  A list of 50 optically observable O stars that are likely on or very near the
ZAMS is presented. They have been selected on the basis of five distinct
criteria, although some of them exhibit more than one. Three of the criteria
are spectroscopic (He II \lambda4686 absorption stronger than in normal
luminosity class V spectra, abnormally broad or strong Balmer lines, weak UV
wind profiles for their spectral types), one is environmental (association with
dense, dusty nebular knots), and one is photometric (derived absolute
magnitudes fainter than class V). Very few of these stars have been physically
analyzed, and they have not been considered in the current framework of early
massive stellar evolution. In particular, they may indicate that the earliest,
embedded phases are not as large a fraction of the main-sequence lifetimes as
is currently believed. Detailed analyses of these objects will likely prove
essential to a complete understanding of the early evolution of massive stars.
