A world staff of astronomers, led by a researcher from the College of Geneva (UNIGE), has proven that the sun’s magnetic exercise has a big affect on its seismic characterization, opposite to predictions in earlier research. Necessary information resembling its dimension, age and chemical composition depend upon it.
These outcomes pave the way in which for in-depth analysis to higher perceive the character of the magnetic exercise and its influence on stellar oscillations. The research is published within the journal Astronomy & Astrophysics.
Asteroseismology, or helioseismology within the case of the sun, is an interesting department of astronomy that research the oscillations of stars.
“To know it, you will need to think about a star as an enormous ball of fuel in fixed movement. Inside this star, there are waves or pulsations that make it vibrate, somewhat just like the sound that resonates in a musical instrument,” explains Jérôme Bétrisey, a postdoctoral researcher within the Astronomy Division of the School of Science on the UNIGE and first writer of the research.
“These vibrations trigger the star’s floor to maneuver barely and alter luminosity recurrently. Due to very exact devices, we are able to detect these variations in luminosity from Earth or from space,” continues the researcher.
Listening to the symphony of the celebs
By observing these modifications, researchers can be taught a fantastic deal concerning the star’s inside construction and decide essential traits resembling its dimension, age, chemical composition or stage within the stellar life cycle. A exact understanding of the traits of stars is crucial, amongst different issues, to find out the properties of the planets that encompass them or to retrace the historical past of the Milky Way.
Regardless of some main successes in latest many years, asteroseismology has additionally proven that there are important variations between observations and the predictions of theoretical fashions of the interior workings of stars.
Over time, numerous strategies have been developed to scale back these discrepancies, with various levels of success. Nevertheless, none of the present strategies contemplate the magnetic exercise of stars, its influence on the outcomes being imagined to be negligible.
The worldwide staff led by Bétrisey has simply demonstrated the alternative. It has established that the age of the sun, as decided by helioseismology, varies considerably in response to the extent of exercise of the solar cycle.
To provide an order of magnitude, the sun is round 4.6 billion years outdated, and variations of as much as 300 million years have been noticed between solar minima. Though these variations could seem small in contrast with the age of the sun, they’re not negligible given the extent of precision that shall be achieved by future space missions.
Seismic age of sun correlates with the solar exercise cycle
To raised perceive the influence of magnetic exercise on the sun, the scientists analyzed 26.5 years of solar information, protecting two full exercise cycles. They divided this information into about 90 small one-year sequence, every three months aside. For every of those sequence, a seismic evaluation was carried out, making it potential to measure the evolution of the sun’s elementary properties resembling its mass, radius and age over time.
Two impartial information units have been used to verify the robustness of the outcomes. One got here from the College of Birmingham’s BiSON (Birmingham Photo voltaic Oscillations Community) community of ground-based telescopes, and the opposite from the GOLF (International Oscillations at Low Frequencies) instrument on board the SOHO (Photo voltaic and Heliospheric Observatory) satellite, which has been orbiting the sun because the mid-Nineties.
Whatever the configuration examined, the age of the sun decided by helioseismology was correlated with the extent of exercise of the solar cycle. They measured variations of round 6% on common between the intervals of solar minimal and most, which may be very important by way of the precision focused for future space missions that can analyze different comparable stars.
For instance, the PLATO (PLAnetary Transits and Oscillations of stars) mission is aiming for a precision of 10% for the age of a star just like the sun.
The research of the GOLF and BiSON information additionally confirmed that the influence of the exercise cycle on the seismic age is extra marked for the extra lively of the 2 cycles studied. This result’s logical and anticipated from a bodily perspective.
“Nevertheless, the sun isn’t a very lively star, which means that the influence of magnetic exercise might be very important for extra lively stars resembling people who PLATO will detect,” provides Bétrisey.
Extra info:
J. Bétrisey et al, Imprint of the magnetic exercise cycle on solar asteroseismic characterisation primarily based on 26 years of GOLF and BiSON information, Astronomy & Astrophysics (2024). DOI: 10.1051/0004-6361/202451365
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University of Geneva
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Scientists present the sun’s magnetic exercise influences the willpower of its seismic age (2024, August 19)
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