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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 97.4 light years: 0 % (0 from 9194 stars)
  • Average mass of Supergiants: 500-10000% solar mass
  • Average radius of Supergiants: 10000-100000% solar radius
  • Average temperature of Supergiants: 3000-35000 K

exoplanet iconSupergiants

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study iconNearest Supergiants

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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
Using the NuSTAR space telescope, researchers have performed a deep analysis of the X-ray binary 4U 1700-37, a system where a compact object—likely a neutron star—is pulling material from a massive supergiant star HD 153919. By studying the high-energy light emitted as this material falls toward the object, the team looked for 'cyclotron lines,' which act as a direct probe of a star's magnetic strength. While no rhythmic pulses were found, the study suggests the neutron star possesses a ...
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study iconResearch in Neutron stars

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