BTW, I just put on line my new page about Interplanetary Flight.
Good page. One minor nit: you say that the heliocentric ecliptic coordinate system isn't quite inertial because of the precession of the earth's axis. Actually that's the reason that the
earth-centered equatorial coordinate system isn't inertial; that's where you see references to epochs like B1950 and J2000.
The ecliptic plane is much more stable than the earth's equatorial plane, but it too wobbles a tiny bit due to out-of-plane perturbations from the other planets, mainly Jupiter. If you want a
truly inertial coordinate system for interplanetary travel, use the barycentric invariant plane of the solar system. The origin is at the solar system's center of mass, dominated by the sun, of course. The reference plane is normal to the total angular momentum vector of the entire solar system, dominated by Jupiter's angular momentum but the other planets do contribute some tiny bits. Technically even the Kuiper Belt and the Oort cloud would have to be included, and since it contains many undiscovered objects the invariant plane is still somewhat ill defined. But probably not by much.
I'm not sure what you use as a longitude reference, probably the location of some distant quasar at the edge of the visible universe.