The sunlight warming your skin today took just eight minutes to travel 93 million miles. But those exact photons spent tens of thousands of years trapped inside the Sun's core.
Born of nuclear fusion, a photon must constantly collide with densely packed atoms in the radiative zone, bouncing in a "random walk" that can last up to 100,000 years before finally reaching the surface and launching into space.
If an atmosphere existed between Earth and the Sun, the acoustic waves generated by the Sun's convective layer would reach Earth as a constant, crushing roar. Heliophysicists calculate that this roar would register on the ground at roughly 100 to 125 decibels—about the volume of a chainsaw or a rock concert, despite the Sun being nearly a hundred million miles away.
The Sun also sheds mass at an astronomical rate. Every second, it converts 600 million tons of hydrogen into helium. In this process, about 4 million tons of matter is converted directly into energy, while another 1.5 million tons is blown away as solar wind. Despite losing 5.5 million tons of mass every second, the Sun is so vast that it has lost only about 0.05% of its total mass over its entire 4.6 billion-year lifespan.
To visualize this scale, consider a coronal mass ejection (CME)—an eruption of magnetized plasma that bursts from the solar atmosphere.
As shown in the image, a single solar prominence dwarfs the entire planet, rendering Earth a tiny speck next to a towering loop of plasma. The Sun accounts for 99.86% of all mass in the solar system, meaning everything else—every planet, asteroid, moon, and living organism—is made from the leftover dust of its creation.