The Webb space telescope has captured auroras on Neptune for the first time, showing a bright auroral glow on the ice giant.
Neptune, located about 3 billion miles away from the sun, has been a challenging target for astronomers to observe due to its distance and cold environment.
Auroras on Neptune are created by energetic particles trapped in its magnetic field, which collide with the upper atmosphere, releasing energy and creating the signature glow.
The detection of auroras on Neptune was made possible by Webb's near-infrared sensitivity, providing clear and detailed images of the phenomenon.
Neptune's auroras are different from those on Earth, Jupiter, and Saturn, as they occur at the planet's mid-latitudes rather than at the poles.
The presence of the trihydrogen cation (H3+) in Neptune's atmosphere confirms the existence of auroral activity, with glowing auroras appearing as cyan splotches in the Webb images.
Neptune's magnetic field, which tilts at 47 degrees from its rotation axis, plays a significant role in the distribution of auroras at the planet's mid-latitudes.
Astronomers discovered a substantial cooling in Neptune's upper atmosphere since the Voyager 2 flyby in 1989, leading to fainter auroras and explaining why they were previously undetected.
The findings from the Webb observations suggest insights into Neptune's magnetic field dynamics and temperature changes, providing valuable information for future studies of the ice giant.
By studying Neptune over a full solar cycle, astronomers aim to unravel the mysteries of its magnetic field origin and tilt, paving the way for future missions to explore Uranus and Neptune.