The core accretion theory explains how planets form through a gradual process where microscopic dust grains in a protoplanetary disc around a new star stick together and grow over millions of years, progressing from dust to pebbles, rocks, boulders, and finally kilometer-sized planetesimals that serve as the seeds of planets.
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How Grains Become Giants #astronomy #shortsAdded:
For most of modern astronomy, the go-to [music] theory for planet formation was a process called core accretion. It all starts inside a huge, spinning cloud of gas and dust [music] around a brand new star. We call this a protoplanetary disc. Inside this disc, microscopic [music] dust grains, no bigger than smoke particles, start sticking together.
Think of it like snowflakes bunching [music] up to make a bigger, heavier clump.
Over millions of years, this just keeps happening. Dust becomes pebbles, [music] pebbles become rocks, rocks become boulders, and those boulders grow into kilometer-sized bodies we [music] call planetesimals. These planetesimals are the real seeds of planets.
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