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Sun-like stars
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Sun-like stars

Sun-like stars are yellow dwarfs on the main sequence. Imagine our solar system as a standard model: these stars have similar mass, temperature, and luminosity to our Sun. In their cores, thermonuclear fusion of hydrogen into helium occurs, providing stability for billions of years. They are ideal candidates for seeking habitable planets because they provide a steady source of energy and heat, much like the engine at the center of our own home. Their surface temperature ranges from about 5,000 to 6,000 degrees Celsius, giving them their characteristic yellowish glow.
  • Percentage of Sun-like stars within 98.5 light years: 4.11 % (391 from 9520 stars)
  • Average mass of Sun-like stars: 80-120% solar mass
  • Average radius of Sun-like stars: 80-120% solar radius
  • Average temperature of Sun-like stars: 5200-6000 K

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Latest news from Sun-like stars

Thick-disk stars identified as hosts to ancient hot jupiter planets
iconToday
iconStars | Exoplanets | Sun-like stars | Hot Jupiter | Planet formatio
Image: Thick-disk stars identified as hosts to ancient hot jupiter planets
Large gas giant planets that orbit very close to their parent stars are known as hot Jupiters. By analyzing a sample of 268 stars, researchers have identified several hot Jupiters orbiting stars belonging to the high-alpha thick disk of our galaxy. The thick disk represents a component of the Milky Way containing older stars with specific chemical signatures, particularly higher amounts of alpha elements like magnesium, silicon, and calcium relative to iron. These systems are significantly older...
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Atmospheric differences between morning and evening sides of planet WASP-39 b revealed
icon12. 10. 2026
iconStars | Exoplanets | Sun-like stars | Hot Jupiter | Planetary atmosphere
Image: Atmospheric differences between morning and evening sides of planet WASP-39 b revealed
Observations of the hot Jupiter WASP-39 b reveal significant differences between its morning and evening atmospheres. Climate models successfully match temperature patterns but still struggle to explain the observed asymmetry in carbon dioxide levels....
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Water vapor detected in the atmosphere of ultrahot Neptune LTT 9779 b
icon9. 10. 2026
iconStars | Exoplanets | Sun-like stars | Planetary atmosphere
Image: Water vapor detected in the atmosphere of ultrahot Neptune LTT 9779 b
New observations of the ultrahot Neptune LTT 9779 b reveal the presence of water vapor on its dayside. The planet shows no signs of thermal inversion or significant atmospheric escape, supporting the theory that it is a tidally locked world....
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Leave-one-out cross-validation provides clarity in radial velocity measurements of exoplanetary systems
icon7. 10. 2026
iconStars | Exoplanets | Sun-like star
Image: Leave-one-out cross-validation provides clarity in radial velocity measurements of exoplanetary systems
New statistical analysis refines planetary data. By checking the influence of individual measurements, researchers revised the mass of HD 119130 b, clarified the orbit of Gliese 4276, and confirmed the three-planet system orbiting Gliese 357....
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Improved atmospheric analysis of WASP-39 b using radius-augmented data processing
icon5. 10. 2026
iconStars | Exoplanets | Sun-like star
Image: Improved atmospheric analysis of WASP-39 b using radius-augmented data processing
New research shows that the atmospheric analysis of WASP-39 b was limited by missing radius data. By incorporating the planet's radius into models, researchers have achieved a highly accurate fit for James Webb Space Telescope data. #Exoplanets #WASP39b #JWST...
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