Absorbance as a logarithmic measurement
Absorbance is unitless and logarithmic, so equal changes in A represent multiplicative changes in transmitted intensity. For example, A = 0.30 corresponds to T ≈ 50%, while A = 1.00 corresponds to T = 10%. This scaling is why spectrometers report absorbance for wide dynamic ranges.
Typical values used in laboratory optics
In UV–Vis work, practical absorbance often falls between 0.10 and 1.50. Below 0.05, noise and stray light can dominate; above about 2.0, very little light reaches the detector. Path lengths are commonly 1 cm cuvettes, but microcells can be 0.1–0.5 cm for concentrated samples.
Choosing path length for sensitivity
Sensitivity increases with path length because A = εlc. Doubling l doubles A at fixed ε and c. If your analyte is weakly absorbing (small ε), using a 5 cm or 10 cm cell can bring absorbance into a measurable range. For strongly absorbing dyes, shorter paths prevent saturation.
Molar absorptivity and wavelength dependence
Molar absorptivity ε depends on wavelength, temperature, and chemical environment. Many organic chromophores have ε from about 1×103 to 1×105 L·mol−1·cm−1 near absorption peaks. Reporting ε should include wavelength (nm) and solvent conditions for reproducibility.
Working with concentration units
This calculator supports mol/L, mmol/L, mol/m³, and g/L. A useful conversion is 1 mol/m³ = 0.001 mol/L. When using g/L, concentration in mol/L equals (g/L) divided by molar mass (g/mol). This is important for proteins, salts, and formulations specified by mass.
Base-10 absorbance versus optical depth
Some fields use the natural-log form I = I₀e−τ, where τ = ln(I₀/I). The two are equivalent through τ = ln(10)·A ≈ 2.3026A. Switching bases does not change the physics; it changes the numerical scale and how you interpret “one unit” of attenuation.
Measurement tips that improve linearity
Use a proper blank, keep cuvettes clean, and match the reference solvent. Stray light and detector limits can bias high-absorbance readings. Mix solutions thoroughly and allow temperature to equilibrate. If you are fitting a calibration curve, collect at least 5 standards spanning the expected concentration range.
When Beer–Lambert assumptions fail
Departures from linearity can occur at high concentration due to molecular interactions, scattering, fluorescence, or refractive-index changes. Turbid samples may require integrating spheres or scattering corrections. If A versus c deviates from a straight line, dilute the sample or choose a different wavelength where absorbance is lower.