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by cletus 758 days ago
There are several possibilities here.

First, the Earth already receives a ton of energy from the Sun that is "wasted". We estimate that at about 10^16 Watts of power, compared to humanity's energy usage, estimated at 10^10-10^11 watts. So Earth has a ton of energy dissipiation "built in" that we're not "using".

Second, there is some inefficiency and thus heat dissipation in converting solar output into usable energy. Doing that in space means a bunch of heat dissipation happens in space rather than on your planet.

Third, it's relatively straightforwward to counter any increased heat dissipation on your planet by reducing that solar output that hits your planet. How? You build something at the EArth-Sun L1 Lagrange point. Reducing that solar output that hits the EArth by 1% would likely be unnoticeable to us but could cool the Earth significantly. Also, what do you build there? Well, lots of things. More orbitals, solar power collectors, etc.

Fourth, how do you get power down to a planet? There are several candidates. One is to beam it down. This adds a conversion cost. But here's another: you build a n orbital ring [1] 100-150km above the EArth's surface. There are a ton of reasons you'd want to do this: interplanetary travel, cheap travel to and from LEO and easier travel across the planet (ie up to the ring, down to another point on Earth on cable cars, basically). But consider this: it gives you a rigid structure to attach solar power collectors to and you can run power transmission cables down from the ring to the planet's surface.

[1]: https://www.youtube.com/watch?v=LMbI6sk-62E

2 comments

I wonder how much reaction mass we’d need every year to keep something stationed at a Lagrange point to block 1% of earth’s light, for combatting global warming. 1% of earth’s light would be a heck of a solar sail.

Looks like 1% would be 13.3 watts per meter, cross section of earth yields ~5.4x10^14 watts. Assuming perfect reflective, multiplying by 2/c gives 3.6x10^6 N. So like half of the thrust of one of Saturn V’s engines? So… a lot of reaction mass, or some really powerful ion engines and a ton of power. So maybe not the most practical idea.

It's true that the L1 Lagrange point is unstable so would need some station-keeping. It's an issue but it's a solvable issue. For one thying you have a bunch of energy to spend. For another, the solar wind itself can be used to provide momentum going out if what you have there is sufficiently light.

But there's another option: statites [1]. Statites are solar power collectors that have an incredibly thin sail to the point that they don't need to orbit the Sun at all. This means you have a bunch more options for positioning. Clearly the Earth will continue to revolve around the Sun but a sufficient swarm of statites on the EArth's orbital plane could have the same net effect as, say, driving beneath a bunch of stationary umbrellas.

Or statites can themselves do station-keeping at L1. They can angle themselves to provide momentum in a bunch of directions. Or they can orbit the L1 point similar to how JWST orbits L2. Their ability to use the solar wind for directional momentum could satisfy station keeping needs.

[1]: https://en.wikipedia.org/wiki/Statite

Oh very cool.

Besides the unstable nature of L1, my main concern was actually mitigating the light pressure of the light being blocked, in order to not be blown earthward, but I guess that’s not really considering that these things could manipulate their solar sails/shades like the statites you’re mentioning.

Are you capitalizing it like EArth for a reason or just a typo? Just wondering as you use it a few times but are flip flopping.