Home Technology News Sci-Tech நட்சத்திர ‘கிளிச்சிங்’ தொடர்பான புதிய தடயங்களை வானியலாளர்கள் கண்டுபிடித்துள்ளனர்

நட்சத்திர ‘கிளிச்சிங்’ தொடர்பான புதிய தடயங்களை வானியலாளர்கள் கண்டுபிடித்துள்ளனர்

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நட்சத்திர ‘கிளிச்சிங்’ தொடர்பான புதிய தடயங்களை வானியலாளர்கள் கண்டுபிடித்துள்ளனர்

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எரியும் நட்சத்திரம் சூரியன் விண்வெளி விளக்கம்

சிவப்பு ராட்சதர்கள் உட்புற மையத்தில் பெரிய அளவிலான கட்டமைப்பு மாறுபாடுகள் அல்லது “குறைபாடுகளை” அடிக்கடி அனுபவிக்கும் புதிய அறிகுறிகளை ஆராய்ச்சியாளர்கள் கண்டுபிடித்துள்ளனர்.

சமீபத்திய கண்டுபிடிப்புகள் கணிசமான எண்ணிக்கையிலான நட்சத்திரங்கள் அவற்றின் மையங்களில் முறைகேடுகளை வெளிப்படுத்துகின்றன என்பதைக் காட்டுகின்றன.

வானத்தில் உள்ள பிரகாசமான நட்சத்திரங்கள் சிலவற்றின் உள் செயல்பாடுகளை ஆய்வு செய்யும் முறையை விஞ்ஞானிகள் கண்டுபிடித்துள்ளனர்.

சர்வதேச ஆராய்ச்சியாளர்களின் குழு, தரவைப் பயன்படுத்துகிறது[{” attribute=””>NASA’s Kepler space telescope, has uncovered new evidence that red giants – stars that have reached the end of their lifecycle and have depleted their hydrogen supply – frequently experience significant structural variations, or “glitches,” deep within their inner core.

The stellar glitches popularized in the media have to do with a star’s rotation, but lead author Mathieu Vrard studies a different kind of defect. The glitches in this study can affect a star’s oscillations or the frequencies and paths that sound waves travel when passing through a star.

Red clump stars, helium-core burning objects, are often used in astrophysical studies as probes of distance to measure aspects like galaxy density and to learn more about the physical processes behind stellar chemical evolution. So it’s vital that scientists understand why these discontinuities happen, said Vrard, a postdoctoral research associate in astronomy at the Ohio State University.

“By analyzing these variations, we can use them to obtain not only the global parameters of the star but also information on the precise structure of those objects,” he said.

The study, recently published in the journal Nature Communications is the first to perform detailed observational characterizations on the deepest layers of these red giants.

In order to determine if these glitches were becoming more prevalent across certain star groups, the team selected a sample of 359 red giants that were below a certain stellar mass, and measured various properties and individual frequencies of each star.

The team found proof that 24 of the red giants surveyed (about 7% of those in the sample) had experienced intermittent structural discontinuities at one point or another during their lifetime. While 7% may not seem like much, if applied to all of the known stars in our universe, the number of stars that have these irregularities would be enormous.

There are two main theories that explain how these disturbances might work. The first scenario posits that glitches are present throughout the star’s evolution, but are generally very weak and below the threshold for what astronomers would categorize as a true discontinuity.

The second suggests that irregularities are “smoothed out” by some unknown physical process that later leads to changes in the structure of the star’s core.

As it turns out, the first scenario is not supported by this study’s model, which predicts that glitches observed are actually a common occurrence, but more precise data is needed before scientists can confidently subscribe to the second.

“What we think is that the second theory might hold up better because the first one didn’t make sense with our observations,” Vrard said.

As the study offers a better characterization of the physical processes taking place inside red-giant stars, Vrard’s work could potentially have large implications for the field of asteroseismology – a branch of astronomy that studies the internal composition of stars using the oscillations of sound waves – and for galactic archaeology, a field that uses detailed stellar fossil records to uncover the history of the universe.

And though Vrard’s current analysis has come to an end, he aims to build on the scientific community’s knowledge of red-giant stars by examining more precise data that could help cultivate even more refined stellar models.

Reference: “Evidence of structural discontinuities in the inner core of red-giant stars” by Mathieu Vrard, Margarida S. Cunha, Diego Bossini, Pedro P. Avelino, Enrico Corsaro and Benoît Mosser, 16 December 2022, Nature Communications.
DOI: 10.1038/s41467-022-34986-z

The study was funded by NASA and the European Regional Development Fund.



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