Spectrophotometer
A spectrometer is an instrument that provides information about the intensity of radiated energy. It determines the ratio between the intensity of light emitted from an internal source and that which passes through a given solution. This ratio can be used to determine the concentration of dissolved molecules in a sample.
Before a sample is measured, the spectrophotometer is set to measure at a certain wavelength. The detected wavelength can be tuned to a value optimal for measuring a specific compound.
On measurement, the spectrophotometer returns data as absorbance values (A). Absorbance is calculated as
The relationship between absorbance and concentration is linear and is described by Beer-Lambert Law:
where c is the concentration of the solution, l is the pathlength, otherwise described as the distance traveled by light when passing through a solution (typically the width of a cuvette), and ε is the extinction coefficient, which is specific for a compound.
Figure 1: Components of a spectrophotometer.
In an example, we will measure concentrations of
There are certain limitations of the Beer-Lambert Law that spectrophotometer users must consider. Some of these are related to technical issues; however, the law does have a real limitation; because it only applies to dilute solutions. When the concentration of an absorbing species increases, so does the frequency of physicochemical interactions among the molecules. Thus, at a given concentration, the molecules will begin to affect the charge distribution of the neighbor molecules. When this occurs, the relationship between absorbance and concentration is no longer linear. As a rule of thumb, one should stay below an absorption value of 1 when doing measurements.
Absorbance is inversely proportional to transmittance (light passing through a sample that is not absorbed). When absorbance