
The James Webb Space Telescope (JWST) has spotted stormy weather in the two brown dwarfs' sky as it made a weather report of such "failed stars".
The twobrown dwarfs have formed a binary pair known as WISE 1049AB which was spotted byNASA's Wide-field Infrared Survey Explorer (WISE) in 2013. The two brown dwarfs are just 6.5light-yearsaway from Earth.
These are the closest brown dwarfs to oursun and hence became the best target for powerfulinfrared instruments of theJames Webb Space Telescope.
A brown dwarf is a celestial object which is big enough to ignite thenuclear fusionof hydrogen to helium and turn into a full-fledgedstar.
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It is also considered big enough to become a planet. The brown dwarfs are believed to be a missing link betweenlowest mass starsM-dwarfs and gas giant planetslikeJupiter.
Earlier, the atmosphere of various brown dwarfs has been investigated, however, due to time-averaged snapshots, the changes in the brown-dwarf atmosphere were not visible.
The brown dwarfs rotate very fast like WISE 1049A which spins on its axis once every 7 hours and the other one once every 5 hours.
The conditions in the atmospheres of the brown dwarfs can alter over time which meant that the scientists were missing a lot of variabilities in their observations.
However, the JWST has the ability to detect the changes over time.
A team headed by the University of Edinburgh's Beth Biller used JWST's Mid-Infrared Instrument (MIRI) to observe WISE 1049AB for 8 hours and then spent another seven hours on it using its Near-Infrared Spectrometer (NIRSpec).
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The researchers discovered that brown dwarfs have tumultuous clouds which are composed of silicate grains and are sweltering in temperatures between 875 degrees Celsius (1,610 degrees F) and 1,026 degrees Celsius (1880 degrees F).
This meant that hot sand was blowing in the winds on the brown dwarfs and it also had carbon monoxide, methane and water vapour in it.
"Our findings show that we are on the cusp of transforming our understanding of worlds far beyond our own," Biller said, in astatement.
"Insights such as these can help us understand the conditions not just on celestial objects like brown dwarfs, but also on giant exoplanets beyond oursolar system. Eventually, the techniques we are refining here may enable the first detections of weather onhabitable planetslike our own, which orbit other stars," he said.
(With inputs from agencies)