Currently, twenty percent of all red M-dwarfs are thought to harbor rocky planets within their habitable zones. Those are the regions around the star where rocky planets could maintain liquid water on their surfaces. Each of these rocky planets is a puzzle piece of how planets are born, evolve and function. But few of these potentially habitable planets have been observationally characterized. That’s because orbitally close-in rocky planets are simply easier to detect as they transit across the faces of these small parent stars.