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GMoromisato ◴[] No.44401068[source]
In case anyone is wondering, we are (sadly) very far from getting an image of this planet (or any extra-solar planet) that is more than 1 pixel across.

At 110 light-years distance you would need a telescope ~450 kilometers across to image this planet at 100x100 pixel resolution--about the size of a small icon. That is a physical limit based on the wavelength of light.

The best we could do is build a space-based optical interferometer with two nodes 450 kilometers apart, but synchronized to 1 wavelength. That's a really tough engineering challenge.

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GolfPopper ◴[] No.44401398[source]
We can do better than that! Using the Sun as a gravitation lens[1], and a probe at a focal point of 542 AU, we could get 25km scale surface resolution on a planet 98 ly away. [2] This would be an immense and time-consuming endeavor, but does seem to be within humanity's current technological capabilities.

1. https://en.wikipedia.org/wiki/Solar_gravitational_lens

2. https://www.nasa.gov/general/direct-multipixel-imaging-and-s...

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os2warpman ◴[] No.44401969[source]
A maintenance-free power source capable of lasting the 200 or so years it would take to make it to 542 AU does not seem within humanity's current technological capabilities.

Parker at its highest velocity could make it there in a century, but it doesn't have to slow down and stop. Or station keep.

When we have a power source that can do 5kW (I just doubled Hubble, 542 AU would probably require much more for communications) for 100 years I'll agree that its design can be refined and its lifespan extended to 200 and 542 AU is within our reach.

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dotnet00 ◴[] No.44402336[source]
With distances that big, is it even necessary to slow down much? The depth of focus is probably a couple dozen AU? Even if it takes the probe a century to get there, if you can squeeze a decade or two of observation out of it without slowing down, there's no reason to bother and instead send a new upgraded telescope every decade or so.

As far as power requirements go, assuming a doubled power demand from Hubble might be a bit excessive. A telescope that far out would have to be nuclear powered, so thermal regulation is 'free'/passive and RCS load is reduced (don't have to constantly adjust to point away from the Earth), which I expect are the biggest power draws on Hubble.

If we assume a 150 year lifetime, with a 3kW draw by EOL and current RTG tech... RTGs have ~6% efficiency, so for 3kW electricity, you need 50kW in heat. RTG electricity output drops ~2% per year, so after 150 years, you have 5% of the initial electrical output, and you get ~0.57W/g of Pu-238. Meaning, you need ~600kg of it to power the telescope this way [https://www.mathscinotes.com/2012/01/nuclear-battery-math/].

That's not a politically feasible amount, but it's not technically impossible with current/near future tech whose development could be spurred on by serious interest in this kind of mission.

'Proper' fission reactors can also do the job, you get higher efficiency and don't have to run the reactors for the entire 150 years besides accounting for decay (e.g. an RTG that needs to provide enough power to keep some clocks running, the electronics and batteries warm, and trigger whatever mechanism would start up the reactor). Probably less than 100kg of Pu-238 just by better reactor efficiency.

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griffzhowl ◴[] No.44403987[source]
Wouldn't there be a problem putting 600kg (or even 100kg) of Pu-238 together, because of supercriticality? I couldn't think of a plausible design, but I know next to nothing about this area. Basically I've heard that if you put a lot of this stuff together it'll make a big explosion
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ben_w ◴[] No.44405063[source]
Criticality isn't hard to avoid, just split it between e.g. 344 units arranged in a 7x7x7 cube with 10cm gaps each way. Or more, I picked that separation and mass division based on guessing.
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griffzhowl ◴[] No.44406831{3}[source]
Yeah, I thought about doing something like that, but that would make many parallel power-generating units that would only last as long as one unit wouldn't it? Maybe the individual units could be subdivided further and the subunits could be brought together only when a previous unit runs out of power. I don't know enough about how it would actually work
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ben_w ◴[] No.44407406{4}[source]
I don't think so. The radioisotope itself is an exponential decay, and only goes faster when critical, not when subdivided; the part I'm not sure about is the thermocouple and why that decays.
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1. griffzhowl ◴[] No.44409380{5}[source]
I see. So the maximum time these units could provide power is the time it would take a subcritical mass to decay to the point that it's no longer useful. So the idea is unworkable for powering very long journeys
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2. ben_w ◴[] No.44411335[source]
Very long journies, eventually everything fails. I suspect that we don't have enough practical experience to be confident of any space mission lasting 100 years even when the power supply is fine.

But also, there are other radioisotopes besides the one currently used. The ~90 year half life of the current normal radioisotope is great for current missions, not the only option.