Betelgeuse (Alpha Orionis)
node · earth · Constellation Orion, as seen from Earth
The nearest red supergiant to the Sun and the clearest available example of a massive star in its final phase. Joyce and colleagues (2020) combined asteroseismic, evolutionary and hydrodynamic modelling of its 400-day pulsation to derive a mass of about 16.5 to 19 solar masses, a radius near 764 solar radii and a distance near 168 parsecs - about 548 light-years - and concluded that it is burning helium in its core with on the order of 100,000 years to go. Between October 2019 and March 2020 it faded by more than a magnitude in the visible in the episode known as the Great Dimming; imaging and modelling published in Nature in 2021 attributed it to a dust clump condensing above a cooled patch of the photosphere following a surface mass ejection. In 2025 a probable direct detection of a close stellar companion of roughly 1.5 solar masses was reported from speckle imaging, resolving a long-standing anomaly in its brightness variations. Not a place on Earth.
Read in · 1
Evidence · 3
Timeline
No dated observations are stored for this object. Atlas shows what was observed and when — it does not infer a history.
Connections · 1
- Red giant and asymptotic giant branchinstance_of
Assembled narrative · 1
Assembled from 18 blocks · 3 evidence · 17 related
- Story
- The nearest red supergiant to the Sun and the clearest available example of a massive star in its final phase. Joyce and colleagues (2020) combined asteroseismic, evolutionary and hydrodynamic modelling of its 400-day pulsation to derive a mass of about 16.5 to 19 solar masses, a radius near 764 solar radii and a distance near 168 parsecs - about 548 light-years - and concluded that it is burning helium in its core with on the order of 100,000 years to go. Between October 2019 and March 2020 it faded by more than a magnitude in the visible in the episode known as the Great Dimming; imaging and modelling published in Nature in 2021 attributed it to a dust clump condensing above a cooled patch of the photosphere following a surface mass ejection. In 2025 a probable direct detection of a close stellar companion of roughly 1.5 solar masses was reported from speckle imaging, resolving a long-standing anomaly in its brightness variations. Not a place on Earth.
- Knowledge
- Betelgeuse (Alpha Orionis)
- Red giant and asymptotic giant branch
- Connections
- Red giant and asymptotic giant branch
- Betelgeuse fades by more than a magnitude
- A close companion to Betelgeuse is probably detected
- Main sequence (core hydrogen burning)
- Betelgeuse (Alpha Orionis)
- Planetary nebula
- White dwarf
- Betelgeuse fades by more than a magnitude
- Evidence
- Supports a mass of about 16.5-19 solar masses, a radius near 764 solar radii, a distance near 168 parsecs and core helium burning with roughly 100,000 years remaining. All figures come from a search summary of secondary reporting; the paper was not fetched and the distance remains uncertain at roughly the ten-per-cent level.
- Attributes the 2019-2020 Great Dimming to a dust clump condensing above a cooled patch of the photosphere. Journal and volume come from search summaries; the paper was not fetched. Later work, including a 2022 Astrophysical Journal paper describing a surface mass ejection and 2024 tomography, indicates temperature drop and dust extinction contributed in comparable measure.
- Reports speckle-imaging observations with 'Alopeke on Gemini North in 2020 and 2024 yielding a probable detection of a companion of roughly 1.5 solar masses at the predicted separation and position angle. Title, DOI and arXiv identifier come from publisher and preprint listings via search; neither the paper nor the NOIRLab release could be fetched (both domains blocked). The word "probable" is the authors' own and is retained here.
Observed changes · 0
No public Signals are attached to this object. Signals show what changed and when it was observed — never a direction or a rank.
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