GEOINT
Resolution has always cost you a bigger bus.
Ground resolution scales with aperture. Aperture drives bus class, which drives launch cost, which drives how many you can afford and therefore how often you revisit. We are breaking the first link in that chain.
The chain
The economics of space imaging are downstream of one physical fact. To see smaller, collect over a wider aperture. A wider aperture needs a larger bus, a larger fairing, and a larger budget. Constellation operators then trade resolution against revisit, because they cannot buy both.
The second cost is downlink. A high-resolution sensor produces more data than any link can carry, so most of what is collected is never seen, and the latency between collection and answer is measured in tens of minutes.
A different scaling law
Sorting light by spatial mode extracts information that a brightness measurement discards. The information advantage does not come from a larger optic, which means the aperture-to-performance relationship is no longer the one everyone else is designing against.
And because the sensor output is a compact modal measurement, inference happens on the spacecraft. What comes down is the answer.
What that buys the mission
Small-aperture payloads with large-aperture utility. Modeled performance from a 30 cm class aperture against targets that conventionally demand far more.
Answers on orbit. Task the spacecraft, receive the finding. The image never has to fly.
Change detection in minutes. Simulated GEO scenarios detect change roughly ten times faster than a conventional equivalent.
Buy revisit instead of aperture. Cheaper payloads mean more of them.