Young star clusters give birth to rogue planetary-mass objects
Planetary-mass objects (PMOs) are cosmic nomads: they drift freely through space, unbound to any star, and weigh less than 13 times the mass of Jupiter. While they have been spotted in abundance in young star clusters such as the Trapezium Cluster in Orion (Fig. 1), their origin has puzzled scientists. Traditional theories have suggested that they might be failed stars or planets ejected from their solar systems. An international team of astronomers, in collaboration with the University of Zurich (UZH), has used advanced simulations to demonstrate that these enigmatic objects can form directly from the violent interactions of disks around young stars. “PMOs don’t ...
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