Seaborgium

Category: Transition metal

Atomic Number: 106

Period: 7 | Group: 6

Block: d-block

106
Sg
271.000

Description

Named for Glenn Seaborg while he was still alive — a first for the periodic table.

Physical Properties

Property Value
Phase at STP Solid
Density N/A
Melting Point N/A
Boiling Point N/A
Heat Capacity N/A

Atomic Properties

Property Value
Atomic Mass 271.0000 u
Electronegativity (Pauling) N/A
Oxidation States +6
Electron Configuration

Discovery & History

Discovered By Unknown
Discovery Year 1974
Named After Glenn T. Seaborg

Berkeley Laboratory Achievement (1974)

Seaborgium was discovered in June 1974 by Albert Ghiorso, J. M. Nitschke, José R. Alonso, Carol T. Alonso, M. Nurmia, G. T. Seaborg, and others at the Lawrence Berkeley National Laboratory. This discovery continued the American leadership in superheavy element synthesis during the Cold War era.

SuperHILAC Accelerator Success

The team used Berkeley's Super Heavy Ion Linear Accelerator (SuperHILAC) to bombard californium-249 targets with oxygen-18 ions, producing seaborgium-263, whose half-life they measured as 0.9 seconds (current evaluations give about 1.0 second). This represented a major breakthrough in superheavy element synthesis techniques.

Honoring Glenn T. Seaborg

The element was named "seaborgium" after Glenn T. Seaborg (1912-1999), Nobel Prize-winning chemist who discovered ten transuranium elements and transformed nuclear chemistry. Remarkably, Seaborg was still alive when the element was named, making it the first element named after a living person.

International Controversy and Resolution

Soviet scientists at Dubna contested the discovery priority, leading to another Cold War naming dispute . IUPAC initially rejected "seaborgium" in 1994 but reversed this decision, adopting the name in 1997; the Transfermium Working Group's 1993 report had credited Berkeley with the discovery.

Modern Confirmation (2025)

The 2025 discovery of seaborgium-257 by international collaboration using the TASCA separator at GSI represents the latest advancement in seaborgium research, demonstrating continued progress in superheavy element physics with 22 observed decay events providing detailed nuclear data.

Isotopes

ISOTOPE Neutrons Natural Abundance Half-life Decay Mode
Sg-263 157 - 1.0 sec α (70%), SF (30%)
Sg-265 159 - 14.4 sec SF (50%), α (50%)
Sg-267 161 - 84 sec SF (83%), α (17%)
Sg-269 163 - 130 sec α, SF
Sg-271 165 - 96 sec α (50%), SF (50%)

Data: IAEA Nuclear Data Section, LiveChart of Nuclides, ground-state evaluations, retrieved October 10, 2026. Abundance is the share of atoms in the natural element; a dash means the isotope has no standard natural abundance.

Applications & Uses

Group 6 Chemistry Validation

Seaborgium serves as the crucial test case for understanding Group 6 chemical behavior in superheavy elements, helping scientists determine how chromium, molybdenum, and tungsten chemical properties extend into the superheavy region under strongly relativistic conditions.

Nuclear Structure Research

Scientists use seaborgium to investigate nuclear shell effects and stability patterns in superheavy nuclei. The recent 2025 discovery of seaborgium-257 provides new insights into fission properties and shell effects that influence superheavy element behavior.

Relativistic Chemistry Investigation

Seaborgium enables new studies of relativistic effects in chemical bonding where electron orbital shapes and energies are dramatically altered by very high nuclear charge. These studies validate theoretical predictions about superheavy element chemistry.

Nuclear Decay Process Analysis

Research teams employ seaborgium to study complex decay chains including alpha decay sequences, spontaneous fission, and K-isomeric states. Recent discoveries of K-isomeric states in seaborgium-259 open new avenues for exploring nuclear structure phenomena.

Advanced Detection System Development

Seaborgium research drives innovation in ultra-sensitive analytical techniques including gas-filled separators like TASCA, advanced particle detection arrays, and sophisticated data analysis methods for identifying individual superheavy atoms.

Abundance

Earth's Crust N/A
Universe N/A