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Earth-Sol L1 is probably a bad place for a solar shade. That's where a solar shade of any given size is the most efficient, but the cost of getting it there is
by Tuna-Fish 8y ago
Earth-Sol L1 is probably a bad place for a solar shade. That's where a solar shade of any given size is the most efficient, but the cost of getting it there is much more than the cost of having more, less efficient ones.
A better choice is something akin to a semi-sun-synchronous Molniya-style-orbit. That is, orbit that is somewhat highly elliptical (so a satellite on it spends most of it's time near apogee, and zips through the perigee relatively quickly), and which precesses so that the apogee is always between the earth and the sun.
A satellite on such an orbit can easily spend >70% of it's time between the earth and the sun, and you could send many satellites there for a similar cost to putting just one to Earth-Sun L1.
- Retric 8y agoLEO to L1 is not that bad using solar sails or ionic propulsion. There are going to be real trade-offs to any orbit, but I think the minimum cost is going to be above X mass in L1 means X mass into LEO as you can't use less mass than that in any other orbit.
- Tuna-Fish 8y agoBut then you have to put solar sails or ionic propulsion into the shade. BFR could deploy a completely passive sail directly into such a sun-synchronous elliptical orbit, return to land, and launch again after a few hours.
- Retric 8y agoAnything that blocks that much light is going to be a huge solar sail and need a lot of station keeping. The only reason ionic propulsion might be considered is the they are already going to be solar panels. If you make a large chunk of them from solar panels you then have crazy energy for space based industry and plenty of energy for ionic propulsion. Also, with that much mass in orbit you are going to want some way do move dammaged segments.
- elihu 8y agoSupposing you can re-orient parts of the "huge solar sail" then wouldn't it become rather like the sail of a ship or the wing of a plane, and be usable as a control surface for maneuvering? I'd imagine that in the neighborhood of L1 you would try to find some equilibrium point a little closer in to the sun so that the force of the solar wind matches gravitational pull to the sun. If you start drifting in to the sun, you expose more surface area, and if you're drifting towards the Earth, you re-orient the sail to absorb less solar wind.
- Retric 8y agoThat's the idea I was going with. You let the sun counteract most of the force from your solar sail, but that requires you to constantly to make minor adjustments because unlike a normal orbit it's not even close to stable over time. But, while not necessarily difficult it does prevent a lot of the more simple designs as you can't just toss out a bunch of reflective beach balls with very low pressure or other 'simple' means of blocking sunlight.
- ninkendo 8y agoHow are you going to use a solar sail to go towards L1 from LEO?
- Retric 8y agoYou don't have a keel, but you can use the suns gravity with a similar goal. The sun's gravity is much stronger than a sail's thrust so you can't hover, but you do end up in a higher orbit by aiming it at the sun. However, this averages over an orbit so you don't gain energy over time. But, aim the sail off-center say 45 degrees from the sun and you can pick if that's adding or subtracting angular momentum from your orbit over time. Reduce angular momentum and gravity pulls you into a lower orbit and thus more orbits/year. Reverse that and your gain angular momentum and get fewer orbits per year. L1 is a special case as it's balanced between the sun and earth so you have the same number of orbits per year. Now, rather than just orbiting the sun your also orbiting the earth. But, similar manovers work just fine. PS: It's even more complected as you end up in elliptical orbits if you don't keep things balanced etc, but that's the basic idea.
- tgb 8y agoIs L1 the most efficient for a fixed size? The difference is ~6000 km for LEO versus 1.5 million km for L1 to the Earth's center and the r^2 law means you need to put a lot more area in L1 than in LEO, even after discounting for the fact that in LEO it'll be on the wrong side of the Earth half the time. Filling up appreciable fractions of LEO might have it's own problems.
- Retric 8y agor^2 is not that relevant. The moon is 384,400 km from the earth and can cause a total solar eclipse despite only being 3,474 km wide where the earth is 12,742 km wide. The geometry works out more or less linearly with distance. So 1.5 / 0.384 = 1.065. Which means and object 1.065x as wide as the earth would also provide a total solar eclipse. Making sunshades more than 2x effective L1 vs LEO. PS: Only 1/2 the time they are on the sun facing side, but they are not perpendicular with sunlight for that entire half. At a 45 degree angle a sunshade blocks ~70% as much sunlight vs a 0 degree angle.