I've heard the Sun's habitable zone is approximately from the orbit of Venus to the orbit of Mars.
The sun-like star Beta Comae Berenices has a listed habitable zone from 0.918–1.042 AU even though it has a luminosity of 1.357 ± 0.014[7] L☉. It seems like if a star was more luminous that it's habitable zone would be further away however those distances are nearly the same as the Sun's.
(https://en.m.wikipedia.org/wiki/Beta_Comae_Berenices)
Is the radius of the habitable zone not directly related to the luminosity of a star or is it just more complicated than that?
I was hoping to be able to determine the radius of the habitable zones for these sun-like stars:
https://en.m.wikipedia.org/wiki/HR_511
https://en.m.wikipedia.org/wiki/Beta_Canum_Venaticorum
https://en.m.wikipedia.org/wiki/Sigma_Draconis
The sun-like star Beta Comae Berenices has a listed habitable zone from 0.918–1.042 AU even though it has a luminosity of 1.357 ± 0.014[7] L☉. It seems like if a star was more luminous that it's habitable zone would be further away however those distances are nearly the same as the Sun's.
(https://en.m.wikipedia.org/wiki/Beta_Comae_Berenices)
Is the radius of the habitable zone not directly related to the luminosity of a star or is it just more complicated than that?
I was hoping to be able to determine the radius of the habitable zones for these sun-like stars:
https://en.m.wikipedia.org/wiki/HR_511
https://en.m.wikipedia.org/wiki/Beta_Canum_Venaticorum
https://en.m.wikipedia.org/wiki/Sigma_Draconis