Lower temp (H, He, CH4, H2O, N2, ice) - outer edges
Planetary Compositions
Slide 11
How Did We Get a Solar System?
Inner Planets:
Hot – Silicate minerals, metals, no light elements, ice
Begin to stick together with dust clumps
Slide 12
How Did We Get a Solar System?
Accretion - particles collide and stick together … or break apart … gravity not involved if small pieces
Form planetesimals, up to a few km across
Slide 13
How Did We Get a Solar System?
Gravitational accretion: planetesimals attract stuff
Large protoplanets dominate, grow rapidly, clean up area ( takes ~10 to 25 My)
Slide 14
How Did We Get a Solar System?
Outer Solar System
Cold – ices, gases – 10x more particles than inner
May have formed icy center, then captured lighter gases (Jupiter and Saturn first? Took H and He?)
Slide 15
How Did We Get a Solar System?
Early burst of solar wind - sweeps debris out of system
Gravitational accretion of gas for protoplanets in the coolest nebular parts
Slide 16
? Should have been a planet instead of a debris belt? Jupiter kept it from forming
How Did We Get a Solar System?
Eros image at
Slide 17
Beyond the Gas Giants - Pluto, Charon and the Kuiper Belt objects
Chunks of ice and rock material
Little time / debris available to make a planet – slower!!
How Did We Get a Solar System?
Slide 18
Slide 19
Planetesimals swept up debris
Accretion + Impacts = HEAT
Eventually begin to melt materials
Iron, silica melt at different temperatures
Iron sank – density layering
Slide 20
Differentiation
Separation of homogenous interior into layers of different compositions
Early – hottest time – dense iron-rich material core
Releases additional heat
Leaves mantle with molten ocean enriched in silica