When Will the Sun Transition to a Black Dwarf?

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SUMMARY

The sun is projected to transition to a black dwarf in over a trillion years, with estimates suggesting it could take up to 2 trillion years to cool below 800 K. According to Barrow and Tipler, a white dwarf cools to 5 K in approximately 1015 years, but the presence of weakly interacting massive particles (WIMPs) may prolong this cooling process for up to 1025 years. Current temperatures of white dwarfs, around 4000 K, indicate that significant cooling is required before reaching black dwarf status.

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  • Understanding of stellar evolution and lifecycle
  • Knowledge of thermodynamics related to stellar objects
  • Familiarity with white dwarf characteristics and cooling processes
  • Basic concepts of particle physics, specifically weakly interacting massive particles (WIMPs)
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  • Research the cooling rates of white dwarfs and factors affecting them
  • Explore the role of WIMPs in astrophysics and their implications for stellar cooling
  • Study the lifecycle of stars, focusing on the transition from white dwarf to black dwarf
  • Investigate the thermodynamic principles governing heat escape in stellar objects
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Astronomers, astrophysicists, and students of stellar evolution who are interested in the long-term fate of stars and the physical processes involved in their cooling and transition to black dwarfs.

Richard87
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At what point in time will the sun become a black dwarf? A trillion years?
 
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Longer than a trillion years.

From wikipedia:

"Barrow and Tipler estimate that it would take 10[sup15[/sup] years for a white dwarf to cool to 5 K; however, if weakly interacting massive particles exist, it is possible that interactions with these particles will keep some white dwarfs much warmer than this for approximately 1025 years."

(And WIMPs are a rather good bet)
 
When I read the title I thought of gary coleman for a split second.

Yeah I think its a trillion years
 
Depends on how you define "black" since WIMP heating, according to Adams & Laughlin's estimates, will heat a white dwarf to 63 K, making it still glowing in IR. But if we're talking below the temperature at which an object glows with its own heat, roughly 800 K, then a white dwarf that's presently at ~4000 K will take about ~2 trillion or so years to cool to that point. An isothermal ball would cool quicker (just ~1 trillion years), but real white dwarfs have an opaque outer crust which slows down the escape of heat.
 

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