Understanding Solar Array
How a solar array generates power
Each cell is a semiconductor sandwich that frees electrons when photons strike it — the photovoltaic effect. Space arrays use multi-junction cells, stacking layers of gallium arsenide (GaAs) and related III-V materials so each junction harvests a different slice of the solar spectrum. Today's triple-junction cells convert about 30% of incoming sunlight (the best qualified designs reach ~32%), against roughly 20% for a good terrestrial silicon panel. In Earth orbit the Sun delivers about 1,361 watts per square metre — the 'solar constant' — so array area, not just efficiency, sets how much power a satellite can draw.
| Cell technology | Typical space (AM0) efficiency | Use |
|---|---|---|
| Silicon (Si) | ~14-16% | Early satellites; low cost |
| Single-junction GaAs | ~19% | 1990s workhorses |
| Triple-junction GaAs/Ge | ~28-32% | Industry standard today |
| Four-/five-junction (advanced) | ~32-34% | Highest-performance, emerging |
Deployment, Sun-tracking and eclipse
Because arrays are large and fragile, they launch folded against the satellite and deploy once in orbit — rigid honeycomb panels that unfold like a fan, or flexible 'roll-out' blankets (ROSA) that extend like a tape measure. A Solar Array Drive Assembly then rotates the wings so they stay square-on to the Sun. What happens in shadow depends on orbit: a satellite in low Earth orbit is eclipsed on almost every ~90-minute lap, for up to ~35 minutes at a time, whereas a geostationary satellite basks in continuous sunlight except for two short 'eclipse seasons' around the equinoxes. Whenever sunlight is lost, lithium-ion batteries carry the load and recharge once the array is re-illuminated.
Why arrays are oversized: degradation
A solar array is at its strongest the day it deploys and weakens from then on. High-energy protons and electrons — intense inside the Van Allen belts and during solar storms — knock atoms out of the crystal lattice, while thousands of hot-cold thermal cycles, ultraviolet light and micrometeoroid strikes add further wear. Typical losses run a few per cent per year, so engineers deliberately oversize an array: a spacecraft built for a 15-year life in geostationary orbit must still meet its power budget at 'end of life', which means a generous surplus at 'beginning of life'.
Solar vs RTG: the deep-space limit
Sunlight thins out with the square of distance from the Sun, so an array that yields plenty of power at Earth (1 AU) gets only ~4% as much at Jupiter (~5.2 AU). Solar power stays practical out to roughly Jupiter's orbit — NASA's Juno probe flew enormous wings to manage it — but missions to Saturn and beyond, or into permanently shadowed craters, instead carry radioisotope thermoelectric generators (RTGs) that make electricity from the heat of decaying plutonium. Closer to home, the same abundant sunlight lets big arrays drive electric propulsion, powering ion thrusters for efficient orbit-raising and station-keeping.