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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. (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. (View Less)

During the last sunspot cycle between 1996-2008, over 21,000 flares and 13,000 clouds of plasma exploded from the Sun's magnetically active surface. These events create space weather. Students will learn more about space weather and how it affects... (View More) Earth through reading a NASA press release and viewing a NASA eClips video segment. Then students will explore the statistics of various types of space weather storms by determining the mean, median and mode of a sample of storm events. This activity is part of the Space Math multimedia modules that integrate NASA press releases, NASA archival video, and mathematics problems targeted at specific math standards commonly encountered in middle school textbooks. The modules cover specific math topics at multiple levels of difficulty with real-world data and use the 5E instructional sequence. (View Less)

During the last sunspot cycle between 1996-2008, over 21,000 flares and 13,000 clouds of plasma exploded from the Sun's magnetically active surface. Students will learn more about space weather through reading a NASA press release and viewing a NASA... (View More) eClips video segment. Then students will explore the statistics of various types of space weather storms by determining the mean, median and mode of different samples of storm events. This activity is part of the Space Math multimedia modules that integrate NASA press releases, NASA archival video, and mathematics problems targeted at specific math standards commonly encountered in middle school textbooks. The modules cover specific math topics at multiple levels of difficulty with real-world data and use the 5E instructional sequence. (View Less)

Students will learn about the Transit of Venus through reading a NASA press release and viewing a NASA eClips video that describes several ways to observe transits. Then students will study angular measurement by learning about parallax and how... (View More) astronomers use this geometric effect to determine the distance to Venus during a Transit of Venus. This activity is part of the Space Math multimedia modules that integrate NASA press releases, NASA archival video, and mathematics problems targeted at specific math standards commonly encountered in middle school textbooks. The modules cover specific math topics at multiple levels of difficulty with real-world data and use the 5E instructional sequence. (View Less)

This is a booklet containing 31 problem sets that involve a variety of math skills, including scientific notation, simple algebra, and calculus. Each set of problems is contained on one page. Learners will use mathematics to explore varied space... (View More) science topics including black holes, ice on Mercury, a mathematical model of the Sun's interior, sunspots, the heliopause, and coronal mass ejections, among many others. (View Less)

This is a lesson about magnetism and solar flares. Learners will evaluate real solar data and images in order to calculate the energy and magnetic strength of a solar flare moving away from the Sun as a coronal mass ejection. This is Activity 3 in... (View More) the Exploring Magnetism in Solar Flares teachers guide. (View Less)