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Betelgeuse before, during and after the Great Dimming

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Betelgeuse before, during and after the Great Dimming


Orion and the molecular cloud masking the area. Betelgeuse is the purple star within the higher left. Credit score : Rogelio Bernal Andreo

When a outstanding star within the night time sky all of the sudden dims, it generates quite a lot of curiosity. That is what occurred with the purple supergiant star Betelgeuse between November 2019 and Could 2020. Betelgeuse will finally explode as a supernova. Was the dimming a sign that the explosion was imminent?

No, and new analysis helps clarify why.

Headline writers could not resist the supernova angle, though that rationalization was by no means very possible. Ultimately, it turned clear that ejected dust from the star triggered the dimming. New analysis based mostly on observations earlier than, throughout, and after the Nice Dimming Occasion (GDE) helps the concept that dust from the star itself triggered Betelgeuse’s drop in brightness.

A analysis letter titled “Photographs of Betelgeuse with VLTI/MATISSE throughout the Nice Dimming,” appearing in Month-to-month Notices of the Royal Astronomical Society: Letters, presents the infrared observations of Betelgeuse. The observations seize the star earlier than, throughout, and after the GDE. The lead creator is Julien Drevon, from the Université Côte d’Azur, France, and the European Southern College.

“To raised perceive the dimming occasion, we used mid-infrared long-baseline spectro-interferometric measurements of Betelgeuse taken with the VLTI/MATISSE instrument earlier than (Dec. 2018), throughout (Feb. 2020) and after (Dec. 2020) the GDE,” the analysis letter states. Particularly, their observations deal with silicon monoxide (SiO.)

The authors of the brand new analysis define three steps within the course of that created the GDE.

This determine from the analysis letter exhibits a number of the information the researchers labored with. The highest panel exhibits absolutely the spectra throughout every noticed epoch. The underside panel exhibits the relative flux for the SiO bands. The bands are deeper in the course of the GDE than both earlier than or after. Credit score: J. Drevon et al. 2024

The 1st step

The GDE began with shocks deep inside Betelgeuse. They generated a convective outflow of plasma that introduced materials to the star’s floor. Researchers detected a powerful shock in February 2018 and a weaker one in January 2019. The second, weaker shock boosted the impact of the stronger shock that preceded it, producing a progressive plasma circulation on the floor of Betelgeuse’s photosphere.

Step two

The plasma flowing to the photosphere’s floor created a sizzling spot. Hubble UV observations of Betelgeuse revealed the presence of a luminous, sizzling, dense construction within the star’s southern hemisphere, between the photosphere and the chromosphere.

Step three

Stellar materials detaches from the photosphere and types a fuel cloud above Betelgeuse’s floor. A colder area types underneath this cloud as a darkish spot. Because it’s cooler, dust is allowed to condense above this area and within the a part of the cloud above it. That dust is what blocked a few of Betelgeuse’s luminosity, inflicting the GDE.

Earlier analysis revealed this three-step course of behind the GDE. The authors of the brand new analysis article got down to observe Betelgeuse’s shut circumstellar atmosphere to probe and monitor its geometry. Within the wavelength range they labored in, SiO spectral options are outstanding, they usually’re used to know what occurred with the purple supergiant. In astronomy, SiO is used as a tracer for shocked fuel in stellar outflows because it persists at excessive temperatures.

This determine from the analysis article explains a few of what the researchers discovered. The center column is especially fascinating as a result of it’s a reconstruction of the SiO (2-0) absorption band onto Betelgeuse’s floor for every of the three noticed epochs. The third column is comparable however exhibits the SiO (2-0) optical depth. Total, they constrain the geometry of the dust function that triggered the GDE. Credit score: J. Drevon et al. 2024

Of their article, the authors deal with the SiO (2-0) band and what it signifies. They word how the band’s depth distinction will increase by 14% in the course of the GDE. “Subsequently, plainly in the course of the GDE, we observe brighter constructions within the line of sight,” they clarify.

Subsequent, they word a 50% lower in depth distinction in December 2020. What does it imply?

“The SiO (2–0) opacity depth map exhibits, subsequently, robust temporal variations inside two years, indicative of vigorous adjustments within the star’s atmosphere on this time span,” they write.

Their observations additionally counsel “the presence of an infrared extra within the pseudo continuum in the course of the GDE, which has been interpreted as new sizzling dust fashioned,” Drevon and his colleagues write.

It looks like the Nice Dimming is now not the thriller it as soon as was. It additionally exhibits that Occam’s Razor is alive and effectively: “The reason that requires the fewest assumptions is often appropriate.”

The supernova proposal was enjoyable for some time, and one day, Betelgeuse will explode as a supernova. However earlier than it ever does, there are possible going to be a number of extra episodes of dimming. For now, the authors say that the star is returning to regular.

“The Dec. 2020 observations counsel that Betelgeuse appears to be returning to a fuel and floor atmosphere just like the one noticed in Dec. 2018,” they write, “however with smoother constructions, possibly because of the uncommon quantity of dust just lately fashioned in the course of the GDE within the line of sight.”

Case closed?

Extra info:
J Drevon et al, Photographs of Betelgeuse with VLTI/MATISSE throughout the Nice Dimming, Month-to-month Notices of the Royal Astronomical Society: Letters (2023). DOI: 10.1093/mnrasl/slad138

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Quotation:
Betelgeuse earlier than, throughout and after the Nice Dimming (2024, February 1)
retrieved 1 February 2024
from https://phys.org/information/2024-02-betelgeuse-great-dimming.html

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