Blue and white supergiants are high luminosity stars somewhat cooler than the most luminous main sequence stars. A star like Deneb, for example, has a luminosity around 200,000 L ⊙, a spectral type of A2, and an effective temperature around 8,500 K, meaning it has a radius around 203 R ☉ (1.41 × 10 m). For comparison, the red supergiant Betelgeuse has a luminosity around 100,000 L ⊙, a spectral type of M2, and a temperature around 3,500 K, meaning its radius is about 1,000 R ☉ (7.0 × 10 m). Red supergiants are the largest type of star, but the most luminous are much smaller and hotter, with temperatures up to 50,000 K and more and luminosities of several million L ⊙, meaning their radii are just a few tens of R ⊙. For example, R136a1 has a temperature over 46,000 K and a luminosity of more than 6,100,000 L ⊙ (mostly in the UV), it is only 39 R ☉ (2.7 × 10 m).