Further data adds weight to the dust outburst theory for explaining Betelgeuse’s dimming in 2019

An optical image of Betelgeuse taken in 2017 by a ground-based
telescope, showing its not unusual aspherical shape.
Click for original image.
Further analysis of the data gathered from Beteleguese during its unusual dimming in 2019 to 2020, has now strengthened the hypothesis that the dimming was caused by an outburst of dust from the star, creating a cloud that temporarily blocked its light.
Although the star as a whole appeared to darken, Betelgeuse’s photosphere seemed to actually brighten during the event. The Université Côte d’Azur astronomers say this observation is consistent with a likely theory, supported by observations, that Betelgeuse dimmed from our view due to a burst of dust, in the form of silicon monoxide, coming from the star. In turn, that burst might be related to a sudden cooling of the star’s surface.
“The changes in the structure of the photosphere and the silicon monoxide are consistent with both the formation of a cold spot on the star’s surface and the ejection of a cloud of dust,” the statement reads.
This new data also suggests that this dimming did not presage the star going supernova, but was simply part of the star’s normal fluctuations. Betelgeuse is essentially a giant gasbag that actually pulses not only in light but in shape. In a sense it behaves exactly like a blob of water floating in weightlessness.
An optical image of Betelgeuse taken in 2017 by a ground-based
telescope, showing its not unusual aspherical shape.
Click for original image.
Further analysis of the data gathered from Beteleguese during its unusual dimming in 2019 to 2020, has now strengthened the hypothesis that the dimming was caused by an outburst of dust from the star, creating a cloud that temporarily blocked its light.
Although the star as a whole appeared to darken, Betelgeuse’s photosphere seemed to actually brighten during the event. The Université Côte d’Azur astronomers say this observation is consistent with a likely theory, supported by observations, that Betelgeuse dimmed from our view due to a burst of dust, in the form of silicon monoxide, coming from the star. In turn, that burst might be related to a sudden cooling of the star’s surface.
“The changes in the structure of the photosphere and the silicon monoxide are consistent with both the formation of a cold spot on the star’s surface and the ejection of a cloud of dust,” the statement reads.
This new data also suggests that this dimming did not presage the star going supernova, but was simply part of the star’s normal fluctuations. Betelgeuse is essentially a giant gasbag that actually pulses not only in light but in shape. In a sense it behaves exactly like a blob of water floating in weightlessness.