New theory helps explain and predict the activity of sun-like stars

March 23, 2016
It is easier to determine the age of star clusters than individual "field stars." For example, cluster NGC 1783 shown here is under one and a half billion years old — which is very young for globular clusters. The work by Blackman and Owen might ultimately lead to a new approach to determine a star's age. Image taken with the Advanced Camera for Surveys (ACS) on board the NASA/ESA Hubble Space Telescope.

Researchers have developed a new conceptual framework for understanding how stars similar to our Sun evolve. Their framework helps explain how the rotation of stars, their emission of x-rays, and the intensity of their stellar winds vary with time. According to first author Eric Blackman, professor of physics and astronomy at the University of Rochester, the work could also "ultimately help to determine the age of stars more precisely than is currently possible."

In a paper published today in Monthly Notices of the Royal Astronomical Society, the researchers describe how they have corroborated known, observable data for the of Sun-like stars with fundamental astrophysics theory. By looking at the physics behind the speeding up or slowing down of a star's rotation, its x-ray activity, and magnetic field generation, Blackman says the research is a "first attempt to build a comprehensive model for the activity evolution of these stars".

Using our Sun as the calibration point, the model most accurately describes the likely behavior of the Sun in the past, and how it would be expected to behave in the future. But Blackman adds that there are many stars of similar mass and radius, and so the model is a good starting point for predictions for these stars.

"Our model shows that stars younger than our Sun can vary quite significantly in the intensity of their x-ray emission and mass loss," said Blackman. "But there is a convergence in the activity of the stars after a certain age, so you could say that our Sun is very typical for stars of its mass, radius, and its age. They get more predictable as they age."

"We're not yet at the point where we can accurately predict a star's precise age, because there are simplifying assumptions that go into the model," said Blackman. "But in principle, by extending the work to relax some of these assumptions we could predict the age of for a wide range of stars based on their x-ray luminosity."

At the moment, empirically determining the age of stars is most easily accomplished if a star is among a cluster of stars, from whose mutual properties astronomers can estimate the age. Blackman explains that its age can then be estimated "to an accuracy not better than a factor of 25% of its actual age, which is typically billions of years." The problem is worse for "field stars," alone in space such that the cluster method of dating cannot be used. For these stars, astronomers have turned to "gyrochronology" and "activity" aging - empirically aging the stars based the fact that older stars of known age rotate more slowly and have lower x-ray luminosities than younger stars.

"Over the past few decades astronomers have been able to empirically measure these trends in rotation and magnetic activity for stars like the Sun, but Eric and his collaborators are trying to devise a comprehensive theoretical interpretation," said Eric Mamajek, professor of physics and astronomy at the University of Rochester and one of the astronomers leading the development of empirical methods for determining a star's age. "Ultimately this should lead to improved constraints on the evolution of rotation and activity in Sun-like , and better constraints on how the magnetic properties of our Sun have changed over the course of its main sequence life."

And this is where the developed by Blackman and his coauthor James E. Owen is important: it provides a physics explanation for how stellar rotation, activity, magnetic field, and mass loss all mutually evolve with .

"Only by tackling the entire problem of how stellar rotation, x-ray activity, and mass-loss mutually affect each other could we build a complete picture," said Owen, a NASA Hubble fellow at the Institute for Advanced Study, Princeton. "We find these processes to be strongly intertwined and the majority of previous approaches had only considered the evolution of one or two processes together, not the complete problem."

Explore further: Other suns got the right spin

More information: Eric G. Blackman et al. Minimalist coupled evolution model for stellar X-ray activity, rotation, mass loss, and magnetic field, Monthly Notices of the Royal Astronomical Society (2016). DOI: 10.1093/mnras/stw369

Related Stories

Other suns got the right spin

May 17, 2016

Astrophysicists from the Leibniz Institute for Astrophysics Potsdam (AIP) and the Johns Hopkins University in Baltimore have for the first time measured the rotation periods of stars in a cluster nearly as old as the sun ...

Rotational clock for stars needs recalibration

January 4, 2016

New work from a team of astronomers led by Carnegie's Jennifer van Saders indicates that one recently developed method for determining a star's age needs to be recalibrated for stars that are older than our Sun. This is due ...

The ages of sun-like stars

February 6, 2015

The mass of a star is perhaps its most significant feature. It determines how brightly it shines (a star ten times more massive than the Sun will, during its normal lifetime, shine about forty million times brighter than ...

Magnetic fields on solar-type stars

December 12, 2014

The Sun rotates slowly, about once every 24 days at its equator although the hot gas at every latitude rotates at a slightly different rate. Rotation helps to drive the mechanisms that power stellar magnetic fields, and in ...

X-ray emission from massive stars

October 26, 2015

Massive young stars are known to emit strong X-rays. Unlike the X-ray emission from lower mass stars, however, which arises in stellar photospheres, the X-rays from massive stars are thought to result from powerful shocks. ...

Recommended for you

Hubble catches a transformation in the Virgo constellation

December 9, 2016

The constellation of Virgo (The Virgin) is especially rich in galaxies, due in part to the presence of a massive and gravitationally-bound collection of over 1300 galaxies called the Virgo Cluster. One particular member of ...

Scientists sweep stodgy stature from Saturn's C ring

December 9, 2016

As a cosmic dust magnet, Saturn's C ring gives away its youth. Once thought formed in an older, primordial era, the ring may be but a mere babe – less than 100 million years old, according to Cornell-led astronomers in ...

Khatyrka meteorite found to have third quasicrystal

December 9, 2016

(Phys.org)—A small team of researchers from the U.S. and Italy has found evidence of a naturally formed quasicrystal in a sample obtained from the Khatyrka meteorite. In their paper published in the journal Scientific Reports, ...

0 comments

Please sign in to add a comment. Registration is free, and takes less than a minute. Read more

Click here to reset your password.
Sign in to get notified via email when new comments are made.