| n = p-2 | n = p-1 | n = p | n = p+1 | n = p+2 |
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H 001 99.985% Stable |
n | |||
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H 002 0.015% Stable |
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He 003 0.000137% Stable |
H 003 12.33 yr |
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Li 004 |
He 004
99.999863% Stable |
H 004 |
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Above and at left you find four varient charts in HTML format. Nuclide
identities displayed in this fashion comprise The Incremental Table of
Atomic Isobars.
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Cube Octahedral Equation Icosahedral Equation Our discussion left off examining the isobar-8 so we pick up on isobar-9 which does have a stable nuclide. | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
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We still have the issue of the cube at hand but the rolly/floppy trait is
mitagated, again by the addition of a central nucleon as was the case
with isobar-7. Hence Be-9 is the only stable isotope of Beryllium. All this makes much sence in terms of both close packing and spherical division. If I were to have you guess which isotope of Boron is the most common B-10 or B-11 what information would you use to guide your choice. Observe to your left, the nuclides Li-7, Be-9, and B-11 are marked off with orange, this denotes them as Most Common Isotope. The yellow is used to mark off the nuclides as SUPER Stable for the six most abundant elements. I consider these six isobars as durable beyond stable and favored by nature. The forth most plentiful element is Neon, we will add that now. The fifth and sixth are already on the the chart, Carbon and Nitrogen. we will observe what paterns arise and begin our discusion anew. | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
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Somewhere I ran across a list of the most common elements in the cosmos. I then learned that neon, fourth on the list, was more plentiful than both iron and silicon and is abundant in interstellar space. I knew something was amiss. The Moon-Hecht model does not mark off neon with a completed proton shell and gives no explanation for abundant neon. This idea sat still for a few years!
Stars produce helium from hydrogen and if they have enough mass they begin to burn helium to heavier elements though what is called the C-N-O process. What element would a star produce if it were massive enough to burn oxygen? Yes neon! This nagged at me so I discarded the proton at the vertex notion and played around with the idea of a system of shells but discounted any distinction between protons and neutrons and with each of the eleven most common elements of the cosmos the atomic weight values were found to be additions of platonic numbers ie. 4, 6, 8, 12, and 20. The idea sat for a few more years as the notion of "stability by degree had not fully come upon me.
| n = p-3 | n = p-2 | n = p-1 | n = p | n = p+1 | n = p+2 | n = p+3 | n = p+4 | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
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H 001 99.985% Stable |
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H 002 0.015% Stable |
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He 003 0.000137% Stable |
H 003 12.33 yr |
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Li 004 |
He 004
99.999863% Stable |
H 004 |
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Li 005 |
He 005 |
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Be 006 |
Li 006
7.5% Stable |
He 006 |
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B 007 |
Be 007 |
Li 007
92.5% Stable |
He 007 |
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B 008 |
Be 008 |
Li 008 |
He 008 |
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| llllllllllllllllll | llllllllllllllllll | llllllllllllllllll | llllllllllllllllll | llllllllllllllllll | llllllllllllllllll | llllllllllllllllll | llllllllllllllllll | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| The above table is useful when undertaking a study of stellar nucleosynthesis regarding the non-popularity of the Isobars 5 and 8, however its placement here is to provide an example of how data can be displayed different than that of the Segre Chart. |
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