Extinction Coefficient Formula:
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The extinction coefficient (ε_260) is a measure of how strongly oligonucleotides absorb light at 260 nm wavelength. It is used to quantify DNA/RNA concentration and is essential for molecular biology applications including PCR, sequencing, and hybridization studies.
The calculator uses the extinction coefficient formula:
Where:
Explanation: The formula accounts for the fact that in double-stranded DNA or structured oligonucleotides, base stacking reduces the actual absorbance compared to the sum of individual base contributions.
Details: Accurate extinction coefficient calculation is crucial for determining oligonucleotide concentration, ensuring proper experimental conditions, and achieving reproducible results in molecular biology experiments.
Tips: Enter the sum of base extinction coefficients and sum of modification extinction coefficients in M⁻¹ cm⁻¹. Both values must be non-negative. The calculator automatically applies the 0.9 hypochromicity correction factor.
Q1: What are typical extinction coefficient values for nucleotides?
A: Typical values are approximately: A=15,400, C=7,400, G=11,500, T=8,700 M⁻¹ cm⁻¹ at 260 nm.
Q2: Why is the 0.9 correction factor used?
A: The 0.9 factor accounts for hypochromicity - the reduction in absorbance due to base stacking interactions in oligonucleotides.
Q3: How do modifications affect extinction coefficients?
A: Chemical modifications like fluorescent dyes, biotin, or other tags have their own extinction coefficients that must be added to the base sum.
Q4: When should I use this calculation?
A: Use this for oligonucleotide quantification, primer preparation, and any application requiring accurate DNA/RNA concentration determination.
Q5: Are there limitations to this equation?
A: The 0.9 factor is an approximation; actual hypochromicity may vary with sequence composition, length, and secondary structure.