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Earth and Space Science

ESS1 1 Lifespan of the Sun

Project Zero THINKING ROUTINES--see Phenomenon below

Phenomenon--

Video: Nuclear fusion in the Sun cK-12
What do you know before you see this source?  How does it add to your knowledge?
What do you still need to know?

 

Prior Knowledge/Preview
The Nature of Stars see Chapter 2 AAVSO
Introduction to nuclear science lnl.gov and experiments
Diamonds in the Sky: Stars and Exoplanets SI NASM Stem in 30
 
Inquiry science
       Printable activity
      On-line activity:
--Go to Life Cycles of Stars Practice cK-12
Journey through an Exploding Star-electromagnetic spectrum Smithsonian Learning Lab
    
LAB activities follow all safety guidelines linked above
and in the activity
Lab #1 Investigating H-R graphs see activity 9.2 using Fig 9.3 + tables 9.1 and 9.2 AND Pulsating Star Activity see activity 7.1 and other AAVSO resources
Lab #2 The Power of the Sun Discovery School--see Savage Sun video via YouTube
Lab #3 Nuclear Fusion Activity NASA
Night Sky Network and Teacher info
Lab #4 Supernova Simulation NASA Night Sky Network
Lab #5 Radiation Dose calculation Section 6 NASA

      
EXTENSION material for the curious
Looking at stars: the Messier Marathon -110 astronomical objects NASA
and Which stars go to a supernova? NASA
and Other Supernova Material NASA
Solar Storms and You activities NASA
Solar Wind Meets Cold Space NASA
Solar storms and more page xvi + NASA

 

Compare the Earth and the Sun and see images of the energy being produced

Life and Death of Stars NASA

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 in the form of radiation. HS-ESS1-1
 Clarification Statement and Assessment Boundary
Clarification Statement: 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 Boundary: Assessment does not include details of the atomic and sub-atomic processes involved with the sun’s nuclear fusion.

Aerospace CONNECTIONS:
Applications and examples
Sun probes: Hinode, Solo, Stereo, Parker Solar Probe Washington International School
Lives of Stars (ems) Smithsonian Learning Lab
African Cosmos: Sounds of Stars Smithsonian Institute
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Stamp depicting solar spectrum (all the colors of the rainbow) Philatelic origin CC0

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