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: http://star.arm.ac.uk/~jgd/future.html
Дата изменения: Wed Jan 17 15:58:26 2001 Дата индексирования: Mon Oct 1 21:18:23 2012 Кодировка: |
Point A is where the Sun starts
Hydrogen fusion
Point B is where about half of
the supply of the hydrogen in the core has been used up. This is where
the Sun is in its lifetime right now.
Point C is reached when there is
no more hydrogen in the core and the fusion of hydrogen starts in the shell
around the core. The radius of the Sun will swell to 40% larger than its
present size and twice its present luminosity.
At point D, approximately one and
a half billion years later, the surface of the Sun will be 3.3 times the
size it is now and have a temperature of about 4300 degrees. The temperature
on Earth will increase by 100 degrees, causing all the seas to evaporate
and destroying life on Earth as we know it. Within another 250 million
years, the Sun will grow 100 times larger than it is now and 500 times
more luminous.
At point E the core temperature
of the Sun will rise so high that in one bang, all the rest of the helium
will fuse into carbon, causing one third of the solar envelope to be thrown
out into space.