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Betelgeuse

AstronomyPhysics

Betelgeuse (Alpha Orionis) is a red supergiant in the constellation Orion and one of the brightest stars in the night sky. As a supernova candidate it is a focus of astrophysics research.

astronomy.stars

Metrics

Category

Red Supergiant (M2Iab)High

Spektralklasse M1-2 Ia-ab.

Diameter

~890,000,000 – 1,065,000,000kmMedium

Approx. 640–764 solar radii. Placed in the Solar System, its surface would extend beyond the orbit of Mars.

Mass

~14–19M☉Medium

Current mass in solar masses. Initial mass estimated at 18–21 M☉.

Surface Temperature

3’500KMedium

Effective temperature approx. 3,250–3,690 K.

Relations

Compares toSunMedium

Betelgeuse has 640–764 times the radius of the Sun and 100,000 times its luminosity.

Factor: 700 Sonnenradien · Direction: A_gt_B

Explanations

Draft

Betelgeuse (Alpha Orionis) is a red supergiant in the constellation Orion and one of the brightest stars in the night sky. With a diameter of about 890 to 1,065 million kilometers, it is roughly 700 times larger than our Sun, even though it's only 14–19 times more massive. Its surface temperature of 3500 K gives it a red colour, and it radiates about 100,000 times more light than the Sun. Astrophysicists watch it closely because it's considered a supernova candidate that could explode at any time.

Generated by: claude-haiku-explanation-agent · claude-haiku-4-5-20251001

Sources

NASA Science — What is Betelgeuse?reference
https://science.nasa.gov/universe/what-is-betelgeuse-inside-the-strange-volatile-star/

NASA-Überblick zu Beteigeuze mit physikalischen Daten und Supernova-Prognose.

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Provenance

Status

seed

Review

none

Last Updated

2026-02-17

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