A UV spectrophotometer is a scientific instrument designed to measure the absorption or transmission of ultraviolet (UV) light by a sample. It analyzes the interaction between UV light and the chemical components of the sample. The device typically consists of a light source that emits UV radiation, a monochromator to select specific wavelengths, a sample holder where the substance to be analyzed is placed, a detector to measure the intensity of light passing through the sample, and a data - processing unit to display and analyze the results.
The development of the UV spectrophotometer has its roots in the early understanding of light absorption by substances. In the early 20th century, significant advancements in optical and electronic technologies enabled the creation of the first basic spectrophotometric devices. The first commercial UV - visible spectrophotometer was developed by Arnold O. Beckman in 1940. Since then, continuous improvements in components such as light sources, detectors, and data - handling systems have led to the highly sophisticated and accurate UV spectrophotometers we have today.
The principle of a UV spectrophotometer is based on the Beer - Lambert law, which states that the absorbance (A) of a solution is directly proportional to the concentration (c) of the absorbing species and the path length (l) of the light through the solution. Mathematically, it is expressed as (A=epsilon cl), where (epsilon) is the molar absorptivity (a characteristic constant for a particular substance at a given wavelength). When UV light passes through a sample, the molecules in the sample absorb photons of specific energies corresponding to certain wavelengths. The detector measures the intensity of the incident light ((I_0)) and the intensity of the light emerging from the sample ((I)). The absorbance is then calculated as (A = logfrac{I_0}{I}).