Various issues exist in determining accurate radii of the largest stars, which in many cases do display significant errors. The following lists are generally based on various considerations or assumptions; these include: • Stellar radii or diameters are usually derived only approximately using the
Stefan–Boltzmann law for the deduced stellar
luminosity and
effective surface temperature. •
Stellar distances, and their errors, for most stars, remain uncertain or poorly determined. • Many extended supergiant atmospheres also significantly change in size over time, regularly or irregularly pulsating over several months or years as
variable stars. This makes adopted
luminosities poorly known and may significantly change the quoted radii. • Other direct methods for determining stellar radii rely on lunar
occultations or from eclipses in binary systems. This is only possible for a very small number of stars. • Many distance estimates for red supergiants come from stellar cluster or association membership, because it is difficult to calculate accurate distances for red supergiants that are not part of any cluster or association. • In these lists are some examples of extremely distant extragalactic stars, which may have slightly different properties and natures than the currently largest known stars in the
Milky Way. For example, some red
supergiants in the
Magellanic Clouds are suspected to have slightly different limiting
temperatures and
luminosities. Such stars may exceed accepted limits by undergoing large eruptions or changing their
spectral types over just a few months (or potentially years). ==Lists==