Editing Spectrophotometry (section)

==Overview==
Spectrophotometry is a tool that hinges on the quantitative analysis of molecules depending on how much light is absorbed by colored compounds. Important features of spectrophotometers are spectral bandwidth (the range of colors it can transmit through the test sample), the percentage of sample transmission, the logarithmic range of sample absorption, and sometimes a percentage of reflectance measurement.

A spectrophotometer is commonly used for the measurement of transmittance or reflectance of solutions, transparent or opaque solids, such as polished glass, or gases. Although many biochemicals are colored, as in, they absorb visible light and therefore can be measured by colorimetric procedures, even colorless biochemicals can often be converted to colored compounds suitable for chromogenic color-forming reactions to yield compounds suitable for colorimetric analysis.<ref name=":0" />{{Rp|65}} However, they can also be designed to measure the [[Reflectivity|diffusivity]] on any of the listed light ranges that usually cover around 200–2500&nbsp;nm using different controls and [[calibrations]].<ref name=":1" /> Within these ranges of light, calibrations are needed on the machine using standards that vary in type depending on the [[wavelength]] of the ''photometric determination''.<ref>{{Cite book|title=The essential guide to analytical chemistry|last=Schwedt|first=Georg|date=1997|publisher=Wiley|isbn=9780471974123|location=Chichester, NY|pages=16–17|translator-last=Brooks|translator-first=Haderlie|oclc=36543293|name-list-style=vanc}}</ref>

An example of an experiment in which spectrophotometry is used is the determination of the equilibrium constant of a solution. A certain chemical reaction within a solution may occur in a forward and reverse direction, where reactants form products and products break down into reactants. At some point, this chemical reaction will reach a point of balance called an equilibrium point. To determine the respective concentrations of reactants and products at this point, the light transmittance of the solution can be tested using spectrophotometry. The amount of light that passes through the solution is indicative of the concentration of certain chemicals that do not allow light to pass through.

The absorption of light is due to the interaction of light with the electronic and vibrational modes of molecules. Each type of molecule has an individual set of energy levels associated with the makeup of its chemical bonds and nuclei and thus will absorb light of specific wavelengths, or energies, resulting in unique spectral properties.<ref name=":2" /> This is based upon its specific and distinct makeup.

The use of spectrophotometers spans various scientific fields, such as [[physics]], [[materials science]], [[chemistry]], [[biochemistry]], [[chemical engineering]], and [[molecular biology]].<ref name=":3">{{Cite book|title=Experimental Methods in Modern Biochemistry|last=Rendina|first=George|date=1976|publisher=W. B. Saunders Company|isbn=0721675506|location=Philadelphia, PA|pages=[https://archive.org/details/experimentalmeth00rend/page/46 46-55]|oclc=147990|name-list-style=vanc|url-access=registration|url=https://archive.org/details/experimentalmeth00rend/page/46}}</ref> They are widely used in many industries including semiconductors, laser and optical manufacturing, printing and forensic examination, as well as in laboratories for the study of chemical substances. Spectrophotometry is often used in measurements of enzyme activities, determinations of protein concentrations, determinations of enzymatic kinetic constants, and measurements of ligand binding reactions.<ref name=":0" />{{Rp|65}} Ultimately, a spectrophotometer is able to determine, depending on the control or calibration, what substances are present in a target and exactly how much through calculations of observed wavelengths.

In [[astronomy]], the term spectrophotometry refers to the [[Spectroscopy (astronomy)|measurement of the spectrum]] of a [[celestial object]] in which the [[Spectral flux density|flux]] scale of the spectrum is calibrated as a function of [[wavelength]], usually by comparison with an observation of a spectrophotometric standard star, and corrected for the absorption of light by the Earth's atmosphere.<ref>{{cite journal|last1=Oke|first1=J. B.|last2=Gunn|first2=J. E.|title=Secondary standard stars for absolute spectrophotometry|journal=The Astrophysical Journal|date=1983|volume=266|page=713|doi=10.1086/160817|bibcode=1983ApJ...266..713O}}</ref>