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UCL Earth Sciences

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Planet Dynamics and Evolution

The Earth’s inner core, outer core, lower mantle, upper mantle, the lithosphere, the surfaces and interiors of the Moon, Mars and Venus, meteorites, and, icy moons.

Planet Dynamics and Evolution
Our research covers a wide range of areas spanning the Earth’s inner core, outer core, lower mantle, upper mantle, the lithosphere, the surfaces and interiors of the Moon, Mars and Venus, meteorites, and, more recently, the evolution and interiors of the icy moons such as Titan. The overarching rationale is to understand the properties, behaviour and evolution of the Earth and the other planetary bodies, and their place within the solar system. We use computational mineral physics, experimental mineral physics, field observations and experiments, planetary mission data, thermal evolution models and geodynamic models. 

 

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Research highlights include:

  • Pre-melting in the Earth’s inner core (Vocadlo, Brodholt, Wood)
  • Nickel is “transparent” in the inner core, but as a result of temperature, not composition. (Vocadlo, Brodholt, Wood)
  • The phase diagram of NiSi. (Wood, Dobson, Vocadlo)
  • The stability and elasticity of phases of iron. (Vocadlo, Wood, Brodholt, Dobson)
  • Electrical and Thermal conductivity of the Earth's core are 2-3 times higher than previously estimated. (Pozzo and Alfe`)
  • New estimates of the concentrations of oxygen, silicon and sulphur in the core based on ab initio thermodynamic calculations. (Alfe)
  • Melting curve of iron at Earth's core conditions. (Alfe)
  • High temperature ab initio simulations provide the first robust high-temperature and pressure estimates for the elastic properties of pervoskite and post-perovskite (Brodholt)
  • High-pressure apparatus capable of performing the first controlled rheology experiments under lower mantle conditions (Dobson)
  • The first laboratory experiment that shows that intermediate seismicity can be caused by the dehydration of serpentine (Dobson)
  • Evidence that impact melting is viable alternative to mantle plumes for the formation of a large igneous provinces (Jones)