A statite swarm — solar sails held stationary by radiation pressure balancing gravity, first proposed by Robert Zubrin & Chris McKay (1993) for warming Mars — collects sunlight and redirects it onto a planet's polar CO₂ ice cap to trigger runaway sublimation and thicken the atmosphere.
Reflected power: P = ρ · S · A_total
Added flux at cap: ΔF = P / A_cap (W/m²)
Sublimation rate: dm/dt = ΔF · A_cap / L_s (kg/s)
S = solar constant at planet (Mars ≈ 590 W/m²)
ρ = mirror reflectivity (0–1)
A_total = N · π·r_mirror² (total collecting area)
L_s = latent heat of sublimation, solid CO₂ ≈ 5.9×10⁵ J/kg
The aim-declination angle sets how tightly the reflected beam is focused onto high latitudes — near-grazing angles (close to 90°) spread the beam and lose flux to the horizon, so there is a real trade-off you can explore.
- Mirror count / radius — set N and the per-mirror collecting radius; together with ρ they set total reflected power P.
- Aim declination — how far from the pole the swarm's focal spot sits; steeper angles concentrate flux, shallower ones spread it.
- Reflectivity ρ — the fraction of incident sunlight actually redirected (thin-film Mylar-class sails run 0.85–0.95 in practice).
- The ice cap mass integrates the sublimation rate over time; once a patch fully sublimes it stops contributing further flux absorption there, so the rate visibly slows as the cap thins.
Real proposals (Zubrin/McKay, later NASA-sponsored studies) estimate a ~125 km-radius mirror could raise Mars's south polar temperature enough to start irreversible CO₂ release — this simulator uses the same flux-balance physics at a scale you can tune interactively.