Stray light fakes low A
Aging lamps or dirty optics leak extra light, making strong absorbers read artificially low—linearity often fades past A ≈ 1.5–2.0.
Tips: Press Enter to calculate. Keep values within your spectrophotometer’s linear range (often A ≲ 1.0–1.5).
The Beer–Lambert law relates absorbance \(A\) to molar absorptivity \(\varepsilon\), path length \(l\), and concentration \(c\): \[ A = \varepsilon \, l \, c. \] Provide any three, and the fourth is computed. If you enter percent transmittance, the tool uses \(A = -\log_{10}(T)\) with \(T = \%T/100\).
NADH at 340 nm. Given \(\varepsilon = 6220\ \mathrm{L\,mol^{-1}\,cm^{-1}}\), \(l = 1.00\ \mathrm{cm}\), and \(c = 0.10\ \mathrm{mM}\):
The Beer–Lambert law, sometimes called the Beer–Lambert–Bouguer law, is a cornerstone of modern analytical chemistry and biochemistry. It provides a simple mathematical relationship between the absorbance of light by a sample and three key physical quantities: the molar absorptivity (\(\varepsilon\)), the path length of the light through the sample (\(l\)), and the concentration of the absorbing species (\(c\)). The equation is written as:
\( A = \varepsilon \, l \, c \)
Many spectrophotometers measure % transmittance (%T), the fraction of light that passes through the sample compared to a blank. Absorbance is related by:
\( A = -\log_{10}(T) \), where \( T = \dfrac{\%T}{100} \).
For example, if a sample transmits 25% of the incident light, then \( A = -\log_{10}(0.25) = 0.602 \).
The Beer–Lambert law is widely used in UV-Vis spectroscopy, biological assays (such as protein concentration by absorbance at 280 nm), enzyme kinetics, and even environmental monitoring (detecting pollutants in water). Because absorbance is linear with concentration under ideal conditions, it enables precise and reproducible quantification without destroying the sample.
The relationship holds best for solutions that are dilute, homogeneous, and measured with monochromatic light. At very high absorbance values (A > 2), too little light passes through, leading to inaccuracies. Scattering, fluorescence, or chemical interactions can also cause deviations. For reliable results, always use an appropriate blank, keep within the linear range of your instrument, and report the wavelength used along with ε values.
In summary, the Beer–Lambert law bridges light and matter: by measuring how much light a solution absorbs, you can back-calculate concentration or other variables. This makes it one of the most versatile and important equations in laboratory science.
Aging lamps or dirty optics leak extra light, making strong absorbers read artificially low—linearity often fades past A ≈ 1.5–2.0.
Microvolume specs auto-scale path length (sub-mm); if auto mode glitches, reported concentration can be off by orders of magnitude.
Turbid samples or nanoparticles deflect light, inflating “absorbance” even without chromophores—good blanks and cuvette positioning matter.
Extinction coefficients are specific to wavelength/solvent; drifting a few nm off peak can change ε enough to skew concentration.
Highly fluorescent samples can re-emit and reabsorb light; front-face geometry or shorter path cuvettes keep Beer–Lambert usable.