Element 113 (Nihonium): The Complete Guide

Element 113 is Nihonium (Nh), a synthetic superheavy element first synthesized in 2004 by Japanese scientists. This extremely rare element has atomic number 113, belongs to Group 13 of the periodic table, and was officially recognized in 2016. With its most stable isotope having a half-life of just seconds, Nihonium does not exist naturally and can only be produced in specialized particle accelerators. As the first element discovered in Asia, its name honors Japan ("Nihon" in Japanese).

Element 113: Basic Information and Position in the Periodic Table

Nihonium stands as one of the newest officially recognized elements in the periodic table, representing a significant achievement in nuclear physics and chemistry. Understanding its place in the periodic system provides context for its properties and significance.

Fundamental Properties of Nihonium

Element 113, Nihonium (Nh), possesses the following basic characteristics:

Property Value Notes
Atomic Number 113 Number of protons in nucleus
Element Symbol Nh Officially adopted in 2016
Element Category Post-transition metal Member of the p-block
Group Group 13 (IIIA) Boron group
Period Period 7 Seventh row of periodic table
Electronic Configuration [Rn] 5f¹⁴ 6d¹⁰ 7s² 7p¹ Theoretical configuration
Most Stable Isotope Nihonium-286 Half-life of approximately 10 seconds
Natural Occurrence Synthetic only Does not occur in nature

As a member of Group 13 (the Boron group), Nihonium follows the elements Boron (B), Aluminum (Al), Gallium (Ga), Indium (In), and Thallium (Tl). This placement suggests certain chemical properties, though these remain largely theoretical due to the element's extreme rarity and instability.

Position in the Periodic Table

Nihonium occupies a significant position in the modern periodic table:

  • Periodic table region: Located in the p-block of elements
  • Classification: Considered a post-transition metal, though its chemistry remains largely theoretical
  • Neighboring elements:
    • Element 112: Copernicium (Cn)
    • Element 114: Flerovium (Fl)
    • Element 112 is a transition metal, while Element 114 is classified as a post-transition metal
  • Transactinide series: Part of the transactinide elements (elements with atomic numbers 104-120)
  • Superheavy element status: Among the superheavy elements, defined as having atomic numbers greater than 104

Nihonium's position makes it scientifically significant as it helps complete the seventh row of the periodic table and provides insights into how relativistic effects influence chemical properties in superheavy elements.

Nomenclature History

The journey to naming Element 113 reflects the international nature of scientific discovery and recognition:

  1. Temporary systematic name: Ununtrium (Uut)
    • Based on IUPAC systematic element naming
    • From Latin roots for "one-one-three"
    • Used from 2004-2016 during verification period
  2. Name proposal process:
    • The RIKEN team was granted naming rights after being credited with discovery
    • They proposed "nihonium" in honor of Japan (Nihon)
    • This marked the first element to be named by Asian scientists
  3. Official naming:
    • IUPAC officially approved the name "nihonium" and symbol "Nh" in November 2016
    • The name follows IUPAC's tradition of elements being named after mythological concepts, minerals, places or countries, properties, or scientists

The name "nihonium" holds cultural significance as it recognizes Japanese contributions to chemistry and nuclear physics, broadening the geographical representation of element names beyond Europe and the Americas.

Discovery and Synthesis of Element 113

The discovery of Nihonium represents one of the most challenging scientific achievements in nuclear physics, requiring advanced technology, meticulous experimental design, and years of verification.

The Path to Discovery

The road to officially recognizing Element 113 involved multiple research groups and several milestone experiments:

Date Research Team Achievement
1998-2003 Joint Institute for Nuclear Research (Russia) and Lawrence Livermore National Laboratory (USA) Claimed indirect evidence of Element 113 through decay chains of Elements 115 and 117
July 23, 2004 RIKEN (Japan) - Morita's team First direct synthesis - observed a single atom of Element 113
April 2, 2005 RIKEN (Japan) - Morita's team Second successful synthesis event
August 12, 2012 RIKEN (Japan) - Morita's team Third confirmed synthesis, providing decisive evidence
December 31, 2015 IUPAC Official recognition of discovery, credit given to RIKEN team
November 28, 2016 IUPAC Formal approval of the name "nihonium" and symbol "Nh"

The RIKEN team, led by Kosuke Morita, ultimately received credit for the discovery after producing the most convincing evidence through direct synthesis methods.

Synthesis Methodology

Creating Element 113 requires extremely sophisticated equipment and precise experimental conditions:

RIKEN's Cold Fusion Approach

  • Target material: Bismuth-209 (²⁰⁹Bi)
  • Projectile: Zinc-70 ions (⁷⁰Zn)
  • Acceleration: Linear accelerator at approximately 10% of light speed
  • Nuclear reaction: ²⁰⁹Bi + ⁷⁰Zn → ²⁷⁸Nh + 1 neutron
  • Success rate: Approximately one successful event per 1.5×10¹⁹ zinc ions (extremely rare)

Russian-American Hot Fusion Approach

  • Indirect method: Creating heavier elements that decay to Element 113
  • Target material: Americium-243 (²⁴³Am)
  • Projectile: Calcium-48 ions (⁴⁸Ca)
  • Intermediate product: Element 115 (moscovium)
  • Decay process: Element 115 → Element 113 + alpha particle

The RIKEN team's use of the cold fusion approach with zinc and bismuth was particularly noteworthy as it represented a more direct synthesis method, though it required overcoming extremely low probability of successful nuclear fusion.

Detection and Confirmation Challenges

Identifying and confirming the creation of Element 113 presented enormous technical challenges:

  • Incredibly rare events: Only a few atoms ever created, with production rates measured in atoms per week or month
  • Extremely short half-lives: The element decays within seconds, requiring rapid detection systems
  • Signature identification: Scientists tracked characteristic alpha decay chains to confirm element identity
    • Alpha decay: Element 113 emits helium nuclei (alpha particles) as it transforms into lighter elements
    • Decay chain: Nihonium-278 → Roentgenium-274 → Meitnerium-270 → Bohrium-266
    • Each step in this decay chain has a specific energy signature that can be detected
  • Detection apparatus:
    • Gas-filled detectors to track alpha particles
    • Silicon detectors to measure decay energy with precision
    • Time-of-flight detectors to confirm mass
  • Reproducibility challenges: The extreme rarity of successful synthesis events made reproduction particularly difficult

The RIKEN team's achievement is particularly remarkable given these challenges, requiring patience through years of experiments to gather sufficient evidence for recognition.

Research Limitations and Practical Challenges

Working with Element 113 involves significant limitations:

  • Atom-at-a-time chemistry: Only single atoms are produced, making traditional chemical analysis impossible
  • Extreme resource requirements: Production requires specialized particle accelerators found in only a few facilities worldwide
  • Energy costs: Substantial energy input needed for minimal yield
  • Time constraints: The short half-life severely limits experimental possibilities
  • Verification complexity: Statistical significance requires multiple observation events, sometimes taking years to accumulate

Properties and Characteristics of Nihonium

Given the extreme scarcity and instability of Nihonium, most of our understanding of its properties comes from theoretical predictions rather than direct experimental measurements. These predictions are based on periodic trends, quantum mechanical calculations, and relativistic effects.

Physical Properties

The physical properties of Nihonium, while largely theoretical, can be estimated based on its position in the periodic table and computational models:

Property Predicted Value Basis of Prediction
Physical State (at STP) Likely solid Based on Group 13 trends
Appearance Likely metallic, silvery Similar to other heavy metals
Density 16-18 g/cm³ Computational models
Melting Point ~700°C Theoretical calculations
Boiling Point ~1400°C Estimated from similar elements
Atomic Radius ~170 picometers Quantum mechanical models
Crystal Structure Likely face-centered cubic Based on Group 13 patterns

These properties are significantly influenced by relativistic effects, which become increasingly important for heavier elements. For Nihonium, these effects may cause unexpected deviations from expected periodic trends.

Chemical Properties and Behavior

The chemical nature of Nihonium must be inferred rather than directly observed, due to the impossibility of conventional chemical tests:

  • Predicted oxidation states:
    • Primary: +3 (similar to other Group 13 elements)
    • Possible: +1 (due to relativistic stabilization of the 7s orbital)
    • The +1 state may be more stable than expected due to the "inert pair effect," where the 7s² electrons are less likely to participate in bonding
  • Electronegativity: Estimated around 1.5-1.7 on the Pauling scale
  • Chemical reactivity:
    • Expected to be less reactive than thallium
    • Likely forms ionic compounds with highly electronegative elements
    • May form volatile compounds under certain conditions
  • Theoretical compounds:
    • Nihonium(III) oxide (Nh₂O₃)
    • Nihonium(III) halides (NhF₃, NhCl₃, etc.)
    • Nihonium(I) compounds (NhCl, NhBr, etc.)

Due to relativistic effects, the chemistry of nihonium might deviate significantly from what would be expected based on its position in Group 13. These effects could lead to unique chemical behaviors not seen in lighter members of the group.

Nuclear Properties and Isotopes

The nuclear properties of Nihonium are among its most studied characteristics, as they determine its stability and decay patterns:

Isotope Half-life Decay Mode Discovery/Synthesis
⁴⁸²Nh Microseconds Alpha decay Theoretical only
²⁸³Nh ~100 milliseconds Alpha decay Observed in decay chains
²⁸⁴Nh ~1 second Alpha decay Observed in decay chains
²⁸⁶Nh ~10 seconds Alpha decay Most stable known isotope
²⁸⁷Nh Unknown Likely alpha decay Theoretical only
²⁹⁰Nh Unknown Likely alpha decay Predicted to be more stable due to nuclear shell effects

The search for more stable isotopes of nihonium continues, with particular interest in those that might lie closer to the theorized "island of stability"—a region of the nuclide chart where superheavy elements might exhibit significantly longer half-lives due to nuclear shell effects.

Island of Stability Visualization

The concept of the "island of stability" is central to understanding superheavy elements like nihonium:

Current known elements are relatively stable up to uranium (element 92), after which stability rapidly decreases.

The "island of stability" is predicted to center around elements with:

  • Proton numbers around 108, 114, or 120 (potential "magic numbers")
  • Neutron numbers around 184 (a predicted "magic number")

Element 113 (Nihonium) sits near the edge of this theoretical island. More neutron-rich isotopes of nihonium (potentially ²⁹⁰Nh) might show greater stability if they could be synthesized.

Scientific Significance and Potential Applications

While nihonium has no current practical applications due to its extreme rarity and instability, its discovery and study hold significant scientific value and offer potential insights for future technological developments.

Fundamental Scientific Importance

Element 113 contributes to our understanding of several fundamental aspects of physics and chemistry:

  1. Testing quantum mechanical models:
    • Nihonium's properties help validate quantum theory predictions for superheavy elements
    • Its behavior provides insights into how electron orbitals are structured in extreme cases
    • Helps refine theoretical models used to predict properties of yet-undiscovered elements
  2. Relativistic effects in chemistry:
    • Elements with high atomic numbers experience significant relativistic effects due to electrons moving at substantial fractions of light speed
    • These effects can cause unexpected chemical behaviors that deviate from periodic trends
    • Nihonium helps scientists study how these effects influence electronic structure and chemical bonds
  3. Nuclear structure theory:
    • The synthesis and decay patterns of nihonium provide data to test and refine nuclear models
    • Helps validate predictions about nuclear stability and decay modes
    • Contributes to understanding the limits of the periodic table
  4. Island of stability research:
    • Nihonium's position near the predicted "island of stability" makes its study relevant to this important theoretical concept
    • May provide clues about how to synthesize more stable superheavy elements
    • Helps scientists refine predictions about where longer-lived superheavy elements might be found

These contributions to fundamental science represent the primary value of nihonium research, advancing our understanding of matter at its most extreme.

Current Research Directions

Contemporary research involving nihonium focuses on several key areas:

Synthesis Optimization

  • Goal: Improve production efficiency of nihonium atoms
  • Approaches:
    • Testing alternative target-projectile combinations
    • Refining accelerator beam characteristics
    • Enhancing detection sensitivity
  • Challenges: Extremely low production cross-sections, high energy requirements

New Isotope Discovery

  • Goal: Create and identify more stable isotopes of nihonium
  • Approaches:
    • Using neutron-rich projectiles or targets
    • Exploring reactions that might produce isotopes closer to the island of stability
    • Indirect synthesis through decay of heavier elements
  • Significance: Could provide isotopes with longer half-lives for further study

Chemical Property Investigations

  • Goal: Confirm theoretical predictions about nihonium's chemical behavior
  • Approaches:
    • Ultra-fast chemical separation techniques
    • Gas phase chemistry experiments
    • Advanced computational chemistry models
  • Limitations: Extremely short half-life, single-atom chemistry challenges

Decay Chain Analysis

  • Goal: Better understand decay pathways and daughter products
  • Approaches:
    • High-precision energy measurements
    • Improved timing resolution in detection
    • Cross-referencing with known decay patterns
  • Applications: Helps verify synthetic pathways and improves identification accuracy

Theoretical Future Applications

While current applications are limited to pure research, theoretical future applications might include:

  • Advanced nuclear physics:
    • If more stable isotopes are discovered, they could serve as stepping stones to create other superheavy elements
    • Might provide insights for nuclear fusion energy research
    • Could inform the development of new types of radiation detectors
  • Materials science:
    • Theoretical understanding of nihonium's electronic structure could inspire novel materials design
    • Relativistic effects observed in nihonium might inform the development of materials with unique electronic properties
  • Medical isotopes:
    • While nihonium itself is too unstable, techniques developed for its synthesis and study might be applied to creating medical isotopes
    • Decay chain products might have potential applications in targeted radiotherapy
  • Computing and electronics:
    • Theoretical insights from nihonium's electronic structure might inform quantum computing research
    • Understanding of relativistic electron behavior could influence future electronic material design

It's important to note that these applications remain highly speculative. The extreme difficulty of producing nihonium and its short half-life make practical applications unlikely in the foreseeable future. The element's primary value remains in fundamental research and the advancement of scientific knowledge.

Frequently Asked Questions About Element 113

Why was Element 113 named Nihonium?

Element 113 was named Nihonium (symbol Nh) to honor Japan, where it was first synthesized. "Nihon" is the Japanese word for Japan, literally meaning "land of the rising sun." The name was proposed by the RIKEN team led by Kosuke Morita who first created the element in 2004 and received official discovery credit in 2015. The naming holds historical significance as it represents the first element discovered in Asia and the first named after an Asian country. After the discovery was confirmed, IUPAC (International Union of Pure and Applied Chemistry) granted the Japanese team naming rights, and they chose to highlight their country's contribution to nuclear science. The "-ium" suffix follows the convention for metallic elements. The name was officially approved by IUPAC in November 2016, replacing the temporary systematic name "ununtrium" (Uut) that had been used during the verification period.

How does Element 113 compare to other Group 13 elements?

Element 113 (Nihonium) differs significantly from its Group 13 counterparts (Boron, Aluminum, Gallium, Indium, Thallium) in several ways. While lighter Group 13 elements are relatively stable and naturally occurring, nihonium is synthetic, extremely radioactive, and has a half-life of only seconds. In terms of properties, nihonium is predicted to be more metallic than its predecessors, with relativistic effects causing its chemistry to deviate from expected periodic trends. Unlike boron (a metalloid) and aluminum (a light metal), nihonium is expected to behave as a dense, heavy post-transition metal similar to thallium but with potentially greater stability of the +1 oxidation state due to relativistic effects. Its incredibly high atomic weight (286 for the most stable isotope) dramatically exceeds thallium (204.4), the next heaviest element in the group. While other Group 13 elements have practical applications in everyday life, nihonium exists only in research settings and has no practical uses due to its extreme rarity and instability.

How many atoms of Element 113 have ever been created?

The total number of Element 113 (Nihonium) atoms ever created is extremely small—confirmed reports indicate fewer than 10 atoms have been directly synthesized and positively identified since its discovery. The Japanese RIKEN team led by Kosuke Morita reported three definitive synthetic events: one in 2004, another in 2005, and a third in 2012. The Russian-American collaborations at Dubna and Lawrence Livermore have likely produced a few additional atoms through the decay of heavier elements. The extreme rarity stems from the incredibly low production cross-section for the nuclear fusion reaction, estimated at around one successful event per 10^19 (ten quintillion) zinc ions fired at the bismuth target. This makes nihonium synthesis one of the most resource-intensive processes in science, requiring weeks or months of accelerator time to produce a single atom. Even with recent improvements in synthesis techniques, the total global production remains in the single-digit range, making nihonium one of the rarest human-made substances in existence.

Could Element 113 ever exist naturally on Earth or elsewhere in the universe?

Element 113 (Nihonium) does not exist naturally on Earth and is extremely unlikely to exist naturally elsewhere in the universe under current cosmic conditions. With a half-life of only seconds for its most stable isotope, any nihonium formed during early stellar nucleosynthesis would have decayed billions of years ago. The extreme instability occurs because large nuclei face increasing electrostatic repulsion between protons, which overwhelms the strong nuclear force holding the nucleus together. Theoretical models suggest that tiny traces of superheavy elements might potentially form in extremely energetic cosmic events like neutron star mergers or supernovae, but would decay almost instantly. The only speculative natural source might be if a neutron star with extremely high density could create a "crust" containing superheavy elements through rapid neutron capture, but even this remains highly theoretical. Some scientists have proposed that within the theoretical "island of stability," undiscovered isotopes of superheavy elements might have half-lives of minutes, years, or potentially longer, but no evidence yet supports the natural existence of such isotopes.

What are the next steps in research related to Element 113?

Future research on Element 113 (Nihonium) will focus on several key directions. Scientists aim to create more neutron-rich isotopes that might be closer to the theoretical "island of stability," potentially offering longer half-lives for more extensive study. Researchers will work to improve production efficiency through optimized target-projectile combinations and accelerator techniques to increase the number of atoms available for analysis. Chemical studies will attempt to verify theoretical predictions about nihonium's electronic structure and chemical behavior, particularly how relativistic effects influence its properties. Advanced detection techniques are being developed to better capture the brief signals from nihonium atoms and their decay products. International collaborations between facilities in Japan, Russia, Germany, and the United States will continue exploring questions about superheavy element stability and characteristics. The broader goal remains to deepen our understanding of the limits of the periodic table and the fundamental physics that governs matter at these extremes, potentially opening pathways to discover elements 119, 120, and beyond.