During each iteration of its fierce and familiar 11-year cycle of activity, the turbulent surface of the sun reaches a crescendo, shooting jets of scalding gas and magnetic energy into space at a markedly increased rate. For the first time, astronomers have made continuous, long-term observations of such flare activity on stars outside the solar system, and they’ve found that the stars have cycles of activity and quiescence similar to those of the sun.
At the National Radio Astronomy Observatory in Green Bank, W. Va., Mercedes Richards and her colleagues from Pennsylvania State University in State College recorded radio waves from flares spewing from two nearby star systems, Beta Persei and V711 Tauri. Both include binary pairs–two stars orbiting one another. These systems are close by, which makes them easy to observe, and they’re known to have strong flaring activity. With observations made up to six times a day for 5 years, the team built up a far more comprehensive picture of the stars’ behavior patterns than previous studies had.