Astronomers observe a brown dwarf star hotter than the Sun

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Astronomers observe a brown dwarf star hotter than the Sun
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The brown dwarf star has a temperature of roughly 8,000 kelvins, meaning it is more than 2,000 K hotter than the Sun.

Brown dwarfs have no nuclear fusion reaction in their core like other stars, and they have auroras and atmospheres with storms like planets. On the other hand, they can host their planets like other stars and emit measurable light.

The team of astronomers behind the new analysis looked at observations of the brown dwarf star WD 0032-317 B and the white dwarf WD 0032-317 made using the Ultraviolet and Visual Echelle Spectrograph of the European Southern Observatory's Very Large Telescope. They had expected to find another white dwarf orbiting WD 0032-317 but discovered that the binary system was made up of a white dwarf and a brown dwarf. Based on their observations, detailed in, they found that the brown dwarf has a mass roughly 75–88 times that of Jupiter.White dwarfs are the last evolutionary stage of low and medium-mass stars, like our Sun.

WD 0032-317 is unusually hot for a brown dwarf, mainly due to the intense ultraviolet radiation it receives from its neighboring white dwarf. The brown dwarf is also tidally locked to the white dwarf, meaning it always shows the same side. This means the side of the brown dwarf facing the white dwarf star is always roughly 6,000 K hotter than the night side.

Due to their strange planet-like nature, brown dwarfs are the coldest known star category in the cosmos. Recently a team of astronomers from the University of Sydney analyzed a small distant brown dwarf star with the catchy name T8 Dwarf WISE J062309.94−045624.6 and found that it is the

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