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Brown dwarf stars, often referred to as "failed stars," have an extensive lifespan that can exceed several billion years. Unlike stars that undergo nuclear fusion, brown dwarfs burn their residual heat slowly and do not have a defined end point like more massive stars. They can remain stable and detectable for tens of billions of years, making their life expectancy significantly longer than that of typical stars. As a result, they can persist for a substantial portion of the universe's lifespan.

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5d ago

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