ESS3+p2


 * =ESS3 The origin and evolution of galaxies and the universe demonstrate fundamental principles of physical science across vast distances and time. =

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//Click on the GSE numbers, e.g PS1 (K-2) - POC - 2, in the table below to reach additional information about each GSE. // || Grade Span Expectations (5-8) ||  || Grade Span Expectations (HS) ||   || **Students demonstrate understanding of processes and change over time within the system of the universe (Scale, Distances, Star Formation, Theories, Instrumentation) by…** 9a observing that there are more stars in the sky than can easily be counted, but they are not scattered evenly and not all the same in brightness. || ESS3 (3-4) - 9 **Students demonstrate understanding of processes and change over time within the system of the universe (Scale, Distances, Star Formation, Theories, Instrumentation) by…** 9a __recognizing that throughout history people have identified patterns of stars that we call constellations.__ || ESS3 (5-6) - 9 9a describing the apparent motion/position of the objects in the sky. (e.g. __constellations, planets).__ 9b __identifying the sun as a medium-sized star located near the edge of a disk-shaped galaxy of stars.__ ||  || ESS3 (9-11) - 7 **Students demonstrate an understanding of processes and change over time within the system of the universe (Scale, Distances, Star Formation, Theories, Instrumentation) by...** 7a __applying the properties of waves/particles to explain the movement, location, and composition of the stars and other bodies in the universe__ || ||
 * || Grade Span Expectations (K-4) || 
 * || ESS3 (K-2) - 9
 * Students demonstrate an understanding of the structure of the universe by … **