A team of astronomers has determined how the gas flow from a massive infant star is launched. The researchers used the Atacama Large Millimeter/submillimeter Array (ALMA) to observe the 10-solar-mass protostar ‘Orion KL Source I’ in the Kleinmann-Low Nebula and obtained clear evidence of rotation in the outflow. Artist’s impression of Orion KL Source I. The massive protostar is surrounded by a disk of gas and dust. The outflow is launched from...