This article has been reviewed according to Science X's editorial process and policies. Editors have highlighted the following attributes while ensuring the content's credibility: NASA's SPHEREx (Spectro-Photometer for the History of the universe, Epoch of Reionization, and ices Explorer) space telescope is shedding light on brown dwarfs, celestial objects that blur the line between stars and exoplanets. New findings published in The Astrophysical Journal show that these dark and cloudy worlds have chemically rich atmospheres not unlike the giant planets in our own solar system.
First discovered in the 1990s, brown dwarfs form from collapsing clouds of gas, like stars do, but they aren't hefty enough to sustain hydrogen fusion in their cores. These dimly glowing balls of warm gas also share characteristics with Jupiter and Saturn. In contrast to most planets, however, brown dwarfs drift in darkness, ungoverned by a host star and heated entirely from within.
"They're kind of goth," said Zafar Rustamkulov, lead author of the new study and a scientist at IPAC, Caltech's science and data center in Pasadena, California. "Unlike exoplanets, free-floating brown dwarfs are completely independent celestial objects that will fade into eternity alone. We're still learning how complex they are." Only a few dozen of these "dark wanderers" have been studied in detail with space-based telescopes.
Astronomers want to observe more of them in the wild because much of our understanding of their makeup, storminess and evolution comes from theoretical models. Enter NASA's SPHEREx, an infrared space telescope launched in March 2025 and managed by the agency's Jet Propulsion Laboratory in Southern California. The study authors analyzed SPHEREx observations of 37 nearby brown dwarfs spanning the full brown dwarf temperature range, from about 4,000 to minus 10 degrees Fahrenheit (2,200 to minus 20 degrees Celsius).
The telescope measures their brightness in 102 different colors, from the deepest red our eyes can see to the invisible heat of infrared light, creating a spectrum. These spectra revealed chemically rich atmospheres harboring water, carbon dioxide, carbon monoxide and methane. "We're seeing the signatures of these molecules and how they change from object to object across the entire temperature regime," said study co-author J.
Davy Kirkpatrick, a scientist at Caltech's IPAC. "Our paper concentrated on just three dozen, but we have thousands more that we are in the process of analyzing. I really want to see what bounds the universe places on the variety of brown dwarfs." "From orbit, SPHEREx sees wavelengths of light that are basically impossible to see with telescopes on the ground because water in Earth's atmosphere absorbs them," Rustamkulov said.
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