Jonathan Scott
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There are at least quasi-stable "Halo orbits" around L2 as described in the Wikipedia article Lagrange Point. These can be quite extended to avoid eclipsing.sophiecentaur said:We (i.e. I) fond to easy to forget the relevance of some aspects of big projects. The L2 position is not stable so the situation is very different from setting a course for orbiting round a massive object. The inverse law for GPE of a target planet provides a certain amount of help for getting into orbit, once you are near. There is no such central force around L2 so I imagine everything needs much more precision and you have to make your own quasi orbit around L2 (to avoid being eclipsed by Earth).
The L2 point is relatively close but enables the sun shade to hide all of the sun, the Earth and the moon at the same time.sophiecentaur said:L4 and L5 would probably be less problematical in that respect. L4 and L5 probably have their own disadvantages. Those points are a long way away (many minutes of signal path delay) and a much longer journey time.
