
A New Way to Find Planets in a Telescope’s Shifting Starlight
A physics-based method models JWST’s shifting starlight, improving exoplanet sensitivity and revealing 51 Eridani b at 4.3 micrometers.

A physics-based method models JWST’s shifting starlight, improving exoplanet sensitivity and revealing 51 Eridani b at 4.3 micrometers.

Exoplanet rings may boost a planet’s reflected light enough to reveal it—but also distort estimates of its size, brightness, and atmosphere.

A laboratory interferometer combines two apertures and a scanning spectrometer to test sharper, frequency-resolved far-infrared space imaging.