<?xml version="1.0" encoding="UTF-8" ?>
<!-- Created from PDF via Acrobat SaveAsXML -->
<!-- Mapping Table version: 28-February-2003 -->
<TaggedPDF-doc>
<?xpacket begin='﻿' id='W5M0MpCehiHzreSzNTczkc9d'?>
<?xpacket begin="﻿" id="W5M0MpCehiHzreSzNTczkc9d"?>
<x:xmpmeta xmlns:x="adobe:ns:meta/" x:xmptk="Adobe XMP Core 5.6-c015 84.159810, 2016/09/10-02:41:30        ">
   <rdf:RDF xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#">
      <rdf:Description rdf:about=""
            xmlns:xmp="http://ns.adobe.com/xap/1.0/"
            xmlns:pdf="http://ns.adobe.com/pdf/1.3/"
            xmlns:dc="http://purl.org/dc/elements/1.1/">
         <xmp:CreateDate>2018-01-27T19:36:01Z</xmp:CreateDate>
         <xmp:CreatorTool>Word</xmp:CreatorTool>
         <xmp:ModifyDate>2018-01-27T19:36:01Z</xmp:ModifyDate>
         <pdf:Producer>Mac OS X 10.10.5 Quartz PDFContext</pdf:Producer>
         <pdf:Keywords>E=MC2, Solar, Anatomy, electromagnetic, radiation, astronomy, integrated&#xD;&#xA;</pdf:Keywords>
         <dc:format>xml</dc:format>
         <dc:title>
            <rdf:Alt>
               <rdf:li xml:lang="x-default">17.05.01: The Sun and its Energy</rdf:li>
            </rdf:Alt>
         </dc:title>
         <dc:creator>
            <rdf:Bag>
               <rdf:li>Monica Cohen</rdf:li>
            </rdf:Bag>
         </dc:creator>
         <dc:description>
            <rdf:Alt>
               <rdf:li xml:lang="x-default">Science&#xD;&#xA;</rdf:li>
            </rdf:Alt>
         </dc:description>
         <dc:subject>
            <rdf:Bag>
               <rdf:li>E=MC2</rdf:li>
               <rdf:li>Solar</rdf:li>
               <rdf:li>Anatomy</rdf:li>
               <rdf:li>electromagnetic</rdf:li>
               <rdf:li>radiation</rdf:li>
               <rdf:li>astronomy</rdf:li>
               <rdf:li>integrated</rdf:li>
            </rdf:Bag>
         </dc:subject>
      </rdf:Description>
   </rdf:RDF>
</x:xmpmeta>
                                                                                                    
                                                                                                    
                                                                                                    
                                                                                                    
                                                                                                    
                                                                                                    
                                                                                                    
                                                                                                    
                                                                                                    
                                                                                                    
                                                                                                    
                                                                                                    
                                                                                                    
                                                                                                    
                                                                                                    
                                                                                                    
                                                                                                    
                                                                                                    
                                                                                                    
                                                                                                    
                           
<?xpacket end="w"?>
<?xpacket end='r'?>

<P>Curriculum	  Unit	  	  	  	  	  	  	  	  	  	  	  	  </P>

<P>The	  Sun	  and	  Its	  Energy	  </P>

<Part>
<H4>Title Author </H4>

<Sect>
<H5>	  	  	  	  	  	  	  	  	  	  	  	  	  	  	  	  	  	  	  	  	  	  	  	  	  	  	  	  	  	  	  	  KEY	  LEARNING,	  ENDURING	  UNDERSTANDING,	  ETC.	  </H5>

<P>	  	  	  	  	  	  </P>

<P>Monica	  Cohen	  </P>

<P>	  </P>

<P>Students	  model	  and	  analyze	  energy	  generation	  and	  transformation	  in	  the	  Sun.	  Students	  communicate	  their	  understanding	  in	  written	  expression	  and	  as	  a	  creative	  model.	  </P>

<P>	  	  	  </P>

<P>	  </P>
</Sect>

<Sect>
<H5>ESSENTIAL	  QUESTION(S)	  for	  the	  UNIT	  </H5>

<P>	  </P>

<P>How	  is	  energy	  generated	  in	  stars	  and	  how	  is	  it	  able	  to	  impact	  Earth?	  </P>

<P>	  	  	  	  </P>

<Table>
<TR>
<TH>	  	  	  	  	  	  	  	  	  	  	  	  	  </TH>

<TH>	  </TH>

<TH>CONCEPT	  A	  </TH>

<TH>	  </TH>

<TH>	  </TH>

<TH>	  	  	  	  </TH>

<TH>	  </TH>

<TH>	  </TH>

<TH>CONCEPT	  B	  </TH>

<TH>	  </TH>

<TH>	  </TH>

<TH>	  	  	  	  	  	  	  	  	  </TH>

<TH>	  </TH>

<TH>	  	  	  	  	  	  	  	  CONCEPT	  C	  </TH>
</TR>

<TR>
<TH>	  	  </TH>

<TD>	  	  	  Solar	  Anatomy	  and	  Fusion	  </TD>

<TD>	  </TD>

<TD>	  </TD>

<TD/>

<TD>Mass	  vs.	  Star	  life	  </TD>

<TD>Electromagnetic	  Radiation	  from	  Sun	  to	  Earth	  </TD>
</TR>

<TR>
<TH>	  </TH>

<TD>	  	  	  ESSENTIAL	  QUESTIONS	  A	  </TD>

<TD>	  	  	  	  	  	  	  	  	  </TD>

<TD>	  </TD>

<TD>	  </TD>

<TD>	  	  	  ESSENTIAL	  QUESTIONS	  B	  </TD>

<TD>	  </TD>

<TD>	  </TD>

<TD>	  </TD>

<TD>ESSENTIAL	  QUESTIONS	  C	  </TD>
</TR>

<TR>
<TH>	  </TH>

<TD/>

<TD/>
</TR>

<TR>
<TH>	  How	  does	  energy	  get	  from	  the	  core	  of	  the	  sun	  to	  </TH>

<TD/>

<TD>How	  does	  the	  change	  in	  mass	  of	  a	  star	  effect	  the	  length	  </TD>

<TD>What	  happens	  when	  the	  energy	  reaches	  earth?	  </TD>
</TR>

<TR>
<TH>	  	  	  	  the	  earth?	  	  </TH>

<TD>	  </TD>

<TD/>

<TD>of	  a	  star’s	  life?	  </TD>

<TD>And	  how	  do	  we	  know	  that	  energy	  has	  reached	  the	  Earth?	  	  </TD>
</TR>

<TR>
<TH>	  </TH>

<TD/>

<TD/>
</TR>

<TR>
<TH>	  </TH>

<TD>	  	  	  	  	  	  	  	  	  	  	  VOCABULARY	  A	  	  </TD>

<TD>	  </TD>

<TD>	  </TD>

<TD>	  </TD>

<TD>	  </TD>

<TD>	  	  	  	  	  	  	  	  	  	  	  VOCABULARY	  A	  	  </TD>

<TD>	  </TD>

<TD>	  </TD>

<TD>	  </TD>

<TD>	  	  	  	  	  	  	  	  	  	  	  	  	  	  	  	  	  	  	  VOCABULARY	  A	  	  </TD>
</TR>
</Table>
<Figure>

<ImageData src="images/17.05.01_img_0.jpg"/>
	  	  	  	  	  Core	  	  Fusion	  	  	  Radiation	  zone	  Reflection	  Chromosphere	  Convection	  zone	  Absorption	  Corona	  	  	  	  	  </Figure>

<P>Electromagnetic	  Radiation	  	  Microwaves	  Gamma	  rays	  Infrared	  Ultraviolet	  Radio	  waves	  X-‐rays	  	  Solar	  wind	  Visible	  light	  Aurora	  </P>

<P>ADDITIONAL	  INFORMATION/MATERIAL/TEXT/FILM/RESOURCES	  	  </P>

<P>	  	  	  	  	  	  </P>
</Sect>
</Part>
</TaggedPDF-doc>
