Daily Learning Experience Β· Science

Trapped in the Sun

You were just born in the hottest place for 93 million miles. Now you have to get out β€” and it's going to take you longer than the entire history of human civilization.

β–Ύ scroll to begin your escape
0:00 β€” Your birthday

You are a photon.

Picture this. You blink into existence in the core of the Sun, where it is 15 million degrees and the pressure is 250 billion times what you feel at the beach.

A heartbeat ago, four hydrogen nuclei were slammed together so hard they fused into a single helium nucleus. The tiny scrap of mass left over became pure energy β€” became you, a gamma-ray photon, the most energetic kind of light there is.

Above you sit 432,000 miles of blazing plasma. The surface β€” freedom β€” is up there somewhere. You are the fastest thing in the universe. This should be easy.

It will not be easy.

Four hydrogen nuclei fuse into helium β€” and release a flash of light. That's you.

The problem β€” a drunkard's walk

Every millimetre, you crash.

The Sun's interior is so dense that you travel only a few millimetres before smacking into a particle. It swallows you, then spits out a new photon in a random direction. Over and over. You don't cross the Sun β€” you stagger through it blind. Take control below and try to reach the surface.

0
collisions
0%
of the way out
0
years elapsed

This is a sped-up model. A real photon takes so many steps (roughly a trillion trillion) that no computer could animate them β€” here each bounce stands in for a colossal number of real ones. Lower the density and watch the escape get faster: that's exactly why light leaks out of a star's thin outer layers so much quicker than its crushed core.

Roughly 100,000 years later…

You catch a ride.

Somewhere past two-thirds of the way out, the plasma stops just glowing and starts boiling. Enormous columns of hot gas rise like water in a pot, each cell as wide as Texas. You stop crawling and hitch a ride upward on a rising bubble β€” the convection zone β€” covering in a few days a distance that random-bouncing took ages.

The Sun's surface, seen from space, is stitched from millions of these boiling cells. We call the pattern granulation. Watch one breathe:

The finish line

Eight minutes to Earth.

You burst out of the surface β€” no longer a violent gamma ray, but soft, visible, golden light, your energy long since shared out and cooled. After tens of thousands of years trapped inside, the sprint across empty space to Earth takes just eight minutes and twenty seconds. Hit the button and run it.

The sunlight warming your face right now finished a journey that began before the pyramids β€” before farming, before writing. Its trip inside the Sun took longer than all of recorded history. Its trip to you took less time than brushing your teeth.

Mind = blown

Five things to carry out with you

15,000,000Β°
The temperature of the core (in Β°C) where you were born. Hot enough to strip every atom bare.
~1 cm
How far you typically travel between collisions in the dense interior. A few millimetres to a few centimetres.
10,000–170,000 yr
Scientists' estimate of how long the bouncing escape actually takes. "About 100,000 years" is the popular shorthand.
8 min 20 s
The dash from the Sun's surface to Earth once you're finally free. 93 million miles at light speed.
Not "you"
You're absorbed and re-emitted countless times, so the light that reaches Earth isn't the same photon that left the core β€” only its energy survives the trip.
Quiz score: 0 / 6 β€” answer below ⬇
Prove you escaped

The photon's exit exam

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