In reply to  Rick Monteverde's message of Sun, 30 Jan 2005 12:43:39 -1000:
Hi,
[snip]
><wildspeculation> Since the event seemed to develop 'slowly' at first, how 
>about this - a bubble of H & O2 did develop and ignite, but in a burn still 
>slow and/or small enough to be mechanically absorbed by the system. As the 
>fuel was consumed, then - perhaps even synchronously with a returning shock 
>wave from the walls of the vessel from the initial burn - the bubble collapses 
>down against the site of reactions on the screen, causing a tiny supernova. 
></wildspeculation>
[snip]
More wildspeculation; Supernovas may be triggered by hydrino formation and 
collapse when the He3 level at the surface of a large star gets high enough.
(It almost has to be at the surface, because the core is too hot to allow much 
H to exist).

Regards,


Robin van Spaandonk

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