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Supergiants
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Supergiants

Supergiants are the most massive and luminous stars in the universe. Imagine that if the Sun were a pea, a red supergiant would fill the space all the way to Jupiter's orbit. Blue supergiants (classes O, B) are extremely hot, young, and massive stars that burn fuel rapidly. Yellow supergiants (classes F, G) represent a brief transitional phase. Red supergiants (class M) are cooler but emit vast amounts of energy due to their immense surface area. A key relation exists: the higher the mass, the higher the core temperature and pressure, leading to greater size, luminosity, and a violent end as a supernova.
  • Percentage of Supergiants within 98.5 light years: 0 % (0 from 9522 stars)
  • Average mass of Supergiants: 500-10000% solar mass
  • Average radius of Supergiants: 10000-100000% solar radius
  • Average temperature of Supergiants: 3000-35000 K

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Latest news from Supergiants

Observations reveal evidence of a potential stellar companion for the red supergiant Betelgeuse
icon4. 8. 2026
iconStars | | | Supergi
Image: Observations reveal evidence of a potential stellar companion for the red supergiant Betelgeuse
Betelgeuse, one of the most prominent red supergiant stars in the night sky, has long been a subject of intense scientific inquiry. Recent analysis has sought to verify the existence of a secondary star orbiting this massive primary. By examining the star’s long secondary period of variability, which suggested the presence of an orbiting body, researchers targeted the system to confirm if a companion star was indeed present in the vicinity of this stellar giant. Using extreme adaptive optic...
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Probing the magnetic field of a mysterious neutron star in a massive binary system
icon15. 2. 2026
iconStars | NuSTAR | Supergiants | Neutron star
Image: Probing the magnetic field of a mysterious neutron star in a massive binary system
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study iconResearch in Neutron stars

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