JWST Provides First 3D Map of Uranus's Upper Atmosphere
The James Webb Space Telescope has delivered the first three-dimensional mapping of Uranus's ionosphere, revealing temperature variations and auroral structures influenced by the planet's unique magnetic field.
An international team of astronomers has utilized the James Webb Space Telescope (JWST) to create the first three-dimensional map of Uranus's upper atmosphere, known as the ionosphere. This region, extending up to 5,000 kilometers above the planet's cloud tops, is where the atmosphere becomes ionized and interacts with Uranus's magnetic field.
The study, led by Paola Tiranti of Northumbria University in the United Kingdom, employed JWST's Near-Infrared Spectrograph (NIRSpec) to observe Uranus for nearly a full rotation. The observations revealed that temperatures in the ionosphere peak between 3,000 and 4,000 kilometers above the cloud tops, while ion densities reach their maximum around 1,000 kilometers. These findings indicate significant vertical variations within the atmosphere, likely influenced by the planet's unusually tilted magnetic field.
Additionally, the team detected two bright bands of auroral emission near Uranus's magnetic poles, along with a region of depleted emission and density. These structures are thought to be shaped by the unique geometry of Uranus's magnetic field, which is both tilted and offset from the planet's rotation axis.
The study also confirmed that Uranus's upper atmosphere has been cooling since the 1990s, with current average temperatures around 426 Kelvin (153°C), lower than previous measurements. This ongoing cooling trend provides new insights into the energy dynamics of ice giant planets.
These findings offer a deeper understanding of Uranus's atmospheric structure and magnetic interactions, contributing to broader knowledge about ice giants and their behavior within our solar system.