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Titania's atmosphere is predominantly hydrogen with trace elements of nitrogen, oxygen, methane, ammonia and argon making up less than five percent of the total. It has a relative Jovian mass averaging 12.5, suggesting that it is close to that of a Y-type, or ultra-cool, brown dwarf; its physical size is actually five times [[Earth]]'s radii. | Titania's atmosphere is predominantly hydrogen with trace elements of nitrogen, oxygen, methane, ammonia and argon making up less than five percent of the total. It has a relative Jovian mass averaging 12.5, suggesting that it is close to that of a Y-type, or ultra-cool, brown dwarf; its physical size is actually five times [[Earth]]'s radii. | ||
It has an average surface temperature of 300 Kelvin, or a warm | It has an average surface temperature of 300 Kelvin, or a warm summer's day of approximately 80° Fahrenheit. It is colder towards the poles and warmer towards the equator, made possible by immense and violent windstorms that consume the planet. The planet's physical coloration is a brilliant sky-blue from Rayleigh scattering and has an albedo of 0.12. | ||
===Internal characteristics=== | ===Internal characteristics=== |