Older stars rotate faster than expected

Not only humans lose mobility in old age – stars also rotate more slowly then. All stars are born with angular momentum that comes from the rotation of the protostellar cloud. Then, as they get older, their rotation slows in a process called «magnetic braking.» A study published in 2016 by scientists at Carnegie Observatories provided the first evidence that stars at a similar stage of life as the Sun are spinning faster than magnetic braking theories predict. The results of that study were based on a method in which scientists locate dark spots on the surface of stars and track how they move with the stars’ spin. However, while the method has proven robust for measuring angular momentum in younger stars, older stars have fewer stellar spots, which made the effects of this attenuated magnetic braking on these stars difficult to confirm.

In a new study published in Nature Astronomy, researchers at the University of Birmingham used a different approach to confirm that older stars do indeed appear to rotate faster than expected. The team used asteroseismology to calculate how the star rotates. This relatively new field of research allows scientists to measure the vibrations that cause sound waves trapped inside the star. By measuring the different properties of these waves, scientists can reveal certain characteristics of stars, such as their size or age.

In this particular study, the team measured the frequencies of the sound waves produced by the star’s oscillation. As the star rotates, these split into different frequencies. According to the authors, this can be thought of as the sound of two ambulances standing on a traffic circle versus when they are driving in circles. By measuring these frequencies, it is possible to calculate the rate of rotation, for both young and old stars.

One aspect that researchers believe may be key to the change in momentum loss is changes in the star’s magnetic field. Understanding how the magnetic field interacts with rotation will be an important area for future study and is being addressed by the study authors.

The results could also shed light on the activity of our own star over the next billion years, explains co-author Dr. Guy Davies: «These new findings show that we still have much to learn about the future of our own Sun and other stars. This work helps put into perspective whether or not we should expect lower solar activity and harmful space weather in the future. To answer these questions, we need better models of solar rotation, and this work is an important step in improving the models and providing the data needed to test them.»

Sound waves trapped inside stars cause them to vibrate at specific frequencies. These oscillations are visible on the surface and can be measured by astronomers using space telescopes. As a star rotates, these oscillation frequencies change slightly, so it is possible to measure the star’s rotation by looking at how its surface changes over time. The study of these oscillations (called asteroseismology) can also be used to measure properties such as the mass and age of a star. This allows us to understand more precisely how the rotation and activity of stars evolve over time, improving our understanding of stars, exoplanet systems and our own solar system. (Image: Mark Garlick / University of Birmingham)

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  • BrandonQMorris
  • Brandon Q. Morris es físico y especialista en el espacio. Lleva mucho tiempo preocupado por las cuestiones espaciales, tanto a nivel profesional como privado, y aunque quería ser astronauta, tuvo que quedarse en la Tierra por diversas razones. Le fascina especialmente el "qué pasaría si" y a través de sus libros pretende compartir historias convincentes de ciencia ficción dura que podrían suceder realmente, y que algún día podrían suceder. Morris es autor de varias novelas de ciencia ficción de gran éxito de ventas, como la serie Enceladus.

    Brandon es un orgulloso miembro de la Science Fiction and Fantasy Writers of America y de la Mars Society.