Quote: Originally posted by neptunium | the natural reactor in Africa is the proof of what nature can do alone.. so if Pu244 cannot be generated, where does that leaves us for Unbibium 292
and Marinov`s claim?
exactly!! |
He is looking for primordial super-heavy elements that may have survived from the last supernova explosion in the r-process to enrich the solar system
at its birth, not ones made on Earth by natural fission or cosmic ray neutrons. Since Sm-146, with a 108 million year half-life has survived from that
event, then other 100 million year half-life nuclides will as well.
But without an inert natural carrier (stable samarium) there is no known way for the them to become concentrated to detectable levels, if they exist.
Think about the samarium situation. Stable isotope ratios vary throughout the solar system at the level of a few percent or less.* So any ancient
samarium, however far it has decayed today, will still be present in any modern samarium sample, if there is any at all. This is really helpful in
finding it.
When looking for new elements, which may exist on Earth at the same quantity, we do not have this convenient concentration and identification
mechanism.
*This variation is due to fractionation processes after the early nebula collapsed (and which is thought to have been thoroughly mixed and quite
uniform). |