I will discuss the birth of stars. Stars form from the gravitational collapse of small “cores” deep inside giant molecular clouds. Since these clouds are opaque at optical wavelengths, the observations of these collapsing “protostars” must be conducted at radio and infrared wavelengths, where the clouds are more transparent. I will show how the observations reveal the various stages of star formation, from “starless cores,” though “hot cores,” and eventually, young stars. I will pay special attention to the most massive stars, whose origins are especially difficult to understand. A byproduct of this process is the origin of planets, and I will discuss some of the observational evidence that shows young solar systems in the process of formation.