Robin van Spaandonk wrote:
1) Start with a single well shrunken hydrino 2) Add one electron to form Hydrinohydride. 3) Add one proton to form a Hydrino molecule. 4) With a fast particle, break the Hydrino molecule apart into two 5) Return to step one with two Hydrinos, thus doubling your inventory.
Nice bit of speculation. Rather thought provoking in the various implications, but not without a dark side .... Let's don't even go there.
However, it is pretty clear that all of these steps 1-5 would be expected to occur in the solar corona itself, so there is every likelihood that there is already a population of Hy2 in the solar wind and correspondingly in the oceans of earth.
Wish we knew how to harvest them. OTOH, perhaps they are very dense, as the small size suggests, and then they eventually might be expected to settle into the core of earth, being denser even than uranium.
That significant population in the solar corona would likely be true even if gamma radiation from the sun tends to break most Hy2 up as it forms, before it can traverse the 200,000 km thickness of the 'blacklight' part of the corona, and be ejected into the solar wind. There would be an equilibrium level which would increase the further out from the sun they were found.
One other thought. Looking at the hypothetical transmutation of argon + Hy2, and in light of earthly isotopes percentage -- this might be revealing.
99.6% of this gas on earth is 40Ar. Yet 38Ar is ostensibly stable. Yet it is of such extraordinarily low percentage that one wonders if the primordial population were not all 40Ar, and the 38AR is formed secondarily from interaction with Hy2 in the ionosphere. The reasoning behind this is not as moronic as it sounds at first, as very low isotopic percentages often have greater statistical meaning than is apparent -- but more on that later.
Many implications on the solar side, and even more for a hydrino breeder on earth. This could definitely solve all future energy needs of the planet.
Jones
