M
Malenfant
Guest
LGG and SGG does that quite nicely actually. 160,000 km diameter (80k km radius) seems to be the highest you can get for gas giants anyway, after that the radius stays about the same and they get denser as you add more mass.
Canonically (p39, CT bk 6) SGG are 20k to 60k km in radius, and LGG are larger than that (up to 120k km radius, which is just silly - you can't get them that big). Note that by this definition, Saturn is actually an SGG, not an LGG - its polar radius is just over 60k km, and its equatorial radius is 54k ( http://nssdc.gsfc.nasa.gov/planetary/factsheet/saturnfact.html ).
The line between terrestrials and SGG is blurry. If a terrestrial is massive enough to hold onto hydrogen and helium, it can become a GG - and that depends on its density, radius, and distance from the star. A world with earthlike density in the habitable zone can hold onto helium around size A, and hydrogen around size C.
Canonically (p39, CT bk 6) SGG are 20k to 60k km in radius, and LGG are larger than that (up to 120k km radius, which is just silly - you can't get them that big). Note that by this definition, Saturn is actually an SGG, not an LGG - its polar radius is just over 60k km, and its equatorial radius is 54k ( http://nssdc.gsfc.nasa.gov/planetary/factsheet/saturnfact.html ).
The line between terrestrials and SGG is blurry. If a terrestrial is massive enough to hold onto hydrogen and helium, it can become a GG - and that depends on its density, radius, and distance from the star. A world with earthlike density in the habitable zone can hold onto helium around size A, and hydrogen around size C.