The hydrogenation of C-rich Si leads to the formation of two (almost) energetically degenerate H * 2 (C) complexes, each containing one substitutional C (Cs) and two interstitial H atoms which are located at a bond-centered (bc) and an anti-bonding (ab) site, respectively. The two defects are trigonal: Cs − H bc · · · Si − H ab and H ab − Cs · · · H bc − Si. Fourier-transform infrared (FTIR) absorption spectra of these two defects should show two Cs − H and two Si − H stretch modes, but the H ab − Cs mode was absent in earlier studies. The missing line has now been observed by FTIR in especially C-rich Si material. The line is unexpectedly broad, suggesting a very short vibrational lifetime. Partial D substitutions result in the formation of a H ab − Cs · · · D bc − Si center. In this defect, the H ab − Cs line shifts by only 0.3 cm −1 but becomes very sharp, suggesting a long lifetime. The IR line widths show that the vibrational lifetime of the H ab − Cs mode in H ab − Cs · · · D bc − Si is about 16 times longer than that of the same H ab − Cs mode in H ab − Cs · · · H bc − Si. This paper contains experimental data and first-principles calculations which explain this isotope effect.