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               <rdf:li>Michael A. Doody</rdf:li>
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               <rdf:li xml:lang="x-default">18.01.08: We are Made of Star Stuff: The Cosmic Origins on the Elements of Earth</rdf:li>
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               <rdf:li xml:lang="x-default">Science</rdf:li>
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               <rdf:li>NGSS</rdf:li>
               <rdf:li>stars</rdf:li>
               <rdf:li>cosmic</rdf:li>
               <rdf:li>origins</rdf:li>
               <rdf:li>elements</rdf:li>
               <rdf:li>hydrogen</rdf:li>
               <rdf:li>helium</rdf:li>
               <rdf:li>big bang</rdf:li>
               <rdf:li>nuclear</rdf:li>
               <rdf:li>reaction</rdf:li>
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         <pdf:Keywords>NGSS, stars, cosmic, origins, elements, hydrogen, helium, big bang, nuclear, reaction, chemistry</pdf:Keywords>
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<Document>
<P>Curriculum Unit Title:           Author: </P>

<Textbox><Figure>

<ImageData src="images/18.01.08_img_0.jpg"/>
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<P>We Are Made of Star Stuff </P>
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<Textbox><Figure>

<ImageData src="images/18.01.08_img_1.jpg"/>
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<P>Michael A. Doody </P>
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<P> </P>

<P> </P>

<P>KEY LEARNING, ENDURING UNDERSTANDING, ETC.  </P>

<P> </P>

<Textbox>
<P>NGSS Standard HS-ESS1-3 – communicate ideas about the way stars, over their life cycles, produce elements </P>
<Figure>

<ImageData src="images/18.01.08_img_2.jpg"/>
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<P>NGSS Standard HS-PS1-8: develop a model based on evidence to illustrate the changes in the nucleus and the energy released in nuclear processes </P>
</Textbox>

<P> </P>

<P> </P>

<P> </P>

<P>ESSENTIAL QUESTION(S) for the UNIT </P>

<P> </P>

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<ImageData src="images/18.01.08_img_3.jpg"/>
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<P>How do stars produce elements throughout their life cycle </P>
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<P> </P>

<P> </P>

<P> </P>

<P> </P>

<P>   CONCEPT A     CONCEPT B              CONCEPT C </P>

<P> </P>

<Textbox><Figure>

<ImageData src="images/18.01.08_img_4.jpg"/>
</Figure>

<P> </P>

<P>Star Composition </P>
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<ImageData src="images/18.01.08_img_5.jpg"/>
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<P> </P>

<P>Fission vs Fusion </P>
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<ImageData src="images/18.01.08_img_6.jpg"/>
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<P> </P>

<P>Big Bang Nucleosynthesis and Cosmic Recycling </P>
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<P> </P>

<P> </P>

<P> </P>

<P> </P>

<P>             ESSENTIAL QUESTIONS A   ESSENTIAL QUESTIONS B          ESSENTIAL QUESTIONS C </P>

<P> </P>

<Textbox><Figure>

<ImageData src="images/18.01.08_img_7.jpg"/>
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<P>What are the similarities and differences of fusion and fission? </P>

<P>How do fission and fusion impact the formation of elements? </P>

<P> </P>
</Textbox>

<Textbox><Figure>

<ImageData src="images/18.01.08_img_8.jpg"/>
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<P>How can star composition be determined? </P>
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<ImageData src="images/18.01.08_img_9.jpg"/>
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<P>How are light elements formed? </P>

<P>How are heavy elements formed? </P>

<P>How are elements recycled in the universe? </P>
</Textbox>

<P> </P>

<P> </P>

<P> </P>

<P> </P>

<P> </P>

<P>           VOCABULARY A            VOCABULARY B          VOCABULARY C </P>

<P> </P>

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<ImageData src="images/18.01.08_img_10.jpg"/>
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<P>Spectra </P>

<P>Wavelength </P>

<P> </P>
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<ImageData src="images/18.01.08_img_11.jpg"/>
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<P>Fission  </P>

<P>Fusion </P>

<P>Nucleus </P>

<P> </P>
</Textbox>

<Textbox><Figure>

<ImageData src="images/18.01.08_img_12.jpg"/>
</Figure>

<P>Elementary particles  Supernovae </P>

<P>Nucleosynthesis </P>

<P>Light elements </P>

<P>Heavy elements </P>
</Textbox>

<P> </P>

<P> </P>

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<P> </P>

<P>ADDITIONAL INFORMATION/MATERIAL/TEXT/FILM/RESOURCES </P>

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<P> </P>

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<ImageData src="images/18.01.08_img_13.jpg"/>
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<P>Neil deGrass Tyson. 2017. Astrophysics for People in a Hurry. Carl Sagan. 1980. Cosmos. Hyperphysics: hyperphysics.phy-astr.gsu.edu </P>

<P>Chandra X-Ray Center: Chandra.harvard.edu </P>
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