The Kennelly theorem, named in honor of Arthur Edwin Kennelly, allows us to determine the equivalent charge in a star to one given in a triangle and vice versa. The theorem is also often called star-triangle transformation (written Y-Δ) or te-delta transformation (written T -Δ).
Transformation equations
The following table shows the transformation equations as a function of impedances and admittances.
Kennelly equations
Transformation Δ-Y
Depending on impedance
Depending on admissions
Transformation Y-Δ
Depending on impedance
Depending on admissions
Demonstration
The Kennelly equations are analytically demonstrated below.
Triangle to star circuit
Figure 1. Equivalence between loads in star (left) and triangle (right).
Let us assume the values ZAB, ZBC and ZAC of the triangle load in figure 1 are known and we wish to obtain the values ZAT, ZBT and ZCT of its star equivalent. To do this, we will obtain in both circuits the equivalent impedances with respect to points A-B, B-C and A-C and we will equalize them since they are equivalent charges (note that in the star there are always two impedances in series, while in the triangle there are two in series with the third in parallel):
The Kennelly equations are obtained from the previous ones in the following way:
Add the equations (1) and (3) and subtract the result of the (2)
Add the equations (1) and (2) and subtract the result of (3)
Add the equations (2) and (3) and subtract the result of (1)
Star to Triangle
Let us now assume the opposite case, that is, the values ZAT, ZBT and ZCT of the star in the figure are known. 1, we want to obtain the values ZAB, ZBC and ZAC of the equivalent delta load. To do this, the Δ-Y transformation equations will be taken, where for simplification of notation we will take
leaving the following equations:
;
;
By performing the three possible binary multiplications between them, we obtain
And adding them
We split the first member for the value of :
And dividing the second member by :
By matching both results we get one of the transformation equations. The other two can be obtained in the same way by dividing by and