1st time measurement of Rotation Periods of Stars in Cluster nearly as old as the Sun

False-colour image of the stellar open cluster M67. Red, green, blue composite based on Johnson B, V and G bandpass images. Captured with WiFSIP/STELLA on Tenerife. Credit: AIP

It turns out these stars spin around once in ~26 days – just like our Sun. This discovery significantly strengthens what is known as the solar-stellar connection, a fundamental principle that guides much of modern solar and stellar astrophysics. This principle – that the Sun is a star – was only proved in the 19th century when distances to the nearest stars were measured. It enables us to use the Sun, the only star we can observe in detail, to study processes occurring on other stars, and conversely, to use other stars to infer the past and future of our Sun. Stellar rotation periods are a key probe of magnetic phenomena on stars.

The AIP/JHU team worked on the 4 billion year-old open cluster M67, the only accessible cluster of solar-aged stars. They measured the tiny periodic light variations of 20 Sun-like stars caused by starspots on the stellar surfaces being carried across the disk during rotation. Since the examined stars are quite old their starspots are relatively small – similar to spots one can find on our Sun but tiny compared to those visible on younger stars. The measurements were only possible because of the exquisite sensitivity of the Kepler Space Telescope, now repurposed as the K2 mission.

Sydney Barnes states: “We had predicted this would occur, but it has been a real privilege to have been able to actually make the measurements.” Co-author Jörg Weingrill adds: “With the measured rotational periods for stars up to the age of our Sun we can now confidently trace back the evolution of our home star.” http://www.aip.de/en/news/press/m67