Particle.news
Download on the App Store

JWST Hints at Patchy Water-Ice Clouds on Epsilon Indi Ab

The result points to patchy water-ice clouds missing from most current models.

Overview

  • A Max Planck–led team reported on April 22, 2026 that new JWST data for the nearby gas giant Epsilon Indi Ab show less ammonia than models predict.
  • Using JWST’s MIRI coronagraph, which blocks starlight to reveal faint planets, the team compared images at 10.6 μm and 11.3 μm to estimate ammonia in the atmosphere.
  • The weaker ammonia signal, paired with the planet’s faint mid-infrared output, matches a picture of thick, patchy water-ice clouds high in the atmosphere.
  • Epsilon Indi Ab orbits about four times farther from its star than Jupiter does from the Sun, has roughly 7.6 Jupiter masses with a similar diameter, and holds a temperature near 200–300 K.
  • The study in Astrophysical Journal Letters urges cloud-inclusive models, and the team plans more JWST observations as NASA’s Roman telescope is expected to detect reflective ice clouds directly.