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by yongjik
3118 days ago
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This unfortunately reminds me too much of stellar evolution timetable[1]: > Star burns through a succession of nuclear fusion fuels: Hydrogen burning: 10 Myr
Helium burning: 1 Myr
Carbon burning: 1000 years
Neon burning: ~10 years
Oxygen burning: ~1 year
Silicon burning: ~1 day
(...and then it goes supernova.)I hope Bitcoin's end is not as violent. :/ [1] http://www.astronomy.ohio-state.edu/~pogge/Ast162/Unit3/supe... |
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