Clear Orbit Secure Future 2026
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1.2 Phases and uncertainties
Because operational practices evolve over time, the model does not assume a single,
static future. Instead, it projects the risks from 2025 to 2040 in three developmental eras:
Confidence intervals applied to each five-year modelling phase TABLE 1
Phase Period Description Uncertainty
Constellation revolution 2025–2030 Rapid deployment of large constellations per ITU filings ±10%
Constellation maturity 2030–2035 Improved reliability, lower failure rates ±20%
Constellation evolution 2035–2040 Mergers, migration to lower orbits ±50%These uncertainty levels determine the confidence
intervals applied to each five-year modelling
phase. In practice, they define how widely
the model’s outputs – such as object counts,
collision probabilities and debris growth rates –
may vary from baseline scenarios. A ±10%
uncertainty reflects relatively reliable inputs, since
near-term launch manifests and constellation plans are well documented. By contrast, the
±50% uncertainty reflects the compounding
unpredictability of future operator behaviour,
market consolidation, regulatory enforcement
and unplanned fragmentation events. The wider
the uncertainty band, the greater the dispersion
of projected debris densities and collision risks
that feed into the economic model.
1.3 Translating population into risk
Even small annual probabilities accumulate to form a
notable threat across tens of thousands of spacecraft.
For instance, a satellite operating near 805 km in
2035–2040 faces a 1.5% chance of an anomaly
and a 0.55% chance of mission-ending impact per
year, small individually but substantial collectively. To translate broad projections into specific risk
probabilities for a typical satellite, it is crucial to
understand the annual likelihood of an impact for
a representative satellite (3 m2 cross-section) from
three different categories of debris, each with a
different real-world consequence.
Specific risk probabilities for a typical satellite TABLE 2
Symbol Description Likely effect
PC(HNT) Probability of collision by hazardous
non-trackable debris (5 mm–1 cm)Causes a non-mission-ending anomaly,
such as temporary service disruption or
partial damage
PC(LNT) Probability of collision by lethal
non-trackable debris (>1–10 cm)Causes mission-ending damage
or total loss of the satellite
PC(Cat) Probability of close approach
with tracked objectRequires an operator to perform
a collision-avoidance manoeuvre
Clear Orbit, Secure Future: A Call to Action on Space Debris
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