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HandWiki. List of Largest Stars. Encyclopedia. Available online: https://encyclopedia.pub/entry/35508 (accessed on 11 September 2026).
HandWiki. List of Largest Stars. Encyclopedia. Available at: https://encyclopedia.pub/entry/35508. Accessed September 11, 2026.
HandWiki. "List of Largest Stars" Encyclopedia, https://encyclopedia.pub/entry/35508 (accessed September 11, 2026).
HandWiki. (2022, November 21). List of Largest Stars. In Encyclopedia. https://encyclopedia.pub/entry/35508
HandWiki. "List of Largest Stars." Encyclopedia. Web. 21 November, 2022.
List of Largest Stars
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Below is a list of the largest stars currently known, ordered by radius. The unit of measurement used is the radius of the Sun (approximately 695,700 km; 432,300 mi). The angular diameters of stars can be measured directly using stellar interferometry. Other methods can use lunar occultations or from eclipsing binaries, which can be used to test indirect methods of finding stellar radii. Only a few useful supergiant stars can be occulted by the Moon, including Antares A (Alpha Scorpii A). Examples of eclipsing binaries are Epsilon Aurigae (Almaaz), VV Cephei, and V766 Centauri (HR 5171). Angular diameter measurements can be inconsistent because the boundary of the very tenuous atmosphere (opacity) differs depending on the wavelength of light in which the star is observed. Uncertainties remain with the membership and order of the list, especially when deriving various parameters used in calculations, such as stellar luminosity and effective temperature. Often stellar radii can only be expressed as an average or be within a large range of values. Values for stellar radii vary significantly in different sources and for different observation methods. All the sizes stated in this list have various inaccuracies and may be disputed. This list is still a work in progress and various parameters are extremely disputed.

eclipsing binaries luminosity interferometry

References

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  3. Methods for calculating the radius: AD: radius determined from angular diameter and distance L/Teff: radius calculated from bolometric luminosity and effective temperature DSKE: radius calculated using the disk emission EB: radius determined from observations of the eclipsing binary
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