Beer-Lambert Law Calculator

Solve A = εlc for any variable in UV-Vis spectrophotometry.

Science 5 modes T ↔ A UV-Vis ready
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Beer-Lambert law

A = ε · l · c · 5 modes · transmittance converter

Instructions — Beer-Lambert Law Calculator

1

Pick what to solve

Five modes: Absorbance, Concentration, Extinction coefficient ε, Path length l, and Transmittance to Absorbance. The last mode is for converting raw % transmittance into A.

2

Enter your values

ε in L·mol⁻¹·cm⁻¹, path length in cm (standard cuvette is 1.0 cm), concentration in mol/L. The default ε of 15,000 is typical for a strongly absorbing organic chromophore.

3

Check the optimal range

Beer-Lambert is most accurate when A is between 0.1 and 1.0. Above A = 2 the photometer is near its detection limit and the linearity breaks. Dilute samples that read above 2.0.

Formulas

Beer-Lambert law
$$ A = \varepsilon \cdot l \cdot c $$
Absorbance equals molar extinction coefficient times path length times concentration. The foundation of UV-Vis quantitative analysis.
Transmittance to absorbance
$$ A = -\log_{10}(T) = \log_{10}\frac{1}{T} $$
When 10% of light passes through (T = 0.1), absorbance equals 1.0. When 1% passes (T = 0.01), absorbance equals 2.0.
Solving for concentration
$$ c = \frac{A}{\varepsilon \cdot l} $$
Once a calibration curve gives you ε, any unknown's concentration drops out of a single absorbance reading.

Reference

Typical molar extinction coefficients
Chromophoreλ_max (nm)ε (L·mol⁻¹·cm⁻¹)
Tryptophan (protein)280~5,500
NADH3406,220
Hemoglobin (oxy)415~125,000
β-Carotene450140,000
DNA (per base)260~13,200
Permanganate (MnO₄⁻)525~2,500

Article — Beer-Lambert Law Calculator

Beer-Lambert law calculator: solve A = εlc for any variable

The Beer-Lambert law, A = ε · l · c, links the absorbance of a solution to its concentration, the path length of the cuvette, and a substance-specific molar extinction coefficient. It is the foundation of UV-visible spectrophotometry and the basis for nearly every quantitative photometric assay. Absorbance is dimensionless, ε has units of L·mol⁻¹·cm⁻¹, l is in centimetres, and c is in moles per litre.

This calculator solves the Beer-Lambert law in five directions. Compute absorbance from ε, l, and c. Back-calculate any of the three from absorbance. Convert percent transmittance into absorbance directly. The optimal absorbance range for accurate measurement is 0.1 to 1.0 — above 2.0, the photometer is at the edge of its detection limit and the linearity breaks.

What is the Beer-Lambert law?

The Beer-Lambert law (also called the Beer-Bouguer-Lambert law) states that the absorbance A of a homogeneous solution is proportional to the molar extinction coefficient ε, the path length l of the light through the sample, and the concentration c of the absorbing species. The law combines two earlier observations: Lambert (1760) on path length and Beer (1852) on concentration.

Every UV-Vis spectrophotometer in a chemistry lab operates on this principle. The instrument shines monochromatic light through a sample, measures how much exits the cuvette, and reports the absorbance. With ε and l known, concentration drops out of a single reading.

The Beer-Lambert formula in detail

The standard form expresses absorbance as a triple product:

Beer-Lambert formulas
A = ε · l · c
A = −log₁₀(T) = log₁₀(1/T)
T = 10^(−A)

ε is the molar extinction coefficient in L·mol⁻¹·cm⁻¹ — a property of the chemical at a specific wavelength. l is path length in cm; standard cuvettes are 1.0 cm. c is concentration in mol/L. Multiply, and you get a dimensionless absorbance value.

Beer-Lambert absorbance and transmittance

Transmittance T is the fraction of incident light that passes through the sample, ranging from 0 (opaque) to 1 (clear). Absorbance is its negative base-10 logarithm: A = −log₁₀(T). When T = 0.1 (10% passes), A = 1.0. When T = 0.01 (1% passes), A = 2.0. The logarithmic scaling makes absorbance linearly proportional to concentration, while transmittance falls off exponentially.

Did you know

The first practical UV-Vis spectrophotometer, the Beckman DU, hit the market in 1941 and cost $723 — roughly $16,000 in 2024 dollars. It used a quartz prism, a phototube detector, and a hand-cranked wavelength selector. The Beer-Lambert measurements that today take seconds once took several minutes per wavelength.

The molar extinction coefficient (ε)

The molar extinction coefficient, also called the molar absorptivity, quantifies how strongly a substance absorbs at a given wavelength. Values range from below 100 (weak n→π* transitions) to over 100,000 (strongly allowed π→π* transitions in extended chromophores).

ε is a property of the chromophore and the wavelength only — not of concentration or path length. Tabulated values exist for most biological cofactors and common dyes. For unfamiliar compounds, ε is measured by preparing a known concentration and reading the absorbance.

Beer-Lambert calibration curves

For routine quantitation, analysts build a calibration curve. Prepare 5–7 standards spanning the expected concentration range. Measure each at the absorbance maximum (λ_max) in the same cuvette. Plot A versus c — the line should pass through the origin with slope equal to ε × l. Unknowns are read off the curve.

Tip

Aim for absorbance values between 0.1 and 1.0 on every standard. Below 0.1 the signal-to-noise ratio is poor; above 1.0 stray light starts to compress the apparent absorbance. Adjust path length (longer cuvette for dilute samples, shorter for concentrated) before adjusting dilutions.

Beer-Lambert applications in analysis

Protein concentration via A280 (tryptophan absorption at 280 nm with ε ≈ 5,500 L·mol⁻¹·cm⁻¹ per tryptophan). Nucleic acid concentration via A260 (DNA, RNA). NADH/NAD+ assays for enzyme activity. Hemoglobin oxygen saturation in pulse oximetry. Vitamin assays in food analysis. Chlorine concentration in pool water testing. Pharmaceutical content assays.

Hemoglobin
125,000
L·mol⁻¹·cm⁻¹ at 415 nm
DNA (per base)
13,200
L·mol⁻¹·cm⁻¹ at 260 nm

Where the Beer-Lambert law breaks down

The Beer-Lambert law assumes monochromatic light, dilute solutions, and non-interacting absorbers. At high concentrations (typically above 10 mM), molecules begin to interact: refractive index changes, aggregates form, and the assumption of independent chromophores fails. Stray light in the spectrophotometer compresses the apparent absorbance at very high A values.

Polychromatic light bands cause non-linearity because ε varies across the band. Wavelength inaccuracy in the monochromator gives the same effect. Fluorescent samples can return more light than entered, distorting the absorbance reading. For all these reasons, absorbance above 2.0 is rarely trustworthy without specialized instruments.

Common Beer-Lambert pitfalls

Four errors repeat in undergraduate labs. First, neglecting the blank — every measurement needs a reference cuvette containing the solvent. Second, dirty cuvette walls — fingerprints absorb in the UV. Third, bubbles in the optical path — these scatter light and inflate the reading. Fourth, wavelength selection — measure at λ_max, not at an arbitrary wavelength.

Beer-Lambert assumes monochromatic light

If your instrument has a wide bandpass (cheap photometers often have 10 nm or more) and the chromophore's absorption peak is sharp, the apparent ε will be lower than the literature value. Always cite the wavelength and bandwidth alongside any ε you report.

  • Tryptophan at 280 nm — ε ≈ 5,500 L·mol⁻¹·cm⁻¹
  • NADH at 340 nm — ε = 6,220 L·mol⁻¹·cm⁻¹
  • β-carotene at 450 nm — ε ≈ 140,000 L·mol⁻¹·cm⁻¹
  • Permanganate at 525 nm — ε ≈ 2,500 L·mol⁻¹·cm⁻¹
  • Chlorophyll a at 663 nm — ε ≈ 86,300 L·mol⁻¹·cm⁻¹
  • Standard cuvette — 1.0 cm path length

The Beer-Lambert law is a model — like every model, it has a domain of validity. Used inside that domain (dilute solutions, low absorbance, monochromatic light), it is one of the most reliable equations in analytical chemistry. The calculator handles the algebra; the calibration discipline and the sample preparation stay with the analyst.

Microvolume spectrophotometers (NanoDrop and similar) use very short path lengths — typically 1 mm or even 0.05 mm — to extend Beer-Lambert measurements into concentration ranges where a 1 cm cuvette would saturate. A DNA sample at 50 ng/μL in a 1 mm path reads A260 = 1.0, the same value as 5 ng/μL in a 1 cm cuvette. The math is identical; the geometry just shifts the working range.

Diode-array spectrophotometers measure absorbance at every wavelength simultaneously, returning a full spectrum in fractions of a second. This enables real-time monitoring of reactions, chromatography detection, and rapid spectral identification. The Beer-Lambert law still applies wavelength-by-wavelength; the only change is that you read out hundreds of A values at once.

Reflectance spectroscopy applies a Beer-Lambert analog to opaque samples. Diffuse reflectance measurements of powders and surfaces follow the Kubelka-Munk function instead, which is conceptually similar but accounts for scattering. For most aqueous solution work, however, the standard A = εlc form is exactly what you need — and the calculator covers every solve-for direction in one place.

FAQ

The Beer-Lambert law states that absorbance A is proportional to the molar extinction coefficient ε, the path length l, and the concentration c: A = εlc. It is the workhorse of UV-Vis spectrophotometry and the basis for nearly every quantitative photometric assay.
ε measures how strongly a substance absorbs light at a given wavelength, in L·mol⁻¹·cm⁻¹. A value of 10,000 means a 1 M solution in a 1 cm cuvette has absorbance 10,000 — usually impossible to read directly, so analytical work is done at far lower concentrations.
Transmittance T is the fraction of incident light that passes through the sample (0 to 1, or 0 to 100%). Absorbance is the negative log of T: A = −log₁₀(T). T = 0.1 (10% passes) corresponds to A = 1.0.
0.1 to 1.0 absorbance units. Below 0.1 the signal is too close to noise; above 2.0 the photometer is near its detection limit and Beer-Lambert deviations creep in. Dilute samples that read outside this window for the best precision.
Above roughly 0.01 M, molecules interact (forming aggregates or excimers), refractive index changes, and the assumption of independent absorbers fails. Stray light in the spectrophotometer also flattens the apparent curve. Dilute below 10 mM for accurate work.
Prepare 5–7 standards spanning the expected concentration range. Measure each at λ_max in the same cuvette. Plot A vs c and fit a straight line forced through (0, 0). The slope equals ε × l, and you read unknowns off the curve.
Path length l is the distance light travels through the sample, set by the cuvette geometry. Standard cuvettes are 1.0 cm. Microvolume systems (NanoDrop) use 1 mm or shorter paths to enable high-concentration measurements without dilution.
Yes, additively: total A at any wavelength is the sum of εᵢlcᵢ for each absorber. For two components, measure A at two wavelengths and solve the linear system. Spectral deconvolution extends this to many components but needs matrix algebra.