Lectures | Lecture page | Astro103 page |
slow depletion of Hydrogen
Contraction of the helium core -- ``ash''
Burning of Hydrogen in a shell around core
Very intense -
But not hotter!
it must get bigger
A red Giant!
When: Helium fusion ignites explosively
When electrons (or any fundamental particles) are squeezed too hard together, they exert a quantum mechanical pressure due to the ``exclusion principle:''
Once fusion starts, it continues explosively until conditions are so hot the ``degeneracy'' is removed.
. . . and when the fuel's spent?
Contraction of the Carbon core -- ``ash''
Burning of Helium in a shell around core
Burning of Hydrogen in a shell around Helium shell
Very intense -
But not hotter!
it must get bigger
A red Super-Giant
(b) the distribution of evolved stars in the HR diagram
(c) the thermal layers in the collapsing proto-stellar cloud
(d) the layers of ``burning'' of different elements around the core
(e) the different time-scales for ``burning'' different elements
(b) The ratio of protons to neutrons remains constant
(c) degeneracy pressure equals regular pressure
(d) Carbon is being generated at the rate Hydrogen is depleted
(e) energy and matter are converted
Lectures | Lecture page | Astro103 page |