“Terrascope”: The possibility of using the Earth as an atmospheric lens (2019)
arxiv.org
arxiv.org
If so, that could make for either a very unfortunate surprise (i.e. a spacecraft passing through that point suddenly melting to a crisp) or an interesting source of energy if it could be harnessed.
The argument about reversibility is kind of a straw man: it answers "why can't you concentrate all light on a single point" while the real question would be "why can't you concentrate light on a smaller surface" (which you can do actually).
Similarly for the conservation of étendue: maybe you can't "swoosh the light rays closer together" but that also doesn't say you can't concentrate beams on a small surface, which might be sufficient to start a fire.
So really it all comes down to the thermodynamic argument, which has its own problem: it only works if you assume that moonlight has the same temperature as the moon. There's nothing in the article that mentions or justifies this assumption. And obviously a mirror can reflect light that is much warmer than itself, so you definitely have to explain why that's not the case with the Moon (e.g. its albedo and heat dissipation are too low).
(However I love the drawing of the encircling sun, it's great to make the point that no matter how much light you concentrate, it won't heat the body warmer than the light's temperature).
With a mirror you can also burn things if you focus sunlight, but the surface of the mirror stays cool.
An atmospheric lens, however, will reach a maximum of somewhat closer to solar surface temperature, though still lower because of scattering and absorption which definitely isn't trivial on this kind of scale.
https://www.universetoday.com/19981/moon-albedo/
If it had an albedo of 0% it would be a black body and be radiating only thermal radiation at its surface temperature; it's not too far away from that but it is reflecting some "black body" radiation from the sun representative of a higher temperature.
To summarise, you put a telescope beyond the orbit of the moon and use the earth's atmosphere as a lens
It seems to me though that the Earth's atmosphere is always going to be "lit up" one way or another by some phenomenon like the Aurora Borealis, scattering and various sorts of skyglow, so there will be some background, but maybe it is not that bad.
For earth or space based telescopes, we just keep the observer and lens rigidly attached and then move the whole apparatus slowly and carefully (computer controlled) to maintain a straight line.
For an earth-atmosphere lens, you don't have the rigid stability between the observer and the lens. You can't move the target or the earth, so you'd need to keep moving the observer to keep it perfectly in place.
That sounds like a lot of delta-V expended for each observation. It's probably easier to just build a 150m telescope on the moon or in space.
Orbital mechanics is a pretty well understood thing, so figuring out how the earth will move over the next 20 hours isn't that tough.
The rest is just making sure you're able to position the 1m receiver very precisely and move it around in a very controlled way. I'm no expert, but I suspect we've demonstrated both in one or more NASA missions already.
Probably super-expensive, but less of a technical challenge than building a proper 150m optical telescope.
There is a precise point the craft would need to stay at relative to the earth and the target. There aren't any stable orbits that keep a craft at precisely that position, which means you are firing engines for 20 hours straight.
Remember, you don't stay in space unless you are either in a stable orbit, moving at many km/s, or you're firing engines to resist gravity's pull.
A spacecraft to stay at this point for 20 hours would be massive, and 99.9% fuel tanks.
Even though the first image wouldn't be ready for a long time, if you have a lot of targets then you could increase efficiency to something like a tolerable level.
At that distance you would be sampling light that has passed through the Earth's atmosphere at an altitude of 14km. About 8% of the light would be lost, but at that altitude there's little weather to disturb the image.
The Lagrange points are stable positions relative to two bodies, like the earth and the moon or the earth and the sun. But those things are moving, orbiting. The points move with them. The line from the earth to any Lagrange point won't stay stably pointing at any star in the sky.
And even then, the focal point of this atmospheric lens is at a specific distance that is not, afaik, the distance to any Lagrange point.
https://www.youtube.com/watch?v=NQFqDKRAROI
(The whole video is great.)
This setup could resolve the surfaces of exoplanets with its ~100 billion magnification.
JPL is investigating.
Maybe we can put ChatGPT in charge...? :P
So even if we'll live to see this project funded, started and launched, there's pretty much no way we'll still be alive once the sensor probe reaches it's duty station.
Also, the telescope will be pretty much purpose build to look at one thing. Swiveling the telescope to look at something different or to track a moving object involves moving the sensor probe millions of kilometers across space.
https://en.wikipedia.org/wiki/Breakthrough_Starshot
and if you built some kind of "gun" that can shoot those things you could should numerous ones out in different directions to observe different targets and definitely have results in years if not weeks instead of decades.
IIRC this is actually one of the plot points in the Three Body Problem, where they used the sun to send out a signal and make first contact with an alien civilization.
This is like chapter ~one of book one (if you skip over the tangential Chinese politics stuff that I didn't understand on my second read either), so not really a spoiler. In the book it's some magic amplification that happens inside the sun, not based on a physical effect we've actually observed in real life as far as I know.
In this case, it's about gravitational lensing (when using the sun) and additionally atmospheric refraction (when using the earth; terrascope).
I'm also not sure we could use this, as in 3BP, to send anything. What this does is collect light rays coming in essentially parallel and focus it on a line along which we can place a detector. If we emit from somewhere along that line, it would be scattered as a ring the size of the lens (the earth or sun, in the examples, plus whatever altitude we use to avoid clouds or corona) because the rays are basically parallel from there. At least, that's my guess. I didn't understand even what my high school teacher tried to explain about lenses so this is speculation based on a drawing I saw in the terrascope video linked elsewhere in the thread (https://www.youtube.com/watch?v=jgOTZe07eHA).
We would need a train of probes being sent in a row because there is a limited amount of time they will pass through the focal area.