Core composition
Outer Core solid metallic alloy
- -> mainly Fe and Ni + eighter elements such as S and O
- -> less probable or less significant: Si, Ni, H, Mg
Arguments for light element determination mainly follows from considerations on:
- -> abundance in the Earth's mantle, relative to cosmic abundances,
- but losses due to volatility have to be considered too
- (e.g. H very abundant in universe but high losses due to volatility)
- -> ability to form alloys as seen in laboratory experiments and meteorites
- -> ability to lower the density of the core (e.g. good for S, bad for Ni)
For details, see Jeanloz, 1990, Annu. Rev. Earth Planet. Sci., 18, 357-386.
Inner Core solid cristallyed Fe-Ni alloy
- -> may be partially molten
- -> likely to be convectively unstable on very long time scales (see mantle)
- -> seismic travel time anomalies interpreted as a preferred orientation of the
- cristals rather than lateral heterogeneities
- this seismic anisotropy is caused by:
- 1. solid-state convection inducing a preferred orientation of crystallites
- or
- 2. crystal growth with a preferred orientation
Temperature:
- - at CMB: 4000 ± 500 K
- - centre: 5000-6000 K
CMB, core side: mush zone
O, Si, Mg intermixed within iron-alloy fluid core-mantle reaction in mush zone
=> composition of core increasingly contaminated by mantle (O most important)