Lawrencium

Category: Actinide

Atomic Number: 103

Period: 7 | Group: N/A

Block: f-block

103
Lr
262.000

Description

The last actinide, with an electron configuration that broke the expected pattern.

Physical Properties

Property Value
Phase at STP Solid
Density N/A
Melting Point 1900.00 K (1626.85 °C)
Boiling Point N/A
Heat Capacity N/A

Atomic Properties

Property Value
Atomic Mass 262.0000 u
Electronegativity (Pauling) N/A
Oxidation States +3
Electron Configuration

Discovery & History

Discovered By Unknown
Discovery Year 1961
Named After Ernest Lawrence

Berkeley Laboratory Achievement (1961)

Lawrencium was discovered in 1961 by Albert Ghiorso, Torbjørn Sikkeland, Almon E. Larsh, and Robert M. Latimer at the Lawrence Radiation Laboratory, Berkeley, using the Heavy Ion Linear Accelerator (HILAC). This discovery marked the completion of the actinide series and opened the door to superheavy element research.

HILAC Breakthrough Technology

The team used Berkeley's important Heavy Ion Linear Accelerator to bombard californium-252 targets with boron-10 and boron-11 ions. The resulting lawrencium-258 nuclei were detected using innovative recoil techniques and solid-state detectors, representing advanced nuclear physics technology.

Recoil Detection Innovation

The discovery employed pioneering "recoil technique" where lawrencium atoms were deposited onto metallized Mylar tape and moved past series of detectors to measure their characteristic alpha decay. This method became standard for superheavy element identification.

Honoring Ernest Lawrence

The element was named "lawrencium" after Ernest Orlando Lawrence (1901-1958), inventor of the cyclotron and founder of Berkeley Lab. This naming honored American contributions to nuclear physics during the intense Cold War competition in element discovery.

Gateway to Superheavy Elements

As the final actinide element, lawrencium's discovery marked a crucial milestone in nuclear science, providing the foundation for superheavy element research that continues today. It represented the end of one era and the beginning of exploration into uncharted nuclear territory.

Isotopes

ISOTOPE Neutrons Natural Abundance Half-life Decay Mode
Lr-260 157 - 180 sec α, ε
Lr-261 158 - 39 min SF
Lr-262 159 - ~4 hr SF
Lr-264 161 - 4.9 hr SF
Lr-266 163 - ~11 hr 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

Actinide Series Boundary Research

Lawrencium serves as the crucial final actinide element , marking the transition point where f-orbital filling ends and d-orbital filling begins in the superheavy element region. This makes it invaluable for understanding electron configuration patterns and chemical periodicity beyond traditional elements.

Relativistic Chemistry Studies

Scientists use lawrencium to investigate relativistic effects in superheavy atoms, where electron velocities approach significant fractions of light speed. These studies validate quantum mechanical predictions about how chemical properties change under very high nuclear charge conditions.

Chemical Property Investigation

Research teams employ lawrencium in pioneering single-atom chemistry experiments to determine oxidation states, ionic radii, and chemical bonding behavior. These studies help predict properties of even heavier superheavy elements and validate theoretical chemical models.

Nuclear Shell Structure Analysis

Lawrencium isotopes provide critical data for understanding nuclear magic numbers and shell effects that govern superheavy element stability. This research guides predictions about the theorized "island of stability" and optimal pathways for synthesizing elements 104 and beyond.

Advanced Synthesis Technique Development

Studies of lawrencium drive innovation in superheavy element production methods , including hot fusion reactions, target preparation techniques, and separation chemistry that enables isolation and study of individual atoms in extremely small quantities.

Abundance

Earth's Crust N/A
Universe N/A