Drag decay model
For a circular orbit the semi-major axis decays at da/dt = −ρ·√(μa)·(C_d·A/m). The tool integrates this from the initial altitude down to 150 km, interpolating log-density in a reference table (CIRA/SMAD-class values) for the selected solar activity.
Drag make-up: continuous compensation of the drag deceleration a_D = ½·ρ·v²·C_d·A/m gives Δv/year = a_D · 31.6×10⁶ s.
Accuracy: real lifetimes vary with the actual solar cycle phase, attitude history and density model — treat results as order-of-magnitude (±50% is typical even for professional tools). For compliance filings use a full propagator (e.g. NASA DAS/ORSAT-class analysis).
All computation runs locally in your browser.