Beer-Lambert Law:
From: | To: |
The Beer-Lambert Law relates the absorption of light to the properties of the material through which the light is traveling. It states that the concentration of an absorbing species is directly proportional to the absorbance and inversely proportional to the path length and molar extinction coefficient.
The calculator uses the Beer-Lambert Law equation:
Where:
Explanation: The equation shows that concentration is directly proportional to absorbance and inversely proportional to both the molar extinction coefficient and the path length of the sample.
Details: Calculating concentration from absorbance is fundamental in spectroscopy and analytical chemistry. It's used to determine unknown concentrations of solutions in various fields including biochemistry, environmental science, and pharmaceutical analysis.
Tips: Enter absorbance (typically between 0-2 for accurate results), molar extinction coefficient (specific to the substance being measured), and path length (usually 1 cm for standard cuvettes). All values must be positive.
Q1: What is the ideal absorbance range for accurate measurements?
A: The most accurate measurements are typically obtained with absorbance values between 0.1 and 1.0. Values above 2 may be less accurate due to detector limitations.
Q2: Where can I find molar extinction coefficients?
A: Molar extinction coefficients are substance-specific and can be found in chemical literature, databases, or sometimes on the product information sheet for commercial compounds.
Q3: Why is path length important?
A: Path length affects how much light is absorbed. Standard cuvettes have 1 cm path length, but different path lengths require adjustment in calculations.
Q4: What if my absorbance is too high?
A: For high absorbance samples, you can either dilute the sample or use a shorter path length cuvette to bring the measurement into the optimal range.
Q5: Does this work for mixtures of compounds?
A: For mixtures, you typically need absorbance measurements at multiple wavelengths and knowledge of each component's extinction coefficients at those wavelengths.