jedion357 June 25, 2023 - 11:32pm | Cannon Material
Radiation hazard[edit]Despite K-stars' lower total UV output, in order for their planets to have habitable temperatures, they must orbit much near to their K-stars hosts, offsetting or reversing any advantage of a lower total UV output. There is also growing evidence that K-type dwarf stars emit dangerously high levels of X-rays and far ultraviolet (FUV) radiation for considerably longer into their early main sequence phase than do either heavier G-type stars or lighter early M-type dwarf stars.[12] This prolonged radiation saturation period may be sterilising, destroying the atmospheres of, or at least delaying the emergence of life for Earth-like planets orbiting inside the habitable zones around K-type dwarf stars
A K-type star's habitable zone approximately ranges between 0.1–0.4 to 0.3–1.3 AU from the star. Here, exoplanets will receive only a relatively small amount of ultraviolet radiation, especially so towards the outer edge. Pi'Ka'Nair orbit: 0.2 AU T'Zaan orbit: 1.2 Au
Pi'Ka'Nair is warmer and T'Zaan is cooler Note to self: compute a 1 AU journey between the two inhabited planets I might not be a dralasite, vrusk or yazirian but I do play one in Star Frontiers! |