We report on a measurement of a highly forbidden magnetic-dipole transition amplitude in ytterbium using the Stark-interference technique. This amplitude is important in interpreting a future parity nonconservation experiment that exploits the same transition. We find | 5d6s 3 D1|M 1|6s 2 1 S0 | = 1.33(6)Stat(20) β × 10 −4 µ0, where the larger uncertainty comes from the previously measured vector transition polarizability β. The M 1 amplitude is small and should not limit the precision of the parity nonconservation experiment.PACS numbers: 32.70. Cs,32.60.+i,32.80.Ys The proposal to measure parity nonconservation (PNC) in the 6s 2 1 S 0 → 5d6s 3 D 1 transition in atomic ytterbium (Yb) [1] has prompted both theoretical [2,3] and experimental [4,5] studies. The magnetic-dipole (M 1) amplitude for this transition is a key quantity for evaluating the feasibility of a PNC-Stark interference experiment as proposed in [1]. A nonzero M 1 amplitude coupled with imperfections in the apparatus can lead to systematic uncertainties in a PNC experiment. Here we present the first experimental determination of the magnetic-dipole amplitude for the 1 S 0 → 3 D 1 transition. Our method is based on the technique of Stark interference [6,7,8].In the absence of external fields, the 1 S 0 → 3 D 1 transition ( Fig. 1) whereε is the direction of the polarization of the laser light, (E ×ε) q is the q component of the vector in the spherical basis, and the vector transition polarizability β is a real parameter. The magnitude of β was measured [5]:In an electric field, the transition amplitude is the sum of the Stark-induced E1 amplitude and the forbidden M 1 amplitude. The corresponding transition rate iswhere we neglect the contribution from |A(M 1)| 2 since |A(M 1)| ≪ |A(E1 St )| with the electric fields and polarization angles used here. The Stark-induced amplitude is proportional to E. Thus, reversing E changes the total transition rate, allowing the interference term to be isolated from the larger terms. The M 1 amplitude is given bywherek is the direction of propagation of the excitation light. Equation 1 implies that only the M J = ±1 components of the upper state are excited by A(E1 St ),