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Unbalanced Wheatstone Bridge Equivalent Resistance

Learn to calculate equivalent resistance in an unbalanced Wheatstone bridge using Kirchhoff's laws and delta-star transformations.

4 min readPublished 4 June 2026
Current ElectricityKirchhoff's laws

Concept Overview

This problem tests the ability to find the equivalent resistance of a complex circuit, specifically an unbalanced Wheatstone bridge. Unlike a balanced bridge where simplification is straightforward, an unbalanced bridge requires more advanced techniques. We will explore how to apply Kirchhoff's laws and, if necessary, the delta-star (or star-delta) transformation to systematically solve for the equivalent resistance between two specified nodes.

Solution:

Step 1: Understand the Circuit and the Goal We are given a Wheatstone bridge circuit with resistors R1,R2,R3,R4,R_1, R_2, R_3, R_4, and R5R_5. The bridge is not balanced, meaning R1/R2R3/R4R_1/R_2 \neq R_3/R_4. We need to find the equivalent resistance between two specific nodes, say A and B. Let's assume the nodes are the two points where the galvanometer (or the fifth resistor R5R_5) is connected.

Step 2: Apply Kirchhoff's Laws (Method 1 - Direct Application) This method involves setting up a system of linear equations using Kirchhoff's Current Law (KCL) and Kirchhoff's Voltage Law (KVL).

  • KCL: At each junction (node), the sum of incoming currents equals the sum of outgoing currents.
  • KVL: The sum of voltage drops around any closed loop is zero.

Let's denote the nodes of the bridge as follows: the input terminals as P and Q, and the intermediate nodes as A and B. Let R1R_1 be between P and A, R2R_2 between P and B, R3R_3 between A and Q, R4R_4 between B and Q, and R5R_5 between A and B. We want to find the equivalent resistance between P and Q.

Assume a voltage VV is applied across P and Q. Let the currents through R1,R2,R3,R4,R5R_1, R_2, R_3, R_4, R_5 be I1,I2,I3,I4,I5I_1, I_2, I_3, I_4, I_5 respectively. At node A: I1=I3+I5I_1 = I_3 + I_5 At node B: I2=I4I5I_2 = I_4 - I_5 (or I2+I5=I4I_2 + I_5 = I_4 if I5I_5 flows from B to A) Let's assume I5I_5 flows from A to B. At node A: I1=I3+I5I_1 = I_3 + I_5 At node B: I2=I4I5I_2 = I_4 - I_5 At node P: Itotal=I1+I2I_{total} = I_1 + I_2 At node Q: I3+I4=ItotalI_3 + I_4 = I_{total}

Now apply KVL to the loops: Loop PAB: I1R1+I5R5I2R2=0I_1 R_1 + I_5 R_5 - I_2 R_2 = 0 Loop ABQ: I3R3+I4R4I5R5=0I_3 R_3 + I_4 R_4 - I_5 R_5 = 0 Loop PBQ: I2R2+I4R4V=0I_2 R_2 + I_4 R_4 - V = 0 Loop PAQ: I1R1+I3R3V=0I_1 R_1 + I_3 R_3 - V = 0

We have 4 equations and 5 unknowns (I1,I2,I3,I4,I5I_1, I_2, I_3, I_4, I_5). However, we are interested in the total current Itotal=I1+I2I_{total} = I_1 + I_2 for a given voltage VV. We can solve these equations to express I1I_1 and I2I_2 in terms of VV and the resistances. The equivalent resistance ReqR_{eq} will be V/ItotalV / I_{total}. This method can be algebraically intensive.

Step 3: Delta-Star (Δ-Y) Transformation (Method 2 - Simplification) When Kirchhoff's laws become too complex, we can use delta-star transformations to simplify the circuit. A delta (Δ) network consists of three resistors connected in a triangle, and a star (Y) network consists of three resistors connected to a common central point.

Consider the delta formed by resistors R1,R2,R_1, R_2, and R5R_5. We can convert this delta into a star network with a central node (say, C) and three resistors R1C,R2C,R5CR_{1C}, R_{2C}, R_{5C} connected to C and to the original nodes A, B, and P respectively. The transformation formulas are:

R1C=R1R5R1+R2+R5R_{1C} = \frac{R_1 R_5}{R_1 + R_2 + R_5} R2C=R2R5R1+R2+R5R_{2C} = \frac{R_2 R_5}{R_1 + R_2 + R_5} R5C=R1R2R1+R2+R5R_{5C} = \frac{R_1 R_2}{R_1 + R_2 + R_5}

After this transformation, the circuit will have resistors R1C,R2C,R5CR_{1C}, R_{2C}, R_{5C} connected to a new node C. The original resistors R3R_3 and R4R_4 will now be in series with R1CR_{1C} and R2CR_{2C} respectively (or in parallel depending on the configuration). The circuit becomes a simpler series-parallel combination.

Alternatively, we can consider the delta formed by R3,R4,R5R_3, R_4, R_5. Converting this delta to a star with a central node D and resistors R3D,R4D,R5DR_{3D}, R_{4D}, R_{5D} connected to A, B, and Q respectively.

R3D=R3R5R3+R4+R5R_{3D} = \frac{R_3 R_5}{R_3 + R_4 + R_5} R4D=R4R5R3+R4+R5R_{4D} = \frac{R_4 R_5}{R_3 + R_4 + R_5} R5D=R3R4R3+R4+R5R_{5D} = \frac{R_3 R_4}{R_3 + R_4 + R_5}

This will also simplify the circuit into a series-parallel combination.

Step 4: Solve the Simplified Circuit After performing the delta-star transformation, the circuit will be reduced to a combination of resistors in series and parallel. The equivalent resistance can then be calculated using the standard formulas:

  • For resistors in series: Rseries=Ra+Rb+...R_{series} = R_a + R_b + ...
  • For resistors in parallel: $\frac{1}{R_{parallel}} = \frac{1}{R_a} + \frac{1}{R_b} + ...

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