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- From: tarl@sw.stratus.com (Tarl Neustaedter)
- Newsgroups: sci.astro
- Subject: Re: Supernova
- Message-ID: <1eglhnINNm1s@transfer.stratus.com>
- Date: 19 Nov 92 18:14:15 GMT
- References: <1992Nov10.180131.9356@sfu.ca> <1992Nov14.043817.3016@monu6.cc.monash.edu.au> <1edk30INNbd7@transfer.stratus.com> <1992Nov18.172149.27436@Princeton.EDU>
- Organization: Stratus Computer, Inc.
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-
- In article <1992Nov18.172149.27436@Princeton.EDU>, richmond@spiff.Princeton.EDU (Stupendous Man) writes:
- > Actually, while Tarl has explained the slow, gradual brightening of a
- > type II supernova nicely (except for the "light-hours bit" - the envelope
- > of even the largest star is only light-minutes in radius),
-
- *Blush*. I was thinking of the time for the shockwave to travel through
- the star and brain-faulted on light being a different velocity.
-
- > [flash at time of core collapse - neutrinos interact with stellar envelope]
- > If I recall correctly, the "flash" is only a few seconds (minutes?) long
-
- Interesting idea - I hadn't heard of this. But again, this would not be
- perceived by the human eye as a flash, since the same spherical delay
- would cause it to be minutes long.
-
- However, if we assume that the outer envelope of the star is mostly hydrogen
- and helium (a blue giant's chromosphere would not be dominated by metals
- even in the late stages of life), the neutrino-provoked reactions would be:
-
- u + 2D -> 2He =>>> H + H (sproing!)
- u + 3T -> 3He
- u + 3He -> 3Li ==>>>> H + H + H (SSSPpPpPRoing!)
- u + 4He -> 4Li =>>> H + 3He
-
- The cross-sections for some of these have got to be almighty tiny. Would
- there be enough energy converted to heat in this flash to approach within
- 5 magnitudes of the maximum luminosity? Otherwise, this flash would not
- have even brought Sk -69.202 to naked-eye visibility.
- --
- Tarl Neustaedter tarl@sw.stratus.com
- Marlboro, Mass. Stratus Computer
- Disclaimer: My employer is not responsible for my opinions.
-