Nobelium

Category: Actinide

Atomic Number: 102

Period: 7 | Group: N/A

Block: f-block

102
No
259.000

Description

The subject of a decade-long discovery dispute between Swedish, American and Soviet teams.

Physical Properties

Property Value
Phase at STP Solid
Density N/A
Melting Point 1100.00 K (826.85 °C)
Boiling Point N/A
Heat Capacity N/A

Atomic Properties

Property Value
Atomic Mass 259.0000 u
Electronegativity (Pauling) N/A
Oxidation States +2, +3
Electron Configuration

Discovery & History

Discovered By Unknown
Discovery Year 1958
Named After Alfred Nobel

International Discovery Controversy (1957-1966)

Nobelium's discovery became one of the most contentious disputes in Cold War science. The first claim came from the Nobel Institute in Stockholm, Sweden in 1957, followed by competing claims from Soviet scientists at Dubna and American researchers at Berkeley, creating a decade-long priority battle.

Swedish Initial Claim

In 1957, Swedish physicists at the Nobel Institute announced element 102's discovery, bombarding curium-244 with carbon-13 ions . They proposed the name "nobelium" in honor of Alfred Nobel. However, other laboratories couldn't reproduce their results, and the Swedish team eventually retracted their claims.

Soviet Union Success

The definitive synthesis was achieved in 1966 by Georgy Flerov's team at the Joint Institute for Nuclear Research in Dubna, Soviet Union. They successfully created nobelium-256 by bombarding uranium-238 with neon-22 ions, providing conclusive evidence of element 102's existence.

IUPAC Resolution (1992)

The International Union of Pure and Applied Chemistry finally resolved the controversy in 1992, crediting the Soviet team with the official discovery. However, the name "nobelium" was retained due to its widespread use in scientific literature, creating an unusual situation where the namers weren't the discoverers.

Cold War Science Diplomacy

The nobelium controversy reflected broader Cold War tensions in science, with national pride and political prestige tied to element discoveries. The eventual resolution demonstrated international scientific cooperation's ability to overcome political divisions in pursuit of truth.

Isotopes

ISOTOPE Neutrons Natural Abundance Half-life Decay Mode
No-253 151 - 1.62 min α (55%), ε/β⁺ (45%)
No-254 152 - 51.2 sec α (90%), ε (10%)
No-255 153 - 3.52 min ε/β⁺ (70%), α (30%)
No-257 155 - 24.5 sec α, ε, SF
No-259 157 - 58 min α, ε/β⁺, SF

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

Nuclear Chemistry Research

Nobelium plays a critical role in understanding superheavy element chemistry , particularly investigating how electron orbitals behave under very high nuclear charge conditions. Scientists study nobelium to validate relativistic effects predictions in heavy atoms and explore chemical bonding beyond traditional periodic trends.

Actinide Series Boundary Studies

Research teams use nobelium to investigate the end of the actinide series and transition to superheavy elements. This research helps define where f-orbital filling ends and provides insights into electron configuration patterns that influence chemical properties of elements 103 and beyond.

Nuclear Decay Process Investigation

Nobelium isotopes serve as excellent subjects for studying spontaneous fission and alpha decay chains, providing data crucial for understanding nuclear stability limits and predicting properties of undiscovered superheavy elements in the theoretical "island of stability."

Theoretical Model Testing

Physicists employ nobelium in experiments that test quantum mechanical calculations for superheavy atoms, validating theoretical predictions about nuclear shell effects, binding energies, and optimal synthesis pathways for creating even heavier elements.

Advanced Detection Technology

Nobelium research drives development of ultra-sensitive analytical techniques including single-atom chemistry methods, advanced mass spectrometry, and sophisticated radiation detection systems that push the boundaries of what's possible in nuclear science.

Abundance

Earth's Crust N/A
Universe N/A