I
impulse
Guest
Yah about those ceilings... they come essentially "for free" in a sense. The top element is like the top of a bagel- it contains all the air handling, lighting, power and data distribution, water etc. It has a domed upwards shape and the apex is dictated by structural efficiency- making a flat pressurized structure is inefficient- at least at large dimensions. <br /><br />Without my immediate access to the diagrams which outline the architecture concept it is a bit difficult to discuss it but here are some fundamentals:<br /><br />The key thing about exploration transport is that most of the mass we have to move is propellant and most of that is LO2. This is often lost on a lot of folks. So the thing we need the most of has almost no intrinsic "value". It is not a super-complex spacecraft. We need to become absolute experts at moving and storing propellants. Without this you aren't going to Mars and your lunar explorations will be pretty feeble.<br /><br />Storing cryogens can be either hard or easy- you get to pick. The last place to put a cryo depot is in LEO. There is not only the normal solar irradiance but also earth albedo and IR- both of which are significant. Aerodrag is nonzero as well as gravitational/tidal effects. Once you pick an orbital plane you are also quite restricted in when you can go to the moon thereafter. It is far better to burn out of LEO and just get to cislunar space as soon as possible. In other words, you must execute a 3100 m/sec burn to get out of LEO and another 1100 or so for LOI so it is best to do that immediately and reduce the mass of cryos that must be stored. It is far easier to maintain reasonable boiloff rates with reduced masses and in lower heating environments. <br /><br />You don't have to eliminate boiloff- in fact you need to have some. If you plan on staying near the moon you must count on using up stationkeeping propellants. Fortunately it turns out that GH2 makes a wonderful propellant- so we use it exclus