2026-07-072026-07-07http://salesiana.dossiersoluciones.com/handle/123456789/117217The luminosity of the famous red supergiant VY CMa (L ~ 4 - 5 x 10e5 Lsun) is well-determined from its spectral energy distribution and distance, and places it near the empirical upper luminosity limit for cool hypergiants. In contrast, its surface temperature is fundamentally ill-defined. Both contradict a recent paper by Massey, Levesque and Plez (2006). Implications for its location on the HR Diagram and its apparent size are discussed.5 pages, 1 figureAstrophysicsVY Canis Majoris: The Astrophysical Basis of Its Luminositytext