The Leclerc System and Bayard

I'm still in the process of defining much of this and it's subject to change, but my current thinking is that the Leclerc system constitutes the following planets: Corbarans: A hot, rocky, vacuum planet Bertrand: A proto-Venus Fierebras: A hot planet with a tar-like fluid covering the surface Bayard: The inhabited planet Otuel: A small Jovian Aigar: An icy, vacuum rockball These planets orbit a K0V star with .76 of the mass of Sol and nearly half its luminosity and cooler, coming in at 5,062K. (FYI, I haven't yet determined which system of the Wolf cluster Leclerc actually is--I do know I'll override one of those...probably one of these: Ross 486, DM+0 2898, or Gamma Virginis.) Bayard sits at .66 AU from Leclerc and has a diameter of 11,203.2km (6,961.3miles). The planet rotates slowly compared to Earth. One Bayard day is 1,572 hours or 65.5 Earth days, and it orbits Leclerc every 9 days (or 216 Earth days). Its axial tilt is 27.35%. The atmosphere consi...