NASA's James Webb Space Telescope has captured bright auroral activity on Neptune for the first time, revealing the long-sought auroral glow.
Auroras on Neptune are caused by energetic particles trapped in the planet's magnetic field, creating a distinctive glow when they collide with the upper atmosphere.
Previous attempts to image and confirm auroras on Neptune were challenging, making it the missing piece in understanding auroral activity on the giant planets in our solar system.
Using Webb's near-infrared sensitivity, researchers were able to capture detailed images of the auroras on Neptune, showcasing the uniqueness of its auroral activity.
The data collected by Webb also revealed the presence of the trihydrogen cation (H3+) in Neptune's atmosphere, a clear sign of auroral activity.
Unlike Earth, Jupiter, or Saturn, Neptune's auroras are located at mid-latitudes due to the planet's tilted magnetic field, offering new insights into its atmospheric dynamics.
The discovery of Neptune's auroras will aid in understanding its magnetic field interactions with solar particles and provide valuable information for future studies.
Webb's observations indicated a significant temperature drop in Neptune's upper atmosphere since 1989, impacting the intensity of the detected auroral activity.
Future studies using Webb aim to explore Neptune over a solar cycle to unravel mysteries related to its magnetic field and atmospheric dynamics.
This groundbreaking research on Neptune's auroras was led by a team of astronomers and has been published in Nature Astronomy.