How to Measure Fluorescence With a Spectrofluorometer

Fluorescence is a light-emitting phenomenon where a substance absorbs light energy at a specific, high-energy wavelength and then re-emits that energy as light at a longer, lower-energy wavelength. This process, known as photoluminescence, occurs rapidly, typically within nanoseconds of absorption. The unique signature of this re-emitted light allows scientists to identify, track, and measure specific molecules. Because many molecules do not naturally fluoresce, researchers often attach highly fluorescent tags, known as fluorophores, to target substances for study.

Instrumentation: The Spectrofluorometer

The primary instrument used to precisely measure this light emission is the spectrofluorometer, which controls the light directed at the sample and the light collected from it. A spectrofluorometer utilizes four main components arranged to manage the excitation and emission process. The measurement begins with a powerful light source, typically a continuous Xenon lamp or a specific light-emitting diode (LED), which provides the energy needed to excite the sample. This source generates a broad spectrum of light, often ranging from ultraviolet into the visible spectrum.

The light path then encounters the excitation monochromator, an optical component that isolates a narrow band of wavelengths. A diffraction grating within the monochromator separates the incoming light into its constituent wavelengths, allowing the operator to select the wavelength matching the fluorophore’s absorption maximum. The now-monochromatic beam passes into the sample compartment, where the specimen is held within a transparent container, usually a quartz cuvette.

After the light interacts with the sample, the emitted fluorescence is collected at a 90-degree angle relative to the excitation beam. This perpendicular arrangement prevents the intense, unabsorbed excitation light from overwhelming the weaker fluorescent signal. The collected emission light then travels to the emission monochromator, which selects the specific, longer-wavelength fluorescent light while filtering out scattered excitation light. Finally, the selected emission light is directed to a sensitive detector, such as a Photomultiplier Tube (PMT), which converts the photons into a measurable electrical current.

The Mechanics of Fluorescence Measurement

Measuring fluorescence begins with careful sample preparation, typically involving dissolving the fluorophore in a solvent or binding it to a target molecule. The operator programs the spectrofluorometer to select the specific excitation wavelength the fluorophore absorbs most efficiently. This monochromatic beam strikes the sample, causing the fluorophore’s electrons to jump from their ground state to a higher-energy excited state. This excited state is highly unstable and short-lived, lasting only a few nanoseconds.

Before the electron returns to the ground state, the molecule sheds a small amount of absorbed energy, often as heat, through vibrational relaxation. Because this energy loss occurs before light is re-emitted, the resulting fluorescent photon has less energy than the absorbed photon. Consequently, the emitted light has a longer wavelength than the excitation light, adhering to Stokes’ law.

The emission monochromator is systematically scanned across wavelengths longer than the excitation wavelength to capture the full fluorescent output. This scanning produces a spectrum, which is a plot of light intensity versus wavelength. The spectrofluorometer measures the unique spectral fingerprint of the fluorophore, allowing for its detection and quantification even at very low concentrations. The detector measures the number of photons emitted at each wavelength, providing the raw data for analysis.

Interpreting the Results: Key Parameters

The data collected by the spectrofluorometer yields several metrics that characterize the fluorescent substance. The most straightforward measurement is Fluorescence Intensity, the brightness of the light signal, which is often directly proportional to the concentration of the fluorophore in the sample. Researchers use this relationship to perform quantitative analysis, determining the amount of a specific molecule present.

Two characteristic plots generated are the Excitation Spectrum and the Emission Spectrum. The excitation spectrum maps the intensity of the light absorbed across different wavelengths, while the emission spectrum plots the intensity of the light released across the longer wavelengths. The distinct shape and peak position of these spectra act as a unique identifier for the molecule being studied.

The difference between the peak wavelength of the excitation spectrum and the peak wavelength of the emission spectrum is known as the Stokes Shift. This energy gap is a fundamental property of a fluorophore and results from the energy lost during vibrational relaxation. A larger Stokes shift is advantageous for measurement sensitivity because it makes it easier to separate the desired fluorescent signal from the unwanted, scattered excitation light.

The Quantum Yield is a measure of the efficiency of the fluorescence process. It is defined as the ratio of the number of photons emitted to the number of photons absorbed. This metric indicates how effectively a molecule converts absorbed light into fluorescent light.

Where Fluorescence Measurement Is Used

Fluorescence measurement is widely utilized across various scientific disciplines due to its high sensitivity and selectivity. In biochemistry and molecular biology, the technique is routinely used to track specific molecules within living cells, such as monitoring protein-protein interactions or staining DNA. Fluorescent tags allow researchers to observe cellular processes in real-time without causing significant damage to the biological system.

The medical field employs fluorescence in diagnostic and imaging applications, notably in fluorescence-guided surgery, where dyes are injected to make tumors or damaged tissues glow. Environmental scientists use the technique to monitor water quality by detecting trace amounts of pollutants or to track wastewater flow. In material science, spectrofluorometers are used for quality control and to characterize new fluorescent materials, such as those used in organic light-emitting diodes (OLEDs) or solar cells.