Rogue Planets are Born in Young Star Clusters
Rogue planetary-mass objects, also known as free-floating planets (FFPs) drift through space alone, unbound to any other objects. They’re loosely defined as bodies with masses between stars and planets. There could be billions, even trillions of them, in the Milky Way. Their origins are unclear, but new research says they’re born in young star clusters. Some free-floating planets (FFPs) form the same way stars form by collapsing inside a cloud. The International Astronomical Union calls them sub-brown dwarfs. But that can’t account for all FFPs, or isolated planetary-mass objects (iPMOs) as they’re sometimes called. New research in Science Advances shows how FFPs form in young star clusters where circumstellar disks interact with one another. “This discovery partly reshapes how we view cosmic diversity.” Lucio Mayer, University of Zurich The research is titled “ Formation of free-floating planetary mass objects via circumstellar disk encounters. ” Zhihau Fu from the Departmen...