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NASA Heliophysics

Overview

The Science Mission Directorate Heliophysics Division studies the nature of the Sun and how it influences the very nature of space and the planets and the technology that exists there. Space is not completely empty: We live in the extended atmosphere of an active star. Our Sun sends out a steady outpouring of particles and energy known as the solar wind, carrying the Sun’s writhing magnetic field. This extensive, dynamic solar atmosphere surrounds the Sun, Earth, the planets, and extends far out into the solar system.

Studying this system not only helps us understand fundamental information about how the universe works, but also helps protect our technology and astronauts in space from the effects of space weather. Space weather events can interfere with our communications, satellites and power grids. The study of the Sun and space also reveals how stars contribute to the habitability of planets throughout the universe.

Mapping out this interconnected system requires a holistic study of the Sun’s influence on space, Earth, and other planets.  NASA has a fleet of spacecraft strategically placed throughout our heliosphere—from Parker Solar Probe at the Sun observing the very start of the solar wind, to satellites around Earth, to the farthest human-made object, Voyager, which is sending back observations on interstellar space. Each mission is positioned at a critical, well-thought out vantage point to observe and understand the flow of energy and particles throughout the solar system—all helping us untangle the effects of the star we live with.  

Chart showing the spacecraft in orbit that support the Heliophysics Division. The Sun is on the left and missions throughout the solar system are on the right.
Chart showing the spacecraft in orbit that support the Heliophysics Division. Updated January 24, 2024
NASA

The Sun

The sun is a dynamic star, made of super-hot ionized gas called plasma.

The sun’s surface and atmosphere change continually, driven by the magnetic forces generated by this constantly-moving plasma. The sun releases energy in two ways: the usual flow of light that illuminates the Earth and makes life possible; but also in more violent and dramatic ways–it gives off bursts of light, particles, and magnetic fields that can have ripple effects all the way out to the solar system’s magnetic edge.

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Solar activity follows a roughly 11-year cycle. This composite image shows the sun in extreme ultraviolet wavelengths about once a year over the course of a complete solar cycle.
ESA / NASA / SOHO
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