Wet, rocky planets appear to be common in the universe, supported by indirect evidence. The discussion highlights the significance of the term M*sin(i) in exoplanet research, where 'i' represents the orbital inclination relative to the observer. This inclination affects the measurement of a planet's mass, as only a fraction of the wobble caused by the planet's gravitational pull can be observed. Consequently, the true mass of the planet is systematically underestimated, leading to the use of sin(i) in mass calculations. A few exceptional cases allow for more accurate measurements when planets transit in front of their host stars, providing additional data.