home   •  sun   •  light   •  science   •  more   •  about      settings: full/mobile
click to return to our home page
making visual sense of hard ideas

Let's start from something we all know and agree about: Earth's place in the solar system. Starting before history was written down, humans undoubtedly scratched images of the stars and ‘wandering stars’ – the planets – in the sand: the earliest attempts to understand and predict the future, or, the beginning of science.

Our understanding of Earth's place among the planets and stars was, for centuries, based on the obvious fact that we are the center of the universe. Plato's model of heavenly spheres, and the notion of heaven itself, became an article of faith.


Earth (Terra) at the center before 1596

early rendering of Kepler’s heliocentric model

 

Johannes KeplerJohannes Kepler proposed the revolutionary idea that the planets, including Earth, orbit the Sun. With Tycho Brahe's precise data and discovery that planets move in ellipses rather than circles, Kepler mapped the true heliocentric solar system in something approaching our current understanding in 1609

We may also agree that our relationship to our Sun is the Earth's  single most important fact. Sunspot’s whole mission is to help us acquire a clearer and more comprehensive understanding of this fact.

In pursuit of the science, we are not alone: in the last half century, the level and intensity of scientific inquiry about the Sun and light has exploded, and imagery has become the principal way of explaining as well as the primary source of scientific advancement. 

From the summit of Hawaii's Haleakala Observatory, the Inouye Solar Observatory is the main earth-bound site for solar exploration. The best solar viewing is possible from that height because the air is clear and minimally obscured by nearby cities.

Even better, space telescopes have allowed increasingly high resolution and varied spectra unavaliable inside the Earth’s atmosphere.

By 2020, space and imaging technology improved to the point where the European Space Agency was able to place a satellite that approaches the blazing star within a mere 42 million kilometers, where the equipment needed to operate despite the temperature in excess of 500°C.

 

GOES EUV sun images 6 September 2026
Recent extreme ultraviolet (EUV) Sun images by GOES satellites
GOES-R EUV images - 6 September 2026

 

NOAA's Space Weather website explains the importance of forecasting disruptions:

The four spacecraft in the GOES-R series each carry a sophisticated extreme ultraviolet (EUV) telescope called the Solar Ultraviolet Imager (SUVI). This telescope allows forecasters to monitor the Sun’s hot outer atmosphere, or corona. EUV photons are created in the million-degree plasma of the corona and are not visible from the ground, due to the absorption of the Earth’s atmosphere. Observations of solar EUV emission aids in the early detection of solar flares, coronal mass ejections (CMEs), and other phenomena that impact the geospace environment.

 

EUV photons travel at the speed of light and are the first indication we receive at Earth of solar magnetic eruptions and associated flares. These high-energy photons cause changes to the Earth’s ionosphere and can result in significant degradation of radio communications, including complete black outs at some frequencies. The impacts begin only 8 minutes (time for light to travel from the Sun to Earth) after a flare. 

The early warning given when SUVI observes a solar eruption comes at least 15 hours before the associated CME arrives at Earth. This allows forecasters at SWPC to issue the appropriate watches, warnings, and alerts for geomagnetic storms.





 

click to ask Sunspot a question click to send a comment to Sunspot
no nonsense privacy policy
sitemap
Nimda content administration system
written by Michael Potts

file updated 20 August 2026
copyright © 2003-2026 Caspar Institute
this site generated with 100% recycled electrons