This is the first module in the Solar Dynamic Observatory (SDO) Project Suite curriculum. Activities are self-directed by students or student teams using online videos and data from the SDO satellite to explore, research and build knowledge about... (View More) features of the Sun. Students build vocabulary, apply or demonstrate learning through real world connections, and creating resources to use in their investigations. Each activity comes with both a teacher and student guide with sequential instructions and embedded links to the needed videos and internet resources. Activity 1A: Structure of the Earth's Star takes students through the features and function of the Sun's structures using online videos, completing a "Sun Primer" data sheet using information from the videos, and creating a 3D origami model of the Sun. Students use a KWL chart to track what they have learned. Activity 1B: Observing the Sun has students capture real solar images from SDO data to find and record sunspots and track their movement across the surface of the Sun. Activity 1C has students create a pin-hole camera to use in calculating the actual diameter of the Sun, and then calculate scales to create a Earth-Sun scale model. Students reflect on their learning and results at the end of the module. An internet connection and access to computers are needed to complete this module. See related and supplementary resources for link to full curriculum. The appendix includes an alignment to the Next Generation Science Standards (NGSS). (View Less)

This is the second module in the Solar Dynamic Observatory (SDO) Project Suite curriculum. Each activity is self-directed by students or student teams and uses online videos, data from the SDO satellite and hands-on activities to explore, research... (View More) and build knowledge about how and why studying the Sun's electromagnetic energy and magnetic fields help scientists better understand the Sun's activity and space weather. Students build knowledge and vocabulary, apply or demonstrate learning through real world connections and create resources to use in investigations. Both a teacher and student guide is included with sequential instructions and embedded links to the needed videos, tutorials and internet resources. In Activity 2A: The Sun and the EM Spectrum students learn how SDO uses key parts of the Sun's electromagnetic spectrum (EMS) to research regions of the Sun, create an interactive foldable to describe the different wavebands of the EMS, then use real-time SDO image data and the Helioviewer online tool to explore the Sun's regional activity. Tutorials for using Helioviewer and making the EMS foldable are included. Activity 2B: Solar activity and Magnetism has students use information in online videos and slide presentations to demonstrate concepts of magnetism and the relationship between the Sun's variable magnetic fields and sunspots. Activity 3B: Solar Research in Action! Build a Spectroscope has students create a spectroscope to observe the different wavebands of visible light, demonstrate how the Sun emits varying EMS energies, and explain how this information helps scientists understand the composition and activity of both our nearest star, and other stars in the universe. A computer for student-teams and a connection to the Internet are needed to complete this module. See related and supplementary resources for link to full curriculum. The appendix includes an alignment to the Next Generation Science Standards (NGSS). (View Less)

This is the third module in the Solar Dynamic Observatory (SDO) Project Suite curriculum. Each activity is self-directed by students or student teams and utilizes online videos, data from the SDO satellite and hands-on activities to explore,... (View More) research and build knowledge about how the Sun's varying activity impacts Earth and space weather. Each activity provides opportunities to build knowledge and vocabulary, apply or demonstrate learning through real world connections and create resources to use in investigations. Both a teacher and student guide are included with sequential instructions and embedded links to the needed videos, tutorials and internet resources. In Activity 3A: Sun-Earth Interactions, students gather information from online videos and create a 3D model to demonstrate the relationship to Earth's place in space and the affect of Earth's axial tilt on our seasons, then film a short video explaining the reasons for the seasons. Activity 3B: Space Weather, students use online videos to gather information on what space weather is, and its causes and effects, to create a concept map. They then use real-time SDO data to forecast space weather. Activity 3C: Solar Research in Action! Make a Magnetometer has students view information in online videos about to Earth's magnetosphere and the impacts of space weather, then create a magnetometer to detect and visualize changes in the Earth's magnetic fields to monitor solar storm impacts. A computer for student-teams and access to the internet are needed for this module. See related and supplementary resources for link to full curriculum. The appendix includes an alignment to the Next Generation Science Standards (NGSS). (View Less)

This is a lesson about the solar wind, Earth's magnetosphere, and the Moon. Participants will work in groups of two or three to build a model of the Sun-Earth-Moon system. They will use the model to demonstrate that the Earth is protected from... (View More) particles streaming out of the Sun, called the solar wind, by a magnetic shield called the magnetosphere, and that the Moon is periodically protected from these particles as it moves in its orbit around the Earth. Participants will also learn that the NASA ARTEMIS mission is a pair of satellites orbiting the Moon that measure the intensity of solar particles streaming from the Sun. (View Less)

In this lesson, learners will construct a 3D scale model of one of the MMS satellites. After, they will calculate the octagonal area of the top and bottom of the satellites, given the measurements of the satellite. Then, learners will compare the... (View More) octagonal cross-section area of the satellites with the circular cross-section area of the launch vehicle to determine if the eight-sided spacecraft will fit the circular rocket hull. This is lesson one of the MMS Mission Educator's Instructional Guide, which uses examples from the MMS Mission to introduce mathematics (focusing on geometry) in a real-world context. The lessons use the 5E instructional cycle. Note: MMS launched March 12, 2015. For the latest science and news, visit the MMS Mission Website under Related & Supplemental Resources (right side of this page). (View Less)

This is an activity about the measurement of time. Learners model the rotation of Earth over one day by holding a flashlight for the Sun and a blow up globe, and record their observations. Then, they use those observations to create devices that... (View More) will track time and test their devices outside. This final part of this activity requires access to a sunny outdoor location for an extended period of time so learners can test their time measurement devices. (View Less)

This is an activity about understanding how the Earth’s axial tilt changes the angle at which sunlight hits the Earth, contributing to the variations in temperature throughout the seasons. Learners will create a sun angle analyzer in order to see... (View More) what happens to the concentration of sunlight when the Sun is at different angles throughout the year. This will help learners realize Earth’s seasonal temperature differences are directly related to sunlight angle due to the Sun’s overall intensity at locations on the Earth. Finally, learners reflect on the results of the Sun-Earth Survey, which is Activity 2 in this set, and their experiences with all of the other activities in the guide. This is Activity 8, the final activity in the Great Explorations in Math and Science (GEMS) guide titled Real Reasons for Seasons: Sun-Earth Connections. The resource guide is available for purchase from the Lawrence Hall of Science. (View Less)

This is an activity about the size and scale of the Sun-Earth system. Learners will take an imaginary trip to the Sun by comparing images of the Sun and Earth at different points in altitude above the Earth. This is to ultimately conceptualize the... (View More) spherical shape of the Earth, which is key to understanding the cause of the seasons. They will then produce a scale model of the Sun and Earth to reinforce the idea that the distance to the Sun is enormous compared with the size of the Earth. Finally, learners reflect on Question 3 of the Sun-Earth Survey, which is the prior activity in this set. This is Activity 3 in the Great Explorations in Math and Science (GEMS) guide titled Real Reasons for Seasons: Sun-Earth Connections. An additional related activity, entitled Scale Models of the Earth-Moon System and the Solar System, is included in the CD-ROM enclosed with the resource guide. The resource guide is available for purchase from the Lawrence Hall of Science. This activity recommends use of an overhead projector, and requires use of a small scale model toy, such as a car or any other toy made to scale, and a rigid globe or large ball like a soccer ball or basketball. (View Less)