Collisions
Crowded shells raise the risk that one collision triggers more. Screening and removal keep it in check.
Orbit is getting crowded and contested. As sensors improve, the tracked catalog is heading past one hundred thousand objects, so every operator needs to know where everything is, what it is doing, and when to move.
The risks range from debris to deliberate interference, and space weather affects them all.
Crowded shells raise the risk that one collision triggers more. Screening and removal keep it in check.
Close approaches and co-orbital activity need detection, characterization and attribution.
Geomagnetic storms increase drag, scatter the catalog and bring objects down early.
This mission's share of the five layers.
L0 · Ground | Reuse: Space Fence, the Space Surveillance Network, GEODSS, commercial radar and optical networks, civil traffic coordination Add: A distributed small-telescope network for GEO and cislunar space; the shared deep-space radar |
|---|---|
L1 · LEO | Reuse: Optical-crosslink transport mesh; commercial constellations as hosts Add: SSA sensors looking up and out; inspector spacecraft |
L2 · GEO | Reuse: GEO neighbourhood watch; commercial life-extension servicers Add: Maneuverable GEO patrol satellites; refueling depots; debris-removal tugs on a common bus |
L3 · Cislunar | Reuse: Little dedicated capability today Add: SSA sentinels at Earth–Moon L1/L2; relay and timing node |
Concept phase: these are aims, not results.
An architecture is a hypothesis until a reproducible trade study says otherwise.
Every number on these pages is a planning estimate from public sources. The program's job is to replace each one with a traceable result from open analysis tools: stated assumptions, the tool version, the inputs, and the output. The work uses public, unclassified sources only.