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protoplanet
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protoplanet

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thumb|4 Vesta|Vesta is one of the best known examples of a protoplanet. A protoplanet or planetary embryo is an astronomical body originated within a protoplanetary disk that has undergone internal melting to produce a differentiated interior.

~8 min read

Encyclopedic overview

7 sections
Contents
  • The planetesimal hypothesis
  • Evidence in the Solar System - surviving remnant protoplanets
  • Extrasolar protoplanets - observed protoplanets
  • Unconfirmed protoplanets
  • See also
  • References
  • External links

thumb|4 Vesta|Vesta is one of the best known examples of a protoplanet. A protoplanet or planetary embryo is an astronomical body originated within a protoplanetary disk that has undergone internal melting to produce a differentiated interior.

Protoplanets are thought to form out of kilometer-sized planetesimals that gravitationally perturb each other's orbits and collide, gradually coalescing into larger bodies through a process known as "runaway growth". Once accumulated enough mass, protoplanets will begin to assume a spherical shape due to hydrostatic equilibrium and become dwarf planets, those of which that subsequently succeed in dominating their own orbit will become planets proper.

Excerpted from Wikipedia’s “protoplanet” article, available under the CC BY-SA 4.0 licence.

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