Stars & GalaxiesATLAS / DEEP UNIVERSE

DEEP UNIVERSE

Light arrives
with a history.

Light from distant galaxies takes time to reach us, so we observe them as they were when that light was emitted.

Original LUME editorial visualisation of distant galaxies and lensed light
EDITORIAL VISUALISATION Original LUME GRAVITY artwork — an imagined deep field, not telescope data.
01 / REDSHIFT

Stretching light

As space expands, light from distant galaxies is shifted toward longer wavelengths. This measured shift helps relate a signal to cosmic time.

NASA · cosmological redshift
02 / LENSING

Gravity as a lens

Mass bends light. A foreground galaxy or cluster can magnify and distort the view behind it, making otherwise inaccessible sources measurable.

NASA · gravitational lenses
03 / INFERENCE

Estimating distances and masses

Distances, masses and early structures are constrained by multiple observations, models and comparison—not by a single beautiful image.

NASA · measuring galaxy distances

THE DISTANT LIGHT

How we observe distant galaxies.

Read NASA’s galaxies overview