n =
|
p-1 | p |
p+1 | p+2 |
p+3 | p+4 |
H 1 |
|
n |
| | |
|
H 2 |
| |
| |
He 3 |
|
H 3 |
|
| |
|
He 4 |
| |
| |
| |
| |
| |
|
Li 6 |
| |
| |
Be 7 |
|
Li 7
| |
| |
| |
| |
| |
| |
Be 9 |
|
| |
|
B 10 |
|
Be 10 |
| |
| |
B 11 |
|
| |
|
C 12 |
| |
| |
| |
C 13 |
|
| |
|
N 14 |
|
C 14 |
| |
| |
N 15 |
|
| |
|
O 16 |
| |
| |
| |
O 17 |
|
| |
|
| |
O 18 |
| |
| |
F 19 |
|
| |
|
Ne 20 |
| |
| |
| |
Ne 21 |
|
| |
| |
|
Ne 22 |
| |
| |
Na 23 |
|
| |
|
The Incremental Tables are available for your use as you see fit. There are at least three
immediate paths of invetigation you may take to acquaint your self with what The Incremental
Table format can do for you.
One path of investigation could be to flesh out a table by adding all the radionuclides row by
row starting with the short tables.
Stable Isobars to (4)
n = p-1 |
n = p |
001 99.985%
SUPER
Stable
1.007825
|
|
|
002 0.015%
Stable
2.0141017
|
003 0.000137%
Stable
3.0160293
|
|
|
004 99.999863%
SUPER
Stable
4.0026032
|
4c
- -
6a
A different path could be to examine the pattern of all stable Nuclides in incrementing Isobar
rows without labels.
|
A third path would be, as I suggest below, is to begin with elements
appraised as most abundant and add in the less plentiful
as they rank in abundance. The chart crust displays
the most abundant elements
of the earth's crust in the left column, in the right column the elements are reoganized
in order of atomic number.