The Sun is far more than a glowing orb in the sky; it is a complex, multi-layered powerhouse of energy. Understanding its structure is key to understanding how life on Earth is sustained and how solar weather affects our modern technology.

Beyond the interior lies the solar atmosphere, which transitions from the light we see to the outer reaches of space:
Photosphere: The “surface” we see from Earth. It emits the visible sunlight we rely on and is home to cooler, dark regions known as sunspots.
Chromosphere: A thin, vibrant layer of plasma that glows red during eclipses, acting as a transition zone between the surface and the outer atmosphere.
Corona: The Sun’s crowning glory. This wispy outer halo is millions of degrees hotter than the surface and expands outward to form the solar wind.
