Beer-Lambert Law Calculator

Calculate absorbance, transmittance, molar absorptivity, path length, or concentration using the Beer-Lambert Law. Enter any known values and solve for the unknown variable instantly.

A = ε × c × l Absorbance = Molar Absorptivity × Concentration × Path Length
I want to solve for:
unitless
Dimensionless, typically 0 - 3
%
Percentage of light transmitted (0-100%)
L·mol⁻¹·cm⁻¹
Also called molar extinction coefficient
Length of the cuvette / sample cell
Moles of solute per liter of solution

Calculation Results

Beer-Lambert Law Diagram

Light Source I₀ Concentration (c) l (path) I Detector A = -log₁₀(I/I₀) = ε × c × l

What Is the Beer-Lambert Law?

The Beer-Lambert Law, also known as Beer's Law, the Lambert-Beer Law, or the Beer-Lambert-Bouguer Law, is a fundamental relationship in analytical chemistry and spectroscopy. It describes how the absorption of light by a substance is directly proportional to the concentration of that substance and the path length of the light through the sample.

The law is named after three scientists who contributed to its formulation. Pierre Bouguer first observed in 1729 that light intensity decreases exponentially as it passes through an absorbing medium. Johann Heinrich Lambert mathematically expressed this relationship in 1760. Finally, August Beer extended the law in 1852 by showing that absorbance is also proportional to the concentration of the absorbing species in solution.

Today, the Beer-Lambert Law is one of the most widely used equations in chemistry. It forms the theoretical backbone of UV-Vis spectroscopy, colorimetry, and many quantitative analytical methods used in pharmaceutical analysis, environmental monitoring, clinical diagnostics, and food science.

The Beer-Lambert Law Equation Explained

The Beer-Lambert Law is expressed mathematically as:

A = ε × c × l

Where:

Symbol Quantity SI Unit
A Absorbance (optical density) Dimensionless (unitless)
ε Molar absorptivity (molar extinction coefficient) L · mol-1 · cm-1
c Molar concentration of the absorbing species mol/L (M)
l Path length of the sample cell (cuvette) cm

The equation tells us that absorbance is the product of three factors. A higher molar absorptivity means the substance absorbs light more efficiently at the chosen wavelength. A longer path length gives the light more distance to interact with the sample. A higher concentration means more absorbing molecules are present. All three factors increase absorbance proportionally.

What Is Absorbance and Transmittance?

Absorbance (A)

Absorbance is a dimensionless quantity that measures how much light is absorbed by a sample at a particular wavelength. It is defined as the negative base-10 logarithm of the transmittance:

A = -log10(T)   or equivalently   A = log10(I0 / I)

An absorbance of 0 means no light is absorbed (100% transmitted). An absorbance of 1 means 90% of light is absorbed (10% transmitted). An absorbance of 2 means 99% is absorbed (1% transmitted). In practice, reliable spectroscopic measurements are typically obtained for absorbance values between 0.1 and 1.0.

Transmittance (T)

Transmittance is the fraction of incident light that passes through the sample without being absorbed. It is defined as:

T = I / I0 = 10-A

Transmittance is often expressed as a percentage (%T). A sample with 100% transmittance absorbs no light, while a sample with 0% transmittance absorbs all the light. The relationship between absorbance and transmittance is logarithmic, not linear, meaning that equal changes in absorbance correspond to multiplicative changes in transmittance.

What Is Molar Absorptivity?

Molar absorptivity (ε), also called the molar extinction coefficient, is an intrinsic property of a chemical substance that quantifies how strongly it absorbs light at a given wavelength. It has units of L · mol-1 · cm-1.

The value of ε depends on the wavelength of light used, the nature of the absorbing species, and the solvent. For strongly absorbing compounds, ε can be very large. For example, many organic dyes have molar absorptivities of 10,000 to 100,000 L · mol-1 · cm-1, whereas weakly absorbing metal complexes may have values below 100.

Tip: The molar absorptivity at the wavelength of maximum absorption (λmax) is the most commonly reported value and provides the highest sensitivity for quantitative measurements.

Molar absorptivity is typically determined experimentally by measuring the absorbance of solutions with known concentrations at a specific wavelength and using a standard cuvette path length (usually 1 cm).

Step-by-Step: How to Use the Beer-Lambert Law Calculator

  1. Choose what to solve for. Click one of the mode buttons at the top of the calculator (Absorbance, Transmittance, Molar Absorptivity, Path Length, or Concentration). The selected variable will be highlighted and its input field will be disabled.
  2. Enter the known values. Fill in the remaining input fields with your known data. Select appropriate units from the dropdown menus for path length and concentration.
  3. Click "Calculate". The calculator will compute the unknown variable and display all results in the results panel below, along with a step-by-step solution showing the math.
  4. Review the results. The solved variable is highlighted in the results. The calculator also automatically converts between absorbance and transmittance for your convenience.
  5. Try an example. Click the "Load Example" button to populate the fields with sample values (A = 0.5, ε = 100, l = 1 cm) and see how the calculator solves for concentration.

How to Convert Absorbance to Transmittance

Converting between absorbance and transmittance is straightforward using logarithmic relationships:

From Absorbance to Transmittance:
T = 10-A

From Transmittance to Absorbance:
A = -log10(T)

Example: If the absorbance is A = 0.5, then the transmittance is T = 10-0.5 = 0.3162, or 31.62%. Conversely, if 25% of light is transmitted, the absorbance is A = -log10(0.25) = 0.602.

Remember that when converting from percentage transmittance to the fractional form used in the formula, divide by 100 first: if %T = 45%, then T = 0.45 and A = -log10(0.45) = 0.347.

Applications in Spectroscopy and Analytical Chemistry

The Beer-Lambert Law has an exceptionally wide range of applications across science and industry:

Limitations of Beer-Lambert Law

While the Beer-Lambert Law is a powerful tool, it has several important limitations that users should be aware of:

  1. High Concentration Deviations: The law assumes that absorbing molecules behave independently. At high concentrations (typically above 0.01 M), molecular interactions such as aggregation, dimerization, or changes in refractive index cause deviations from linearity.
  2. Stray Light: Imperfect monochromators in spectrophotometers allow small amounts of non-absorbed wavelengths (stray light) to reach the detector, causing apparent negative deviations at high absorbance values.
  3. Non-Monochromatic Light: The law strictly applies only to monochromatic (single-wavelength) light. Using polychromatic light can cause deviations, especially if the absorption coefficient varies significantly across the bandwidth.
  4. Chemical Equilibria: If the absorbing species participates in chemical equilibria (e.g., acid-base reactions, complex formation) that shift with concentration, the effective molar absorptivity changes and the law appears to fail.
  5. Scattering Effects: Turbid or heterogeneous samples scatter light, reducing the transmitted intensity and causing apparent increases in absorbance that are not due to true absorption.
  6. Fluorescence: If the sample fluoresces, re-emitted light can reach the detector and lead to erroneously low absorbance readings.
  7. Path Length Accuracy: The law assumes a precisely known path length. Dirty or scratched cuvette windows, meniscus effects, or incorrect cell positioning can introduce errors.
Best Practice: For the most accurate results, work within an absorbance range of 0.1 to 1.0, use high-quality monochromatic light, and prepare fresh calibration standards in the same solvent as your unknown sample.

Frequently Asked Questions

In most practical contexts, absorbance and optical density (OD) are used interchangeably. Both are defined as A = -log10(I/I0). However, strictly speaking, optical density can also include contributions from scattering, whereas absorbance refers specifically to true absorption. In clear solutions measured with a spectrophotometer, the two values are effectively identical.

At high concentrations, molecules are closer together and can interact with each other through electrostatic forces, hydrogen bonding, or aggregation. These interactions change the effective molar absorptivity, causing the relationship between absorbance and concentration to become non-linear. Additionally, the refractive index of the solution may change significantly at high concentrations, altering the path of light through the sample. The law is most reliable at concentrations below about 0.01 M.

The standard units are: concentration in mol/L (molarity, M), path length in cm, and molar absorptivity in L · mol-1 · cm-1. Absorbance is dimensionless. When using this calculator, any unit conversions (mm to cm, mmol/L to mol/L, etc.) are handled automatically. Just make sure your molar absorptivity value corresponds to the wavelength at which you measured the absorbance.

Yes, the Beer-Lambert Law applies to gases as well as solutions. For gases, the concentration is often expressed in terms of partial pressure or number density, and the absorption cross-section is used instead of molar absorptivity. The law is fundamental to atmospheric spectroscopy, gas sensing, and industrial emissions monitoring. The same principles apply: absorbance is proportional to the amount of absorbing substance in the light path.

To determine molar absorptivity experimentally: (1) Prepare several solutions of known concentration. (2) Measure the absorbance of each solution at the desired wavelength using a spectrophotometer with a cuvette of known path length (typically 1 cm). (3) Plot absorbance vs. concentration. The slope of the line equals ε × l. Since l is known (1 cm), the slope directly gives ε. This process is called creating a calibration curve. Alternatively, you can find published values in chemistry databases and handbooks.

The ideal absorbance range for reliable spectrophotometric measurements is between 0.1 and 1.0 (corresponding to about 10% to 80% transmittance). Below 0.1, the signal-to-noise ratio becomes poor and small errors in transmittance lead to large errors in absorbance. Above 1.0, stray light effects become significant and can cause negative deviations from linearity. If your sample's absorbance falls outside this range, dilute or concentrate the sample, or use a different path length cuvette.

A calibration curve is a practical application of the Beer-Lambert Law. By measuring absorbance values for a series of standard solutions with known concentrations, you can plot A vs. c. According to the Beer-Lambert Law, this plot should be a straight line passing through the origin with a slope equal to ε × l. Once the calibration curve is established, you can determine the concentration of an unknown sample by measuring its absorbance and reading the corresponding concentration from the graph (or using the equation of the best-fit line).