#117 / 118
117Ts[294]
Superheavy / Unknownsolid at STPP-block

Tennessine

Group: 17Period: 7Standard Atomic Weight: [294] u

Why is Tennessine in this position?

Understanding the scientific rationale behind Tennessine's position in the periodic table:

Group Assignment
Group 17

Belongs to Group 17 (Halogens) as the heaviest halogen (7s² 7p⁵).

Period Assignment
Period 7

Belongs to Period 7 because its outermost electrons occupy n=7.

Orbital Block
P-block

Belongs to the p-block because its valence electrons fill 7p orbitals.

Chemical Category
Superheavy / Unknown

Classified as a superheavy halogen, though relativistic effects give it metallic properties.

Atomic Structure & Bohr Shell Model

Shell Distribution: [2, 8, 18, 32, 32, 18, 7]

Bohr Atomic Shell Model(2, 8, 18, 32, 32, 18, 7)

Hover or tap any shell orbit ring to inspect electron counts and 2n² capacities.

117 Protons (p⁺)177 Neutrons (n⁰)
KShell K: Electron 1 of 2Shell K: Electron 2 of 2LShell L: Electron 1 of 8Shell L: Electron 2 of 8Shell L: Electron 3 of 8Shell L: Electron 4 of 8Shell L: Electron 5 of 8Shell L: Electron 6 of 8Shell L: Electron 7 of 8Shell L: Electron 8 of 8MShell M: Electron 1 of 18Shell M: Electron 2 of 18Shell M: Electron 3 of 18Shell M: Electron 4 of 18Shell M: Electron 5 of 18Shell M: Electron 6 of 18Shell M: Electron 7 of 18Shell M: Electron 8 of 18Shell M: Electron 9 of 18Shell M: Electron 10 of 18Shell M: Electron 11 of 18Shell M: Electron 12 of 18Shell M: Electron 13 of 18Shell M: Electron 14 of 18Shell M: Electron 15 of 18Shell M: Electron 16 of 18Shell M: Electron 17 of 18Shell M: Electron 18 of 18NShell N: Electron 1 of 32Shell N: Electron 2 of 32Shell N: Electron 3 of 32Shell N: Electron 4 of 32Shell N: Electron 5 of 32Shell N: Electron 6 of 32Shell N: Electron 7 of 32Shell N: Electron 8 of 32Shell N: Electron 9 of 32Shell N: Electron 10 of 32Shell N: Electron 11 of 32Shell N: Electron 12 of 32Shell N: Electron 13 of 32Shell N: Electron 14 of 32Shell N: Electron 15 of 32Shell N: Electron 16 of 32Shell N: Electron 17 of 32Shell N: Electron 18 of 32Shell N: Electron 19 of 32Shell N: Electron 20 of 32Shell N: Electron 21 of 32Shell N: Electron 22 of 32Shell N: Electron 23 of 32Shell N: Electron 24 of 32Shell N: Electron 25 of 32Shell N: Electron 26 of 32Shell N: Electron 27 of 32Shell N: Electron 28 of 32Shell N: Electron 29 of 32Shell N: Electron 30 of 32Shell N: Electron 31 of 32Shell N: Electron 32 of 32OShell O: Electron 1 of 32Shell O: Electron 2 of 32Shell O: Electron 3 of 32Shell O: Electron 4 of 32Shell O: Electron 5 of 32Shell O: Electron 6 of 32Shell O: Electron 7 of 32Shell O: Electron 8 of 32Shell O: Electron 9 of 32Shell O: Electron 10 of 32Shell O: Electron 11 of 32Shell O: Electron 12 of 32Shell O: Electron 13 of 32Shell O: Electron 14 of 32Shell O: Electron 15 of 32Shell O: Electron 16 of 32Shell O: Electron 17 of 32Shell O: Electron 18 of 32Shell O: Electron 19 of 32Shell O: Electron 20 of 32Shell O: Electron 21 of 32Shell O: Electron 22 of 32Shell O: Electron 23 of 32Shell O: Electron 24 of 32Shell O: Electron 25 of 32Shell O: Electron 26 of 32Shell O: Electron 27 of 32Shell O: Electron 28 of 32Shell O: Electron 29 of 32Shell O: Electron 30 of 32Shell O: Electron 31 of 32Shell O: Electron 32 of 32PShell P: Electron 1 of 18Shell P: Electron 2 of 18Shell P: Electron 3 of 18Shell P: Electron 4 of 18Shell P: Electron 5 of 18Shell P: Electron 6 of 18Shell P: Electron 7 of 18Shell P: Electron 8 of 18Shell P: Electron 9 of 18Shell P: Electron 10 of 18Shell P: Electron 11 of 18Shell P: Electron 12 of 18Shell P: Electron 13 of 18Shell P: Electron 14 of 18Shell P: Electron 15 of 18Shell P: Electron 16 of 18Shell P: Electron 17 of 18Shell P: Electron 18 of 18QShell Q: Electron 1 of 7Shell Q: Electron 2 of 7Shell Q: Electron 3 of 7Shell Q: Electron 4 of 7Shell Q: Electron 5 of 7Shell Q: Electron 6 of 7Shell Q: Electron 7 of 7TsZ = 117

Educational Note: This Niels Bohr planetary model visually illustrates principal quantum energy shells ($n=1, 2, 3\dots$) and electron counts. In modern quantum mechanics (Schrödinger model), electrons do not orbit in fixed circular planetary tracks, but exist as 3D probability clouds (orbitals: $s, p, d, f$) governed by the Heisenberg uncertainty principle.

Electron Shell Filling Breakdown

Shell K (n=1):2 / 2 electrons (100%)
Shell L (n=2):8 / 8 electrons (100%)
Shell M (n=3):18 / 18 electrons (100%)
Shell N (n=4):32 / 32 electrons (100%)
Shell O (n=5):32 / 50 electrons (64%)
Shell P (n=6):18 / 72 electrons (25%)
Shell Q (n=7):7 / 98 electrons (7%)
Aufbau Electron Configuration
1s² 2s² 2p⁶ 3s² 3p⁶ 3d¹⁰ 4s² 4p⁶ 4d¹⁰ 4f¹⁴ 5s² 5p⁶ 5d¹⁰ 5f¹⁴ 6s² 6p⁶ 6d¹⁰ 7s² 7p⁵

Neutral ground state configuration. Valence electrons: 7.

Atomic & Quantum Properties

Electronegativity (Pauling)Not available
1st Ionization Energy742.9 kJ/mol
Electron Affinity-165.9 kJ/mol
Atomic Radius (empirical)138 pm
Common Oxidation States+1, +3
Crystal StructureUnknown

Physical & Thermal Properties

Density at STP7.2 g/cm³ (predicted)
Melting Point450 °C (723 K)
Boiling Point610 °C (883 K)
Magnetic OrderingParamagnetic
Discovery Year2010
Discovered ByJoint Institute for Nuclear Research (Dubna), Lawrence Livermore & Oak Ridge National Lab

Real-World Uses, Occurrence & Compounds

Major Industrial & Everyday Uses
  • Frontier scientific research into relativistic spin-orbit coupling in superheavy halogens
Occurrence in Nature

Synthesized in accelerators by bombarding Berkelium-249 targets with Calcium-48 projectile ions.

Etymology & Name Origin

Named in honor of the US State of Tennessee, home to Oak Ridge National Laboratory and Vanderbilt University

Important Chemical Compounds
None (single atoms produced)
Interesting Chemical Facts
  • The synthesis of Tennessine required 22 milligrams of rare Berkelium-249 produced over an entire year at the Oak Ridge reactor in Tennessee.
  • Unlike light halogens (F, Cl, Br, I), Tennessine is predicted to be a dark metallic or metalloid solid rather than a diatomic nonmetal.
  • The longest-lived isotope, Tennessine-294, has a half-life of 78 milliseconds.
Safety & Handling Note

Highly radioactive; produced only on a single-atom basis.