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         <pdf:Keywords>Science, universe, NASA, Rover, Mariner, Astronomy, Optics, Electromagnetic spectrum, telescope, luminosity, spectroscopy</pdf:Keywords>
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               <rdf:li xml:lang="x-default">18.01.01: The Universe We See</rdf:li>
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               <rdf:li xml:lang="x-default">Science</rdf:li>
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               <rdf:li>Lars Andrew Jensen</rdf:li>
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               <rdf:li>Science</rdf:li>
               <rdf:li>universe</rdf:li>
               <rdf:li>NASA</rdf:li>
               <rdf:li>Rover</rdf:li>
               <rdf:li>Mariner</rdf:li>
               <rdf:li>Astronomy</rdf:li>
               <rdf:li>Optics</rdf:li>
               <rdf:li>Electromagnetic spectrum</rdf:li>
               <rdf:li>telescope</rdf:li>
               <rdf:li>luminosity</rdf:li>
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The Universe We See                 Lars Jensen                       Students will apply their understanding of waves to learning about light as it is important in astronomy. Students will be able to describe the main properties of light, how     light changes as it moves through the universe, and how light interacts with matter. Students will asl understand the diﬀerent regions of the electromagnetic spectrum and their sources in astronomy. Students will also be able to develop a model for explaining evidence of the Big Bang from their understanding of light. What changes about light as it travels through space away from a star the emitted the light?What would the night sky look like if our eyes could see diﬀerent regions of the electromagnetic spectrum, not just visible light?How can we use spectra observations to determine the chemical composition of diﬀerent planetary atmospheres? Intensity of Light     The Sky Through Diﬀerent Eyes Spectral Lines of Diﬀerent Atmospheres Text: OpenStax Astronomy                                                                     a                                                                                                   a                                                                                                  a                                                                                                                                                       What changes about light as it travels   through space away from a star the       emitted the light?                                                     a                   What would the night sky look like if our eyes    could see diﬀerent regions of the electromagnetic spectrum, not just visible light?                        How can we use spectra      observations to determine the    chemical composition of diﬀerent planetary atmospheres?                  a                                         Speed of light, Wavelength, Frequency,         Intensity, Brightness, Luminosity, Inverse Square Law Radio waves, Microwaves, Infrared,               Visible, Ultraviolet, X-Ray, Gamma Ray Spectra, apparent color, emission      spectrum, </Figure>
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