Orbital debris — where it appears
Named by 4 essays across 2 fields — each of them below, with the objects they name alongside it.
A collision rate that needs no collision
The flux through an orbital shell is a gas-kinetic calculation with no orbits in it. Production goes as the square of the population and removal goes as the first power, so a quadratic overtakes a linear once and never comes back — and which side of that a shell is on is decided by its altitude.
Where the mass is and where the light is
A population that grinds itself up settles into a size distribution with a fixed slope, and that slope puts almost all the mass in the largest bodies and almost all the cross-section in the smallest. So a debris disc's brightness measures a population whose mass it says nothing about, and the two are connected only by the exponent.
A satellite that drifts to one of two longitudes
The Earth's equator is elliptical by about seventy metres. That one harmonic of the gravity field gives geostationary orbit a potential with two minima, so an unattended satellite slides towards the nearer one and stays — and every operational slot in the ring is paid for with fuel, every year, forever.
The fragments nobody can see and cannot shield against
A catastrophic collision in low orbit makes about a thousand pieces big enough to track and sixty thousand big enough to destroy a spacecraft. The catalogue is under two per cent of the hazard, the gap is not one better radars will close, and the fragments' lifetimes span a factor of twenty-five within a single event.
Named alongside it
The objects these essays reach for when they reach for this one.
Ballistic coefficientKessler syndromeOrbital lifetimeArea-to-mass ratioAsteroid familyBreakup modelCollision cross-sectionCollisional cascadeConjunction analysisConjunction assessmentCritical densityCross-section