TPT
Total:
$0.00

Northern Lights Activity Electromagnetic Forces Auroras Solar Storms Sunspots

Rated 4.8 out of 5, based on 5 reviews
4.8 (5 ratings)
;
Williams Hands On Science
1.5k Followers
Grade Levels
6th - 12th, Homeschool
Standards
Formats Included
  • Google Slides™
Pages
16 pages
$3.50
$3.50
Share this resource
Report this resource to TPT
Williams Hands On Science
1.5k Followers
Made for Google Drive™
This resource can be used by students on Google Drive or Google Classroom. To access this resource, you’ll need to allow TPT to add it to your Google Drive. See our FAQ and Privacy Policy for more information.

What educators are saying

This was used as sub plans while I was out. The students were engaged, loved the lesson, and this was by far the best sub day I have had in a long time. Easy for the him to follow and the students maintained engagement and showed positive behaviors.
I really liked this resource. I used it for the magnetic fields unit but I think its better suited for sun/ Space unit. I loved the opportunity for writing and graphing.
Also included in
  1. Looking for a complete, standalone year-long curriculum for integrated NGSS Physics, Energy, Waves, Astronomy, Earth’s History, Science and Engineering Practices, Crosscutting Concepts, and Evolution? Look no further than this student-centered, inquiry-based, hands-on bundle! Designed to align with
    Price $205.00Original Price $366.00Save $161.00
  2. This 2-3 week, hands-on, engaging and easy to deliver unit is so fun to teach! Save time and money and let me plan your electricity and magnetism unit for you! If you are teaching the NGSS disciplinary core idea PS2.B: Types of Interactions (electricity and magnetism), this resource is perfect for y
    Price $17.00Original Price $25.00Save $8.00

Description

This engaging, Google Ready, NO PREP resource will wow your students! This resource is great as an introduction, a scaffold, review or sub plan. If you are teaching the NGSS standard PS2.B: Types of Interactions: Electric and magnetic (electromagnetic) forces, this resource is perfect for you!

What Students Do:

  • First I show an amazing video about the Northern Lights as the engage to get the student’s attention. Students are asked, “What causes the Northern Lights, also known as the Aurora Borealis?” without any prior knowledge for metacognitive purposes.

  • Students then make an interactive graph of Sunspot Number Every 2 years from 2004-2020.

  • Students then compare the graph of sunspot numbers to the number of geomagnetic storms that cause the Northern Lights/Aurora Borealis.

  • Students then watch a video called, “What Is An Aurora?” and Revise their background knowledge: What causes the northern lights, also known as the Aurora Borealis? Use Sunspots, Solar Storms and Electrically Charged Particles in your answer.

Students will then wrap up the lesson with answering the following 4 questions:

1. Cause and Effect: What is the relationship between the two data sets?

2. Patterns: How can you explain this pattern?

3. Patterns: Based on the data, what will happen in the future?

4. When solar storms make it through earth’s protective magnetic shield, what are two things that we can experience on earth?

This assignment took 45 minutes for my 8th graders.

You get the following:

-4 Google Slides Student Copy

-12 Google Slides Slideshow for classroom management, pacing and the key.

-Link to the latest sunspot data.

The following concepts are included:

Magnetic field or Magnetosphere

Magnetic Poles

Earth as a large magnet

Sun Spots

Solar Flares

Solar Wind

Magnetically Charged Particles

North and South Poles

Aurora or Northern Lights

Click here and save over 40% by buying my Electricity Magnetism

Bundle that has all my forces, energy, astronomy, waves and evolution resources.

NGSS Standards:

PS2.B: Types of Interactions

Electric and magnetic (electromagnetic) forces can be attractive or repulsive, and their sizes depend on the magnitudes of the charges, currents, or magnetic strengths involved and on the distances between the interacting objects. (MS-PS2-3)

Forces that act at a distance (electric, magnetic, and gravitational) can be explained by fields that extend through space and can be mapped by their effect on a test object (a charged object, or a ball, respectively). (MS-PS2-5)

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

Analyzing and Interpreting Data, Scientific investigations produce data that must be analyzed in order to derive meaning. Because data patterns and trends are not always obvious, scientists use a range of tools—including tabulation, graphical interpretation, visualization, and statistical analysis—to identify the significant features and patterns in the data. Scientists identify sources of error in the investigations and calculate the degree of certainty in the results. Modern technology makes the collection of large data sets much easier, providing secondary sources for analysis.

Asking questions and defining problems in grades 6–8 builds from grades K–5 experiences and progresses to specifying relationships between variables, and clarifying arguments and models.

Ask questions that can be investigated within the scope of the classroom, outdoor environment, and museums and other public facilities with available resources and, when appropriate, frame a hypothesis based on observations and scientific principles. (MS-PS2-3)

CCC1: Patterns

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

Cause and Effect

Empirical evidence is required to differentiate between cause and correlation and make claims about specific causes and effects. (HS-LS3-1), (HS-LS3-2)

Stability and Change

Much of science deals with constructing explanations of how things change and how they remain stable. (HS-ESS2-7)

Feedback (negative or positive) can stabilize or destabilize a system. (HS-ESS2-2)

Thank you for taking a look!

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

Thank you for taking a look!

Please follow me on TpT for new products and check me out on Instagram for my products in action!

https://www.instagram.com/williams_hands_on_science/

Total Pages
16 pages
Answer Key
Included
Teaching Duration
45 minutes
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.

Standards

to see state-specific standards (only available in the US).
NGSSMS-PS2-3
Ask questions about data to determine the factors that affect the strength of electric and magnetic forces. Examples of devices that use electric and magnetic forces could include electromagnets, electric motors, or generators. Examples of data could include the effect of the number of turns of wire on the strength of an electromagnet, or the effect of increasing the number or strength of magnets on the speed of an electric motor. Assessment about questions that require quantitative answers is limited to proportional reasoning and algebraic thinking.
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.
NGSSMS-ESS1-1
Develop and use a model of the Earth-sun-moon system to describe the cyclic patterns of lunar phases, eclipses of the sun and moon, and seasons. Examples of models can be physical, graphical, or conceptual.

Reviews

Questions & Answers