Stars & GalaxiesATLAS / STARS & GALAXIES

WORLDS AROUND OTHER STARS

Exoplanets.
Signals become worlds.

We rarely see these planets directly. We find them in the small, repeatable changes they cause in a star’s light and motion.

Original LUME artistic visualisation of a planet passing in front of a distant star
EDITORIAL VISUALISATION Original LUME GRAVITY artwork — an imagined transit scene, not telescope data.

SCHEMATIC SIGNAL

A repeatable dimming.

Light received from the star
baselinetransit
Illustration of a transit light curve. Depth and timing must be measured from data; this graphic is not an observation.
01 · TRANSIT

A star dims.

A planet crossing its star blocks a fraction of the light. Repeated dips can reveal its size and orbit.

NASA · transit method
02 · RADIAL VELOCITY

A star moves.

The gravity of an orbiting planet makes its star shift towards and away from us. Spectra record that motion.

NASA · radial velocity
03 · DIRECT IMAGING

A world separates.

Advanced instruments can suppress starlight and isolate the much fainter glow of a planet.

NASA · direct imaging

WHAT WE KNOW / WHAT REMAINS OPEN

What can we learn after detecting a planet?

Atmospheres, clouds and climates require further observations. Every method reveals a different part of the same system.

Read the NASA overview