We present the development of Fermi-level crossings from the clean to the h
ydrogen-saturated (110) surface of molybdenum at room temperature. The well
-known adsorbate-induced phonon anomaly is discussed in terms of a quasi-on
e-dimensional Fermi-surface nesting and giant Kohn anomaly. Our experiment
resolved an existing discrepancy between earlier photoemission data and Fer
mi-surface contours calculated within density-functional theory. Moreover,
it is found that the Fermi-surface nesting is fully established at hydrogen
coverages where the phonon anomaly just barely forms.