Your master tool to knowledges and calculations. related to isotopes.
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This module introduces the structure of coordination complexes, including ligand types, denticity, coordination number, geometry, and systematic IUPAC naming.
The geometry of coordination complexes depends primarily on the coordination number. The most common geometries are summarized below.
| Coordination Number | Geometry | Example |
|---|---|---|
| 2 |
Linear
|
[Ag(NH₃)₂]⁺ |
| 4 |
Tetrahedral
|
[NiCl₄]²⁻ |
| 4 |
Square Planar
|
[PtCl₄]²⁻ |
| 5 |
Trigonal Bipyramidal
|
Fe(CO)₅ |
| 5 |
Square Pyramidal
|
[CuCl₅]³⁻ |
| 6 |
Octahedral
|
[Co(NH₃)₆]³⁺ |
Ligands differ in denticity, donor atoms, and ligand field strength. Explore common ligands used in coordination chemistry.
This module explores the electronic structure of transition-metal complexes and uses Valence Bond Theory and Crystal Field Theory to predict hybridization, spin state, and magnetic behavior.
Determine the electron configuration of a transition metal and its cation, then find the resulting d-electron count and magnetic behavior.
Predict hybridization, geometry, inner-orbital vs outer-orbital character, and magnetic behavior of coordination complexes using Valence Bond Theory.
Explore d-orbital splitting, electron configuration, spin state, magnetic behavior, CFSE, and Jahn–Teller tendencies of coordination complexes using Crystal Field Theory.
This module explores how different ligand arrangements around a metal center produce geometric and optical isomers and influence observable properties such as color.
Generate common geometric isomers of coordination complexes, including cis/trans and fac/mer arrangements.
Detect common cases of optical activity in coordination compounds and visualize enantiomeric pairs.
Estimate crystal field splitting (Δ₀), predict absorbed wavelength, and determine the observed color of a coordination complex.
Ligand field strength:
Crystal field splitting (Δ₀): cm⁻¹
Absorbed wavelength: nm
Absorbed color:
Observed color:
Crystal field splitting energy is related to photon energy:
Δ₀ = hν
ν = c / λ
Therefore:
Δ₀ = hc / λ
Solving for wavelength:
λ = hc / Δ₀
Using spectroscopic units:
λ (nm) = 10⁷ / Δ₀ (cm⁻¹)