NASA's James Webb Telescope reveals glowing auroras and stormy skies on a starless alien world

Astronomers from Trinity College Dublin utilized the telescope's unmatched precision to study the starless world SIMP-0136, a fascinating rogue planet.
PUBLISHED 4 HOURS AGO
An artist’s concept shows what the isolated planetary-mass object SIMP 0136 could look like based on recent observations from NASA’s James Webb Space Telescope (Cover Image Source: NASA, ESA, CSA | Joseph Olmsted; edited by Starlust staff)
An artist’s concept shows what the isolated planetary-mass object SIMP 0136 could look like based on recent observations from NASA’s James Webb Space Telescope (Cover Image Source: NASA, ESA, CSA | Joseph Olmsted; edited by Starlust staff)

In a groundbreaking "weather report" from beyond our solar system, the James Webb Space Telescope (JWST) has provided the most precise atmospheric analysis to date of a searing-hot, free-floating world. A team of astronomers from Trinity College Dublin leveraged the telescope's unprecedented sensitivity to study SIMP-0136, a rogue planet that orbits no sun, as per Trinity College Dublin

An artist’s impression of the extrasolar world, SIMP-0136 (Image Source: Trinity College Dublin | Dr Evert Nasedkin)
An artist’s impression of the extrasolar world, SIMP-0136 (Image Source: Trinity College Dublin | Dr Evert Nasedkin)

The key takeaway from the new data is the discovery of intense, Northern Lights-like activity, characterized by powerful auroras that dramatically heat the planet's upper atmosphere, similar to the displays observed on Earth and Jupiter. The observations, which tracked minuscule variations in the planet’s brightness as it rotated, allowed researchers to map changes in its temperature and chemical composition. The findings, published in Astronomy & Astrophysics, paint a picture of a turbulent world.

The Aurora Borealis appears in the sky on January 8, 2017 near Ester Dome mountain about 10 miles west of Fairbanks, Alaska (Cover Image Source: Getty | Lance King)
The Aurora Borealis appears in the sky on January 8, 2017 near Ester Dome mountain about 10 miles west of Fairbanks, Alaska (Representative Image Source: Getty | Lance King)

"At over 1,500° C, SIMP-0136 makes this summer’s heat wave look mild,” stated lead author Dr. Evert Nasedkin, a Postdoctoral Fellow in Trinity’s School of Physics. The subtle temperature fluctuations, measured to within 5 degrees Celsius, suggested the presence of rotating atmospheric disturbances resembling Jupiter's Great Red Spot. Surprisingly, however, the planet’s heavy cloud cover remained uniformly constant across its surface. These aren't water clouds; given the extreme heat, they are made of silicate grains, the same material found in sand. 

This April 1, 2018, enhanced-color image of Jupiter’s Great Red Spot was captured by NASA’s Juno spacecraft (Image Source: NASA/JPL-Caltech)
This April 1, 2018, enhanced-color image of Jupiter’s Great Red Spot was captured by NASA’s Juno spacecraft (Image Source: NASA/JPL-Caltech)

By analyzing the light across different wavelengths, the team was able to infer the weather dynamics, from the atmospheric temperature and chemical makeup to the precise location of the clouds. The findings demonstrate the immense power of combining JWST's cutting-edge datasets with advanced modeling techniques. 

The James Webb Space Telescope (JWST or Webb) observes outer space to detect anomalies. Elements of this image are furnished by NASA (Representative Image by alex-mit / Getty Images)
The James Webb Space Telescope (JWST or Webb) observes outer space to detect anomalies. Elements of this image are furnished by NASA (Representative Image Source: Getty | alex-mit)

SIMP-0136 is a behemoth located just 20 light-years from Earth in the constellation Pisces, according to NASA. While it possesses the structure and composition of a gas giant, it holds the unusual designation of a rogue planet because it is not gravitationally bound to any host star. This free-floating giant is roughly 13 times the mass of Jupiter and is estimated to be approximately 200 million years old, making it one of the brightest isolated planets or brown dwarfs visible from the Northern Hemisphere. Despite its scorching surface temperature of approximately 825° C (about 1,500° F), it is relatively cool compared to stars. This means it emits insufficient visible light to be seen from Earth, nor does it have a sun to illuminate it.



 

Researchers carefully monitored SIMP-0136's brightness over two full rotations in July 2023. By tracking the subtle variations in light across different wavelengths, they could detect a variety of atmospheric phenomena as different sides of the object rotated into view. This analysis not only revealed the varying cloud cover at different atmospheric depths and the precise temperature changes in the high atmosphere but also illuminated shifts in its carbon chemistry, providing a detailed picture of the giant’s complex atmospheric dynamics. The ability to map such detailed changes on a world so distant and dark underscores a revolutionary step in understanding exoplanetary science. 

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