What is the mystery light NASA’s telescope just picked up around this failed star?
Astronomers found signs of auroral activity on an isolated brown dwarf after investigating the celestial objects using the James Webb Space Telescope.
Astronomers witnessed mysterious light around a failed star in an unexpected celestial discovery using NASA’s James Webb Space Telescope.
A group of astronomers witnessed infrared emissions from methane surrounding a brown dwarf, likely due to energy in its upper atmosphere and indicating it as an aurora akin to Earth's northern and southern lights, NASA announced Tuesday. But the problem is that there's no clear source for that energy.
"We expected to see methane because methane is all over these brown dwarfs," said Jackie Faherty, an astronomer at the American Museum of Natural History in New York who was awarded time to investigate 12 brown dwarfs using the JWST. "But instead of absorbing light, we saw just the opposite: The methane was glowing. My first thought was, what the heck? Why is methane emission coming out of this object?"
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Brown dwarfs are commonly known as failed stars since they have greater masses than even large planets like Jupiter, but still aren't large enough to create the nuclear fusion that powers stars, according to NASA.
The one Faherty's team recently discovered, named W1935, isn't near any apparent heat sources like stars, meaning it remains cold. They also found another brown dwarf that was nearly identical in composition and shared other significant features. Energy in that brown dwarf's atmosphere cooled with increasing altitude — as the astronomers expected.
But W1935, which is 47 light-years from Earth, for some reason warmed at higher altitudes, baffling Faherty's team.
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"This temperature inversion is really puzzling," Ben Burningham, a lead modeler of the brown dwarfs' computer model study, said. "We have seen this kind of phenomenon in planets with a nearby star that can heat the stratosphere, but seeing it in an object with no obvious external heat source is wild."
The astronomers looked at Jupiter and Saturn, which have aurorae of their own, for clues. They concluded that internal processes like those found on Jupiter and Saturn could be a heat source for W1935. Interstellar plasma or particles from a nearby active moon are alternative theories.
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Aurorae, like the northern and southern lights, occur when a charged particle collision releases a flash of light and heat in Earth's upper atmosphere, according to NASA. Astronomers have previously detected radio emissions from warmer brown dwarfs and predicted auroral activity as the most likely explanation, but W1935 is the first and coldest auroral candidate outside the solar system with the signature of methane emission, NASA said.
"With W1935, we now have a spectacular extension of a solar system phenomenon without any stellar irradiation to help in the explanation," Faherty said.
The JWST launched in December 2021, but took another six months to become fully operational and start showing glimpses into the vast universe. The $10 billion device has allowed astronomers, like Faherty and her team, to see "exquisite detail" of celestial objects as shown in the investigation of the brown dwarfs, NASA said.
"With Webb, we can really open the hood on the chemistry and unpack how similar or different the auroral process may be beyond our solar system," Faherty said.
Click here to see more JWST images.