 Here we are zooming into LHA120N150, a star-forming region near the outskirts of the famous Torantula nebula in the Large Magellanic Cloud. This cloud of gas and dust, as well as the many young and massive stars surrounding it, is an excellent laboratory for studying the origins of massive stars. Theoretical models for the formation of massive stars suggest that they form within clusters of stars, but observations indicate that up to 10% of them formed in isolation. With the help of Hubble, astronomers are trying to find out whether the isolated stars visible in the nebula truly formed alone or just moved away from their original stellar grouping. However, such a study is not an easy task. Young stars, before they fully form, especially massive ones, look very similar to dense clumps of dust. This star-forming region contains several dozens of these objects. They are a mix of unclassified sources, some probably young stellar objects, and others probably dust clumps. Only detailed analysis and observations will reveal the true nature, and that will help to finally solve the unanswered question of the origin of massive stars.