Common Difference — Definition, Formula & Examples
The common difference is the fixed amount you add (or subtract) to get from one term to the next in an arithmetic sequence. It stays the same throughout the entire sequence.
For an arithmetic sequence , the common difference is the constant for all positive integers .
Key Formula
Where:
- = The common difference
- = The current term in the sequence
- = The next term in the sequence
How It Works
To find the common difference, subtract any term from the term that follows it. If you get the same result for every pair of consecutive terms, the sequence is arithmetic and that result is . A positive means the sequence increases, a negative means it decreases, and produces a constant sequence. Once you know and the first term , you can generate the entire sequence or jump directly to any term using .
Worked Example
Problem: Find the common difference of the arithmetic sequence 7, 13, 19, 25, 31, … and then find the 10th term.
Find d: Subtract the first term from the second term.
Verify: Check another pair to confirm the difference is constant.
Find the 10th term: Use the nth-term formula with , , and .
Answer: The common difference is , and the 10th term is 61.
Why It Matters
The common difference appears throughout Algebra 2 and Precalculus whenever you model situations with steady, constant change — monthly savings deposits, evenly spaced seating rows, or uniform dose increases. Recognizing quickly also lets you set up arithmetic series to find totals without adding every term individually.
Common Mistakes
Mistake: Confusing common difference with common ratio.
Correction: The common difference is found by subtracting consecutive terms (). The common ratio is found by dividing them () and belongs to geometric sequences, not arithmetic ones.
