WASP-94Ab is a hot-jupiter gas giant located ~690 light-years from Earth in the constellation Microscopium. It became the first exoplanet on which a repeating daily weather cycle was confirmed, reported by sagnick-mukherjee and david-sing in Science (May 21, 2026) using jwst’s NIRISS instrument and limb-resolved transmission-spectroscopy (src-jwst-wasp-94ab-weather-cycle-2026-05).

Properties

ParameterValue
Distance~690 light-years
Radius1.72 R_Jup
Mass~0.45 M_Jup
Orbital period3.95 days
Orbital distance~5.1 million miles (closer than Mercury to the Sun)
Surface temperature>2,200 °F (1,200 °C)
RotationTidally locked (permanent day/night sides)

Daily weather cycle

  • The permanent morning (leading) limb is blanketed in thick magnesium-silicate clouds (vaporized rock), detected at 9σ.
  • The evening (trailing) limb is clear, showing water-vapor absorption at 10σ.
  • The evening limb runs ~450 K hotter than the morning limb.
  • Proposed mechanism: clouds condense on the cool nightside, ride equatorial super-rotation winds to the morning terminator, then sink or evaporate as they cross into the dayside.

Why it matters

Separating the two limbs corrected a decade of cloud-contaminated, full-disc data. WASP-94Ab’s inferred oxygen and carbon abundance dropped from “hundreds of times” Jupiter’s to only ~5× Jupiter’s — a value consistent with standard gas-giant formation. The blended-limb vs limb-resolved estimates differ at >4σ. The same cloud-cycle pattern was later found on WASP-39b and WASP-17b, suggesting pre-JWST hot-Jupiter composition estimates may be systematically biased. See exoplanet-atmosphere-models and the biosignatures caveat on limb-asymmetry averaging bias.

A sibling jwst limb-resolved finding — a dawn–dusk atmospheric asymmetry on the ultra-hot Jupiter wasp-121b (Gapp et al., Nature Astronomy, 2026) — independently reinforces that blended-disc methods miss longitudinal structure (src-jwst-wasp-121b-dawn-dusk-2026-06).