Spectrophotometry: Measuring Concentration with Light

How spectrophotometers measure absorbance and transmittance to determine concentration, from cuvettes and wavelength selection to calibration curves.

Quick answer

Spectrophotometry determines the concentration of a colored solution by shining light through it and measuring how much light is absorbed. A spectrophotometer compares the light passing through the sample to a blank, reporting absorbance, which grows linearly with concentration in dilute solutions.

A=−log⁡10TA = -\log_{10} T

Unit: absorbance is unitless; transmittance as a decimal or percent

Example: If a sample transmits 10% of the incoming light (T = 0.10), its absorbance is A = −log(0.10) = 1.00. A solution that transmits only 1% of the light has an absorbance of 2.00.

What you will learn

  • Describe how a spectrophotometer measures light absorption
  • Convert between transmittance and absorbance
  • Explain the roles of the blank, cuvette, and wavelength selection
  • Build and use a calibration curve to find an unknown concentration
  • List common sources of error in absorbance measurements

The core idea: color tells concentration

Many substances reveal their concentration through color: a darker blue copper solution simply contains more copper ions than a pale one. Spectrophotometry turns that everyday observation into a precise measurement. Instead of trusting the human eye, an instrument called a spectrophotometer shines light of a chosen wavelength through the sample and measures exactly how much light comes out the other side.

Because the relationship between absorbed light and concentration is mathematical — and linear in dilute solutions — a single absorbance reading can reveal an unknown concentration with impressive accuracy. The technique is fast, inexpensive, and non-destructive, which is why it appears in nearly every analytical laboratory.

How a spectrophotometer works

Light travels a controlled path inside the instrument:

  1. Light source: a lamp produces a broad spectrum of light (visible lamps for colored solutions, deuterium lamps for ultraviolet work).
  2. Wavelength selector: a prism or diffraction grating isolates one narrow wavelength band — the color most strongly absorbed by the analyte.
  3. Sample holder: the solution sits in a small transparent container called a cuvette, usually with a 1 cm light path.
  4. Detector: measures the intensity of light that passed through the sample and compares it to the intensity through a blank.

The blank — a cuvette of pure solvent — is measured first to zero the instrument. This subtracts any light absorbed by the solvent and the cuvette walls, so the final reading reflects only the analyte.

Transmittance and absorbance

Two numbers describe what the light did inside the cuvette. Transmittance (TT) is the fraction of incoming light that makes it through the sample:

T=II0T = \frac{I}{I_0}

where I0I_0 is the incident intensity and II is the transmitted intensity. Absorbance (AA) expresses the same information on a logarithmic scale:

A=−log⁡10TA = -\log_{10} T

The logarithm matters: each absorbance unit represents a tenfold drop in transmitted light. A solution with T=0.10T = 0.10 (10% transmitted) has A=1.0A = 1.0; T=0.01T = 0.01 (1% transmitted) gives A=2.0A = 2.0. Absorbance is the more useful quantity because, in dilute solutions, it is directly proportional to concentration — the foundation of the Beer-Lambert law.

Choosing the right wavelength

Not all wavelengths are equal. Each absorbing substance has an absorption spectrum — a curve of absorbance versus wavelength — with a peak at the wavelength it absorbs most strongly (λmax\lambda_{max}). Measuring at λmax\lambda_{max} gives the largest signal for a given concentration, which means the smallest relative error.

There is also a neat color relationship: a substance absorbs most strongly in the complementary color of what you see. A blue solution looks blue because it transmits blue light and absorbs orange-red light, so its λmax\lambda_{max} sits in the orange-red region. In practice, you scan the spectrum once to find the peak, then make all quantitative measurements at that wavelength.

Measure at the peak

Always determine the wavelength of maximum absorbance first and measure there. It gives the strongest signal and the most reliable calibration curve.

Calibration curves

To convert absorbance readings into concentrations, chemists build a calibration curve (also called a standard curve):

  1. Prepare a series of standard solutions with known concentrations spanning the expected range.
  2. Measure the absorbance of each standard at λmax\lambda_{max}, using the blank to zero the instrument.
  3. Plot absorbance (vertical axis) against concentration (horizontal axis) — the points should form a straight line through the origin.
  4. Measure the unknown sample's absorbance and read its concentration off the line.

Using several standards instead of a single conversion factor averages out small errors and immediately reveals problems: if the points curve instead of lining up, the samples may be too concentrated for the linear range.

Practical tips and errors

Accurate spectrophotometry depends on careful technique:

  • Handle cuvettes by the frosted sides only. Fingerprints on the clear faces scatter light and inflate absorbance.
  • Remove bubbles from the sample; they scatter the beam unpredictably.
  • Re-zero with the blank if you change wavelengths or if the instrument has been sitting.
  • Dilute samples that read above about A=1.5A = 1.5 so they fall in the reliable linear range.
  • Match cuvettes: the blank and sample cuvettes should be an optically matched pair, and plastic cuvettes are for visible light only — they absorb ultraviolet.

With these habits, a benchtop spectrophotometer routinely measures concentrations to within a percent or two — remarkable precision from simply shining light through a colored liquid.

Variables and units

SymbolNameUnitMeaning
TTtransmittanceunitless (decimal)Fraction of incident light transmitted through the sample, from 0 to 1.
AAabsorbanceunitlessLogarithmic measure of light absorbed by the sample; proportional to concentration.
I0I_0incident light intensityarbitrary detector unitsIntensity of light entering the sample.
IItransmitted light intensityarbitrary detector unitsIntensity of light emerging from the sample.

Common mistakes

✗ Absorbance and transmittance are just two words for the same thing.

They are inversely related on a logarithmic scale: absorbance equals negative log of transmittance. A transmittance of 10% (0.10) means an absorbance of 1.0, and 1% transmittance means an absorbance of 2.0.

✗ You can estimate concentration accurately just by eyeballing the color.

Human vision is unreliable for quantification — lighting, background, and individual perception all vary. A spectrophotometer measures light intensity objectively and reproducibly, which is what makes the result trustworthy.

✗ Any wavelength will work as long as the solution has some color.

Sensitivity peaks at the wavelength of maximum absorbance. Measuring elsewhere gives a weak signal where small errors matter more, degrading the quality of the analysis.

✗ A higher absorbance reading is always better.

Above an absorbance of about 1 to 2, very little light reaches the detector, so stray light and noise dominate the reading. Samples that read too high should be diluted into the reliable range instead.

Real-world applications

  • Water quality laboratories measure nitrate and phosphate levels in drinking water

  • Clinical labs determine hemoglobin and other blood components from light absorption

  • Food manufacturers verify dye content and color consistency in products

  • Molecular biologists quantify DNA and RNA by their absorbance at 260 nm

  • Environmental scientists track pollutants in rivers and wastewater

Frequently asked questions

Why must the cuvette be wiped clean before measuring?

Fingerprints, dust, and water spots scatter or absorb the light beam, which falsely raises the absorbance reading. Wiping the outside of the cuvette with a lint-free tissue before each measurement removes this source of error.

What is a blank, and why do you need one?

A blank is a cuvette containing only the solvent (no analyte), used to zero the instrument. It cancels out light absorbed by the solvent and the cuvette itself, so the reported absorbance comes only from the substance you care about.

Why measure at the wavelength of maximum absorbance?

Sensitivity is highest at the wavelength of maximum absorbance, so small concentration differences produce the largest signal changes there. Measuring at the peak also minimizes the relative error from instrument noise and small wavelength drifts.

Can spectrophotometry measure a colorless solution?

Not directly with visible light, since there is nothing to absorb it. Colorless analytes can be measured in the ultraviolet range if they absorb there, or they can be reacted with a color-forming reagent that converts them into a colored product.