Concept

Radial drift — where it appears

The inward spiral of solid particles in a gas disc, caused by gas that orbits slightly slower than a lone particle would because its own pressure partly supports it. Pebbles of a millimetre to a metre feel the headwind most and can drift to the star in a few hundred orbits.

Named by 2 essays across one field — each of them below, with the objects they name alongside it.

Named alongside it

The objects these essays reach for when they reach for this one.

Protoplanetary discThe snow lineAccretion rateCarbonaceous chondriteCondensation sequenceDisc evolutionEquilibrium temperatureFormation timeJupiterPebble accretionPebble isolation massPlanetesimal

All concepts