  The Canadian MOST satellite is a unique platform for observations of bright
transiting exoplanetary systems. Providing nearly continuous photometric
observations for up to 8 weeks, MOST can produce important observational data
to help us learn about the properties of exosolar planets. We review our
current observations of HD 209458, HD 189733 with implications towards the
albedo and our progress towards detecting reflected light from an exoplanet.
