AstronomyWebb finds signs of possible aurorae on isolated brown...

Webb finds signs of possible aurorae on isolated brown dwarf

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This artist idea portrays the brown dwarf W1935, which is situated 47 light-years from Earth. Astronomers utilizing NASA’s James Webb Area Telescope discovered infrared emission from methane coming from W1935. That is an sudden discovery as a result of the brown dwarf is chilly and lacks a number star; subsequently, there is no such thing as a apparent supply of vitality to warmth its higher environment and make the methane glow. The crew speculates that the methane emission could also be as a consequence of processes producing aurorae, proven right here in purple. Credit score: NASA, ESA, CSA, Leah Hustak (STScI)

Astronomers utilizing NASA’s James Webb Area Telescope have discovered a brown dwarf (an object extra huge than Jupiter however smaller than a star) with infrared emission from methane, seemingly as a consequence of vitality in its higher environment. That is an sudden discovery as a result of the brown dwarf, W1935, is chilly and lacks a number star; subsequently, there is no such thing as a apparent supply for the higher environment vitality. The crew speculates that the methane emission could also be as a consequence of processes producing aurorae.

These findings are being introduced on the 243rd meeting of the American Astronomical Society in New Orleans.

To assist clarify the thriller of the infrared emission from methane, the crew turned to our solar system. Methane in emission is a typical function in fuel giants like Jupiter and Saturn. The upper-atmosphere heating that powers this emission is linked to aurorae.

On Earth, aurorae are created when energetic particles blown into space from the sun are captured by Earth’s magnetic area. They cascade down into our environment alongside magnetic field lines close to Earth’s poles, colliding with fuel molecules and creating eerie, dancing curtains of sunshine. Jupiter and Saturn have related auroral processes that contain interacting with the solar wind, however additionally they get auroral contributions from close by lively moons like Io (for Jupiter) and Enceladus (for Saturn).

For remoted brown dwarfs like W1935, the absence of a stellar wind to contribute to the auroral course of and clarify the additional vitality within the upper atmosphere required for the methane emission is a thriller. The crew surmises that both unaccounted inner processes just like the atmospheric phenomena of Jupiter and Saturn, or exterior interactions with both interstellar plasma or a close-by lively moon could assist account for the emission.

A detective story

The aurorae’s discovery performed out like a detective story. A crew led by Jackie Faherty, an astronomer on the American Museum of Pure Historical past in New York, was awarded time with the Webb telescope to analyze 12 chilly brown dwarfs. Amongst these have been W1935—an object that was found by citizen scientist Dan Caselden, who labored with the Yard Worlds Zooniverse challenge—and W2220, an object that was found utilizing NASA’s Broad Discipline Infrared Survey Explorer.

Webb revealed in beautiful element that W1935 and W2220 seemed to be close to clones of one another in composition. Additionally they shared related brightness, temperatures, and spectral options of water, ammonia, carbon monoxide, and carbon dioxide. The hanging exception was that W1935 confirmed emission from methane, versus the anticipated absorption function that was noticed towards W2220. This was seen at a definite infrared wavelength to which Webb is uniquely delicate.

“We anticipated to see methane as a result of methane is throughout these brown dwarfs. However as an alternative of absorbing mild, we noticed simply the other: The methane was glowing. My first thought was, what the heck? Why is methane emission popping out of this object?” mentioned Faherty.

Webb finds signs of possible aurorae on isolated brown dwarf
Astronomers used NASA’s James Webb Area Telescope to review 12 chilly brown dwarfs. Two of them – W1935 and W2220 – seemed to be close to twins of one another in composition, brightness, and temperature. Nevertheless, W1935 confirmed emission from methane, versus the anticipated absorption function that was noticed towards W2220. The crew speculates that the methane emission could also be as a consequence of processes producing aurorae. Credit score: NASA, ESA, CSA, Leah Hustak (STScI)

The crew used pc fashions to deduce what is perhaps behind the emission. The modeling work confirmed that W2220 had an anticipated distribution of vitality all through the environment, getting cooler with rising altitude. W1935, alternatively, had a shocking consequence. The very best mannequin favored a temperature inversion, the place the environment obtained hotter with rising altitude.

“This temperature inversion is de facto puzzling,” mentioned Ben Burningham, a co-author from the College of Hertfordshire in England and lead modeler on the work. “We now have seen this type of phenomenon in planets with a close-by star that may warmth the stratosphere, however seeing it in an object with no apparent exterior warmth supply is wild.”

Clues from our solar system

For clues, the crew seemed in our personal yard to the planets of our solar system. The gas giant planets can function proxies for what’s seen occurring greater than 40 light-years away within the environment of W1935.

The crew realized that temperature inversions are distinguished in planets like Jupiter and Saturn. There’s nonetheless ongoing work to grasp the causes of their stratospheric heating, however main theories for the solar system contain exterior heating by aurorae and inner vitality transport from deeper within the environment (with the previous a number one rationalization).

Brown dwarf aurora candidates in context

This isn’t the primary time an aurora has been used to elucidate a brown dwarf commentary. Astronomers have detected radio emission coming from a number of hotter brown dwarfs and invoked aurorae because the probably rationalization. Searches have been carried out with ground-based telescopes just like the Keck Observatory for infrared signatures from these radio-emitting brown dwarfs to characterize the phenomenon additional however have been inconclusive.

W1935 is the primary auroral candidate exterior the solar system with the signature of methane emission. It is also the coldest auroral candidate exterior our solar system, with an efficient temperature of about 400 levels Fahrenheit (200 levels Celsius), about 600 levels Fahrenheit hotter than Jupiter.

In our solar system, the solar wind is a major contributor to auroral processes, with lively moons like Io and Enceladus enjoying a task for planets like Jupiter and Saturn, respectively. W1935 lacks a companion star totally, so a stellar wind can not contribute to the phenomenon. Whether or not an lively moon may play a task within the methane emission on W1935 is but to be seen.

“With W1935, we now have a spectacular extension of a solar system phenomenon with none stellar irradiation to assist in the reason,” Faherty famous. “With Webb, we will actually ‘open the hood’ on the chemistry and unpack how related or totally different the auroral course of could also be past our solar system,” she added.

Quotation:
Webb finds indicators of doable aurorae on remoted brown dwarf (2024, January 10)
retrieved 10 January 2024
from https://phys.org/information/2024-01-webb-aurorae-isolated-brown-dwarf.html

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