Category: Actinide
Atomic Number: 103
Period: 7 | Group: N/A
Block: f-block
The last actinide, with an electron configuration that broke the expected pattern.
| 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 |
| Property | Value |
|---|---|
| Atomic Mass | 262.0000 u |
| Electronegativity (Pauling) | N/A |
| Oxidation States | +3 |
| Electron Configuration |
| 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.
| 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.
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.
| Earth's Crust | N/A |
|---|---|
| Universe | N/A |