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Williams Hands On Science
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Description

Students learn how the science of Winter Solstice, the day of the year, how the length of days change, how it affects temperatures and how the angle of the sun changes through a C.E.R. (Claim Evidence Reasoning) graphic organizer. This is great for getting your students to explain phenomena in a meaningful way and it allows you as the instructor to adequately assess their understanding of concepts. The students figure out what the "Claim" is in the article, they then use data that supports the claim in the "Evidence" section, draw visual evidence and then explain why the evidence supports the claim in the "Reasoning" section. 

The article has the following concepts:

Winter Solstice

Summer Solstice

Northern & Southern Hemisphere

The Sun’s Position in the Sky

Angle of the Sun’s Rays

Tilt of Axis

Poles

Equator

Latitude

Tropic of Capricorn

Length of Day

Take a look at my CER Mega bundle!

This is great for a current event, sub plan, homework, critical thinking, scaffolding and/or reinforcement of concepts!

You get a CER graphic organizer, an editable key, the article, tips for CER and the link to the website in the article.

NGSS Standards:

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)

This model of the solar system can explain eclipses of the sun and the moon. Earth’s spin axis is fixed in direction over the short-term but tilted relative to its orbit around the sun. The seasons are a result of that tilt and are caused by the differential intensity of sunlight on different areas of Earth across the year.

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)

This model of the solar system can explain eclipses of the sun and the moon. Earth’s spin axis is fixed in direction over the short-term but tilted relative to its orbit around the sun. The seasons are a result of that tilt and are caused by the differential intensity of sunlight on different areas of Earth across the year.

SEP's

Asking Questions and Defining Problem:

Students at any grade level should be able to ask questions of each other about the texts they read, the features of the phenomena they observe, and the conclusions they draw from their models or scientific investigations. 

Engaging in Argument from Evidence:

In 9–12 builds on K–8 experiences and progresses to using appropriate and sufficient evidence and scientific reasoning to defend and critique claims and explanations about the natural and designed world(s). Arguments may also come from current scientific or historical episodes in science.

Construct an explanation based on valid and reliable evidence obtained from a variety of sources (including students' own investigations, models, theories, simulations, peer review) and the assumption that theories and laws that describe the natural world operate today as they did in the past and will continue to do so in the future. (HS-ESS1-2)

CCC's

CCC1: Patterns

Observed patterns of forms and events guide organization and classification, and they prompt questions about relationships and the factors that influence them.

Systems and System Models

Models (e.g., physical, mathematical, computer models) can be used to simulate systems and interactions—including energy, matter, and information flows—within and between systems at different scales. (HS-LS2-5)

Energy and Matter

Changes of energy and matter in a system can be described in terms of energy and matter flows into, out of, and within that system. (HS-LS1-5), (HS-LS1-6)

Energy cannot be created or destroyed—it only moves between one place and another place, between objects and/or fields, or between systems. (HS-LS1-7), (HS-LS2-4)

Energy drives the cycling of matter within and between systems. (HS-LS2-3)

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
7 pages
Answer Key
N/A
Teaching Duration
30 minutes
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Standards

to see state-specific standards (only available in the US).
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.
NGSS5-ESS1-2
Represent data in graphical displays to reveal patterns of daily changes in length and direction of shadows, day and night, and the seasonal appearance of some stars in the night sky. Examples of patterns could include the position and motion of Earth with respect to the sun and selected stars that are visible only in particular months. Assessment does not include causes of seasons.
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.

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