| He 2 | Ne 10 | Ar 18 | Kr 36 | Xe 54 | Rn 86 | Uu o 118 | Uho 168 | Buo 218 |
The algorithm is important for the outer structure and appearance of the atom-cover.
The chemical and physical qualities are caused here.
The rare-gas-algorithm is bandage-limb and seam-position between two shells.
It defines the borderline between two shells.
It defines also how many shells / orbital can be existing.
Noble-gases possess the stable electron- configuration of all elements.
An inert-gas represents the sum of all used orbital of its shell-subgroup.
" However. Pauli´s Nobel Prize-winning work did not provide a solution to the question
which I shall call the "closing of the periods"-- that is why the periods end, in the sense of
achieving a full-shell configuration, at atomic numbers 2, 10, 18, 36, 54, and so forth. "
Literature Cited: Scerri, Eric R. Journal of Chemical Education Vol.75 No.11, Nov 1998, P.1384
How Good is the Quantum Mechanical Explanation of the Periodic System?
![[Picture]](../images/aglarule.gif)
The Inert-gases can be calculated with this algorithm.
| A(n)=Int((n+2)/2)^2*2 | see also: mathematical formulas or | |
| E(n) = E (n-1) + A(n) | download: Excel-file formel.zip (7KB) |
![[Picture]](../images/aglarule.gif)
Approximation-formula for the inert-gas algorithm (tendencial)
y = -1E-21x^6 + 3E-17x^5 - 2E-13x^4 + 0,1667x^3 + x^2 + 2,0551x
![[Picture]](../images/aglarule.gif)
| No. | Melting Point °C | Melting Point ° F | Boiling Point °C | Boiling Point ° F |
| 2 | -272 | -457,6 | -268,6 | -451,48 |
| 10 | -248,6 | -415,48 | -246,1 | -410,98 |
| 18 | -189,3 | -308,812 | -186 | -302,8 |
| 36 | -157,2 | -250,96 | -153,4 | -244,12 |
| 54 | -111,9 | -169,42 | -108,1 | -162,58 |
| 86 | -71 | -95,8 | -61,8 | -79,24 |
| 118 | -30,3 | -22,54 | -22,6 | -8,68 |
| 168 | 11,1 | 51,98 | 19,7 | 67,46 |
| 218 | 52,4 | 126,32 | 62,0 | 143,6 |
| 290 | 93,8 | 200,84 | 104,3 | 219,74 |
| 362 | 135,1 | 275,18 | 146,6 | 295,88 |
| 460 | 176,5 | 349,7 | 188,9 | 372,02 |
| 558 | 217,8 | 424,04 | 231,2 | 448,16 |
| 686 | 259,2 | 498,56 | 273,5 | 524,3 |
| 814 | 300,5 | 572,9 | 315,8 | 600,44 |
| 976 | 341,9 | 647,42 | 358,1 | 676,58 |
| 1138 | 383,2 | 721,76 | 400,4 | 752,72 |
| 1338 | 424,6 | 796,28 | 442,7 | 828,86 |
| 1538 | 465,9 | 870,62 | 485,0 | 905 |
| 1780 | 507,3 | 945,14 | 527,3 | 981,14 |
| 2022 | 548,6 | 1019,48 | 569,6 | 1057,28 |
| 2310 | 589,9 | 1093,82 | 611,9 | 1133,42 |
| 2598 | 631,3 | 1168,34 | 654,2 | 1209,56 |
(tendencial)
y = 1E-15x^6 - 2E-12x^5 + 6E-10x^4 + 7E-08x^3 - 5E-05x^2 + 1,025x + 8,7552
![[Picture]](../images/aglarule.gif)
| APSIDIUM © | Created: | 2001-01-13 | nobelgass.pdf | |
| Last Updated: | 2003-03-25 |
![[Picture]](../images/aglarule.gif)
J. Li, B. E. Bursten, B. Liang, and L. Andrews, "Noble Gas-Actinide Compounds:
Complexation of the CUO Molecule by Ar, Kr, and Xe Atoms in Noble-Gas Matrices,"
Science, 295, 2242-2245 (2002).
http://www.chemistry.ohio-state.edu/cgi/brochure?Faculty=bursten