Initial thoughts on the updated Alpha Centauri B add-on
Posted: 14.04.2005, 23:59
Hi folks...
I'm beginning to sketch out my entry for the Toliman (Alpha Centauri B) System, and thought I'd run them by you. Once I get a generalized idea of what I want, I'll start on the ssc file(s).
PLANET I: Baahki is a lower-massed world kept geologically active by the massive tidal stretching produced by its large (approximately half the diameter of Baahki itself), volcanically active moon. The second and smaller moon, while further out, also adds something to this effect. While the planet has no tectonic plates, volcanic activity and erosion slowly changes the surface over tens of millions of years.
PLANET II: Eutresca is a smaller, rocky world, heavity cratered. It is similar to Mercury in that it is quite dense for its small size.
PLANET III: Mephinos is Mars-like, with polar caps of water and carbon dioxide ice, and a cold and dry surface composed of rocky, cratered highlands and relatively smooth, nearly featureless lowlands. There are a number of very obvious dry river channels on the surface, along with corresponding erosional land forms, and many of these channels extend for hundreds of miles. Clearly, Mephinos was once quite wet. Today, as ide from some deep subsurface hot spots, it is largely geologically inert. It possesses two moons, one of which is a very small cratered ball, while the outer moon is a captured, irregular asteroid.
PLANET IV: NESSOS: This is a Panthalassic world, and the most masive planet orbiting either of the stars of the greater Alpha Centauri System. It has a substantial ring system, and a single large and cratered moon.
Thoughts are more than welcome. My biggest concern is the set up of Baahki and its moons, this world being the primary planet of interest for the system. I really like the idea of a planet being kept geologically active and habiutable due to lunar tidal influences, and hope that this is realistic enough to be able to keep.
Thanks!
...John...
I'm beginning to sketch out my entry for the Toliman (Alpha Centauri B) System, and thought I'd run them by you. Once I get a generalized idea of what I want, I'll start on the ssc file(s).
PLANET I: Baahki is a lower-massed world kept geologically active by the massive tidal stretching produced by its large (approximately half the diameter of Baahki itself), volcanically active moon. The second and smaller moon, while further out, also adds something to this effect. While the planet has no tectonic plates, volcanic activity and erosion slowly changes the surface over tens of millions of years.
PLANET II: Eutresca is a smaller, rocky world, heavity cratered. It is similar to Mercury in that it is quite dense for its small size.
PLANET III: Mephinos is Mars-like, with polar caps of water and carbon dioxide ice, and a cold and dry surface composed of rocky, cratered highlands and relatively smooth, nearly featureless lowlands. There are a number of very obvious dry river channels on the surface, along with corresponding erosional land forms, and many of these channels extend for hundreds of miles. Clearly, Mephinos was once quite wet. Today, as ide from some deep subsurface hot spots, it is largely geologically inert. It possesses two moons, one of which is a very small cratered ball, while the outer moon is a captured, irregular asteroid.
PLANET IV: NESSOS: This is a Panthalassic world, and the most masive planet orbiting either of the stars of the greater Alpha Centauri System. It has a substantial ring system, and a single large and cratered moon.
Thoughts are more than welcome. My biggest concern is the set up of Baahki and its moons, this world being the primary planet of interest for the system. I really like the idea of a planet being kept geologically active and habiutable due to lunar tidal influences, and hope that this is realistic enough to be able to keep.
Thanks!
...John...