Drag & decay

LEO Drag & Decay Timeline

How long does a satellite stay up? Atmospheric drag at 400-800 km is small but relentless. Plot the curve.

How this model works & what it omits

King-Hele simple-atmosphere drag, exponential density table fit to NRLMSISE-00. solar activity tiers, mass/area/Cd inputs. orbit-mean approximation. flight design needs MSIS-90/2000 + numerical propagation.

This satellite orbital decay calculator integrates the King-Hele (1964) drag formulation numerically from your starting altitude until reentry - or a 50-year horizon - with atmospheric density from a reference table fit to NRLMSISE-00 (Picone et al., 2002) at three solar-activity tiers. It reports orbital lifetime, the altitude-vs-time decay curve, the initial decay rate, and the ballistic coefficient for any satellite in low Earth orbit (LEO), from a 1U CubeSat to a station-class platform. It is an engineering trade-study estimate; flight design needs MSIS-class density models and numerical propagation (Vallado 2013, ch. 8).

Every satellite in LEO is slowly losing altitude. Even at 600 km, the atmosphere has enough density (~10⁻¹³ kg/m³ at moderate solar activity) that the few grams of mass swept up per second by a typical smallsat translate to several metres of altitude lost per day. Over years, the loss compounds; eventually the orbit dips into denser air below ~150 km, the satellite tumbles, and reentry happens within hours.

This tool uses the King-Hele simple-atmosphere drag formulation: da/dt = -CD · A · ρ(h) · √(μ · a) / m, integrated numerically with an adaptive timestep until either reentry (100 km threshold) or the 50-year simulation horizon. Atmospheric density comes from a 15-point reference table fit to NRLMSISE-00 (Picone et al., 2002) annual-mean output at three solar-activity tiers (F10.7 ≈ 70 / 150 / 230). Between table entries, density is interpolated linearly in log space against altitude.

The ballistic coefficient BC = m / (CD · A) is the single most important parameter: high BC (heavy, small frontal area) decays slowly; low BC (light, large frontal area like deployed solar panels) decays fast. A 3U CubeSat at 4 kg / 0.03 m² has BC ≈ 60 kg/m²; a deployed International Space Station (ISS)-class platform at 100 t / 2500 m² has BC ≈ 18 kg/m². Solar activity multiplies density by roughly 5× from minimum to maximum at any given altitude, which translates to roughly 5× decay-rate change.

What this tool does not capture: diurnal density variation, geomagnetic-storm transients, ballistic-coefficient changes from attitude variation (tumbling vs gravity-gradient), drag-modulating sails, propulsive reboost. The 25-year reentry guideline (IADC 02-01, NASA-STD-8719.14B) is the regulatory anchor for mission lifetime planning.

pick a class, then dial mass / area / solar activity.

Orbit

circular orbit; King-Hele simple-atmosphere model.

Spacecraft

ballistic coefficient = m / (Cd × A).

Atmosphere

reference table fit to NRLMSISE-00; engineering trade study only.

Decay timeline: time to reentry 2.47 years, ballistic coefficient 90.9 kg/m².

Decay timeline

BC 90.9 kg/m² · orbit period 94.6 min

2.47 years

Time to reentry

903 days

Same, in days

90.9 kg/m²

Ballistic coefficient

69.7 m/day

Initial decay rate

1.4e-12 kg/m³

ρ at start

100 km

Final altitude

altitude vs time

0 km125 km250 km375 km500 km0 d7 mo1.2 y1.9 y2.5 y
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Common questions

How long will a CubeSat stay in orbit?

For a typical 3U CubeSat (4 kg, 0.03 m² frontal area) at moderate solar activity, this model gives roughly four months from 400 km, under two years from 500 km, about seven years from 600 km, and nearly three decades from 700 km. Starting altitude dominates everything else, because atmospheric density falls off roughly exponentially with height - load a preset above and change the starting altitude to see the CubeSat orbital-lifetime curve swing.

What drag coefficient (Cd) should I assume?

Cd = 2.2 is the standard engineering value for satellites in free-molecular flow at orbital velocity (Cook 1965), and it is this tool's default. Unless you have mission-specific aerodynamic analysis for your geometry and attitude, 2.2 is the accepted trade-study assumption.

What is the ballistic coefficient, and why does it dominate decay?

BC = m / (CD · A) - mass over drag coefficient times frontal area. High BC (heavy, compact) decays slowly; low BC (light, or trailing deployed solar panels) decays fast. A 3U CubeSat at 4 kg / 0.03 m² has BC ≈ 60 kg/m²; a deployed ISS-class platform at 100 t / 2500 m² has BC ≈ 18 kg/m². Deployables can be a deorbit feature: more area, faster reentry.

How much does solar activity change orbital decay?

Roughly 5× in density at any given altitude from solar minimum to maximum - and because the effect compounds along the whole decay trajectory, the lifetime spread is wider still: the same 3U CubeSat at 500 km reenters in about half a year at solar maximum in this model, versus nearly seven years at solar minimum. That spread is why lifetime predictions carry large honest error bars: nobody knows the future F10.7 flux.

Can I use this for an FCC 5-year-rule check?

This page estimates natural decay only. For a pass/fail screen against the Federal Communications Commission (FCC) 5-year rule, the European Space Agency (ESA) Zero Debris standard, or the legacy 25-year guideline - with remediation sizing when a limit is missed - use the satellite deorbit compliance calculator, which runs the same King-Hele lifetime model against each regime's limit.

References

  • King-Hele, D. (1964). Theory of Satellite Orbits in an Atmosphere. Butterworths.
  • Picone, J. M., Hedin, A. E., Drob, D. P., Aikin, A. C. (2002). NRLMSISE-00 empirical model of the atmosphere. JGR 107(A12).
  • Cook, G. E. (1965). Satellite drag coefficients. Planetary and Space Science 13(10), 929-946.
  • Vallado, D. A. (2013). Fundamentals of Astrodynamics and Applications, 4th ed., ch. 8 (Perturbations).
  • IADC 02-01, NASA-STD-8719.14B - the 25-year reentry guideline.
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