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Webb Produces First 3D Map of Uranus’s Upper Atmosphere

The vertical map ties the planet’s auroral structure to its off‑center magnetic field to clarify how ice giants move energy.

Overview

  • Using JWST’s NIRSpec Integral Field Unit, researchers observed Uranus for nearly a full 15‑hour rotation on 19 January 2025 and mapped up to 5,000 kilometers above the cloud tops.
  • Temperatures peak between roughly 3,000 and 4,000 kilometers while ion densities peak near 1,000 kilometers, with an average temperature of about 426 K that is lower than prior measurements.
  • Webb data confirm a multi‑decade cooling trend in Uranus’s upper atmosphere first noted in the early 1990s.
  • Two bright auroral bands appear near the magnetic poles with a depleted region between them, features linked to the planet’s highly tilted and offset magnetic field and its changing field lines.
  • The peer‑reviewed study, led by Paola Tiranti under JWST GO program 5073 (PI Henrik Melin) and published in Geophysical Research Letters, provides a first vertical view of the ionosphere and includes a timelapse spanning nearly one Uranian day.