u/FineFinish7297

I’ve been thinking about distributed CubeSat-based observation architectures and trying to understand them from a systems engineering perspective rather than a mission-specific one.

The idea would be a loosely or tightly coordinated network of small satellites performing shared observational tasks (optical or other sensing modalities), with some level of distributed coordination and data fusion.

Not a single mission, but a system-of-systems with:

• distributed sensing nodes (CubeSats)
• coordinated observation scheduling
• inter-node communication (or ground-mediated sync)
• shared calibration strategies
• distributed data processing / fusion pipelines
• possibly near-real-time transient detection workflows

From a systems engineering standpoint, I’m trying to understand where the real limiting factors emerge when you scale coordination across multiple independent orbital nodes.

Some questions I’m particularly interested in:

• Where does coordination complexity become dominant over hardware constraints?
• How hard is cross-node calibration in practice for meaningful data fusion?
• What are the real bottlenecks: timing synchronization, bandwidth, orbital mechanics constraints, or something else?
• At what point does the system stop being “distributed instruments” and become “independent instruments with post-hoc aggregation”?

Curious how people here would break down the system-level failure modes or scaling limits.

With modern synchronization, edge computing, low-cost sensors, and global connectivity, I’m wondering whether a genuinely distributed telescope architecture is becoming technically realistic.

Not just remote observatories, but a coordinated network of geographically separated optical systems operating as a collaborative observation infrastructure.

Potentially involving:

• synchronized observations across regions
• distributed tracking/monitoring
• shared calibration pipelines
• real-time data aggregation
• AI-assisted filtering and anomaly detection
• coordinated transient event capture

It feels like several enabling technologies have quietly matured at the same time, but most astronomy infrastructure still seems relatively centralized.

I’m curious whether the main bottleneck at this point is:

• instrumentation quality,
• synchronization precision,
• software architecture,
• data throughput,
• organizational complexity, or something else entirely.

Interested in hearing perspectives from people working with optics, satellites, sensing systems, distributed systems, RF, imaging pipelines, etc.

What do people think about the idea of a collaborative telescope network?

Not just one observatory, but a distributed community where members coordinate observations, share data, track events, and potentially create a kind of crowd-powered telescope infrastructure.

Feels like something that should already exist at scale.

Curious whether people here think the technical/community side is actually feasible.