This is a photograph of the universe at 380,000 years old.

Planck 2018 all-sky map of the cosmic microwave background: an oval sky with mottled blue and orange temperature fluctuations
photon mean free path: too shortuniverse opaque
−300 μK+300 μK

ESA / Planck Collaboration / 2018 legacy releasegalactic coordinates, Mollweidelight received here: now

lmove over the sky b· T2.72548 K ΔT·

The temperature of the oldest light, today.

2.7255 K

About 0.0001 K warmer or cooler, depending where you look.

That tiny difference became everything you can see.

Minus 270 degrees. Planck's detectors were cooled to a tenth of a kelvin so that their own warmth would not drown it.

We exaggerate the differences so you can see them. Those differences were enough.

Try to look earlier.

Before about 380,000 years, the universe was a plasma. Free electrons scattered every photon within a short distance, so light could not travel. When atoms formed, it could. This map is that moment.

Drag toward the beginning.

now380,000 yrthe beginning

You cannot look farther with light.

It is behind everything you see.

The light comes from every direction at once. Whatever you are facing, it is there, past the last star.

How the picture came into focus.

COBE DMR four-year map: coarse blotches
COBE · 1992 · 7°
WMAP nine-year map: finer structure
WMAP · 2012 · 0.2°
Planck 2018 map: fine-grained fluctuations
Planck · 2018 · 5′

Tap one to see it above.

COBE: NASA / COBE Science TeamWMAP: NASA / WMAP Science TeamPlanck: ESA / Planck Collaboration

−300 μK+300 μK

ESA / Planck Collaborationl 0° at centre · b +90° at topT₀ = 2.7255 K

You are looking at the oldest light you can see.

It left when the universe was about 380,000 years old.

It arrived while you were here.

Look up.