On Fri, 18 Sep 2009 04:05:50 -0700, you wrote:

>
>Hello list, 
>These metallic elements are so common in stony meteorites - as we know... now, 
>don't they originally form at the cores of stars, and the traces of these 
>metals that contained during the earliest days of the formation of our Solar 
>System, are the remnants of nearby dead stars that exploded millions or 
>billions of years before the Solar System started to emerge? 
>

Everything heavier than hydrogen, helium (and a little bit of Lithium and
Beryllium) was cooked up in stars.
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