Science Activation

Helio Highlights: October 2025

Explore This Section

ScienceScience ActivationHelio Highlights: October…HomeFramework for Heliophysics Education
AboutHelio Big Idea 1.1Helio Big Idea 1.2Helio Big Idea 1.3Helio Big Idea 2.1Helio Big Idea 2.2Helio Big Idea 2.3Helio Big Idea 3.1Helio Big Idea 3.2Helio Big Idea 3.3Helio MissionsHelio TopicsResource DatabaseAbout NASA HEATMore
HighlightsSpace Math5 min read

Helio Highlights: October 2025

5 Min Read

Helio Highlights: October 2025

NASA Education Specialist Christine Milotte demonstrates heliophysics activities during a teacher professional development event hosted by the NASA Heliophysics Education Activation Team (HEAT) at the Dallas Arboretum, Saturday, April 6, 2024.

Credits:
NASA/Keegan Barber

The Sun and Our LivesOn a clear night, you might see thousands of stars in the sky. Most of these stars are dozens or hundreds of light years away from us. A light year is the distance a beam of light travels in a year: about 5.88 trillion miles (9.46 trillion kilometers). This means that for those stars we see at night, it takes their light, which travels at about 186,000 miles per second (or about 300 thousand kilometers per second), dozens or hundreds of years to reach us.
But in the daytime, we only see one star: the Sun. It dominates the daytime sky because it is so close – about 93 million miles (or 150 million kilometers) away. That distance is also called one astronomical unit, and its another unit of measurement astronomers use to record distance in space. But even if 1 astronomical unit seems like a long way, it’s still about 270 thousand times closer than Alpha Centauri, the next nearest star system.
The Sun isn’t just close – it’s also gigantic! The Sun is large enough to fit more than a million Earths inside it, and has more mass than 330 thousand Earths put together. Its light also provides the energy which allows life as we know it to flourish. For these reasons, the Sun is a powerful presence in our lives. We all have a relationship with the Sun, so knowing about it, and about the benefits and hazards of its presence, is essential.
Teaching About the SunAutumn is when most students in the United States return for a new school year after summer vacation. This back-to-school time offers a wonderful opportunity to reach students fresh off of a few months of fun in the Sun and capture their imaginations with new information about how our native star works and how it impacts their lives.
To that end, NASA conducts efforts to educate and inform students and educators about the Sun, its features, and the ways it impacts our lives. NASA’s Heliophysics Education Activation Team (HEAT) teaches people of all ages about the Sun, covering everything from how to safely view an eclipse to how to mitigate the effects of geomagnetic storms.
This “Our Dynamic Sun” banner is one of many educational outreach products offered by NASA HEAT. It uses imagery of the Sun at..

Read more