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LCLU Coffee - How to Build a PlanetAdd to your list(s) Download to your calendar using vCal
If you have a question about this talk, please contact Paul B. Rimmer. Rapid accretion of rocky planets and the outgassing of their first atmospheres Terrestrial planets have traditionally been thought to form by collisions between protoplanets taking place mostly after the dissipation of the protoplanetary disc, on time-scales of 30-100 million years. I present here a new theoretical model where terrestrial planets grow instead by accreting small pebbles in the protoplanetary disc within 3-5 million years. I discuss how the immense pebble accretion heat leads to extensive melting of the growing planets and to the emergence of deep magma oceans. Volatiles such as water, carbon and nitrogen are accreted with the pebbles and partitioned between atmosphere, magma ocean and core. The end of the accretion phase leads to rapid crystallisation of the magma ocean and outgassing of the first atmosphere. I will show how the atmospheric composition of young planets is key to understanding the origin of life. This talk is part of the LCLU Coffee Meetings series. This talk is included in these lists:Note that ex-directory lists are not shown. |
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