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NASA Heliophysics Education

The NASA Heliophysics Education Activation Team's (NASA HEAT) Framework for Heliophysics Education outlines key concepts, practices, and strategies for integrating solar science into educational curricula and learning activities. It provides educators, scientists, and outreach professionals with a cohesive set of Heliophysics Big Ideas that align with the three questions that drive NASA's heliophysics research. 

What is heliophysics?

Heliophysics is the study of our star, the Sun [helio], and how its behavior [physics] affects Earth, the solar system, and the very nature of space.

The Science Mission Directorate Heliophysics Division studies the nature of the Sun, and how it influences the very nature of space – and, in turn, the atmospheres of planets and the technology that exists there. Space is not, as is often believed, completely empty; instead, we live in the extended atmosphere of an active star. Our Sun sends out a steady outpouring of particles and energy – the solar wind – as well as a constantly writhing magnetic system. This extensive, dynamic solar atmosphere surrounds the Sun, Earth, the planets, and extends far out into the solar system.