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The Galactic Terrestrial Zone in a Cosmological Context

People Involved

Professor Brad Gibson

Project Description

The mineralogy of terrestrial planets is controlled by the elemental ratios of carbon-to-oxygen and magnesium-to-silicon. Earth-like planets are shaped by rock-forming oxide species, predominantly in the form of magnesium silicates such as olivine and pyroxene. Conversely, material rich in carbon with respect to oxygen leads to terrestrial planets rich in various carbide species and graphite. Informed by recent developments in the simulation of terrestrial planets and the statistics of planet-host star chemistry, the proposed student will model the evolution of the Milky Way and trace the spatial and temporal distribution of C/O and Mg/Si, identifying the fraction of the stars in our Galaxy that lie within what we call the Galactic Terrestrial Zone (GTZ). Of the 10 billion (roughly solar mass) stars in the GTZ today, we will predict what fraction formed from proto-planetary material with a chemical composition suitable for the formation of Earth-like extra-solar planets (low C/O; high Mg/Si), and what fraction form within Galactic pockets rich in the radiogenic isotopes crucial for heating terrestrial planets. Both semi-numerical Galactic Chemical Evolution models and fully cosmological chemo-dynamical simulations will be employed.

Status Project Complete
Value £1,200.00
Project Dates Jul 17, 2017 - Sep 1, 2018
Partner Organisations No Partners

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