The formation of the Solar System Lecture Series The Solar System

The formation of the Solar System

  1. The event took place on
Ricardo Hueso Alonso

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  1. Ricardo Hueso AlonsoRicardo Hueso Alonso

    Es Doctor en Ciencias Físicas y profesor titular en la Escuela Técnica Superior de Ingenieros de Bilbao de la Universidad del País Vasco. En su trayectoria como investigador ha trabajado en diversas áreas del Sistema Solar, principalmente en el estudio de las atmósferas densas de planetas gigantes como Júpiter y Saturno y también en las atmósferas de Venus y Titán, la mayor de las lunas de Saturno. Paralelamente también ha trabajado en la evolución temprana del Sistema Solar, la formación de planetas gigantes como Júpiter y en la formación de sistemas planetarios extrasolares. Ricardo Hueso es autor de más de 50 artículos de investigación en revistas especializadas destacando varias publicaciones en Nature.

The Solar System was formed around 4670 million years ago from a cloud of gas an dust which formed the central star and a circumstellar disk. The current structure of our solar system with the rocky planets in the inside, like Earth and Mars, and the formation of giant exterior planets like Jupiter and Saturn, speaks to us about the physical processes that took place in that time when our planetary system took shape. In parallel, the astrophysicist are obtaining a growing number of observations from similar disks around very young stars that allow us to study live the formation of planets in those stars. In our Solar System the exterior planets (the gas giants Jupiter and Saturn, and the  frozen giants Uranus and Neptune) formed rapidly due to an abundance of light materials acquiring enough mass to attract hydrogen gas of the protosolar nebula and gravitationally dominate its surroundings. The interior planets took much longer to form due to a lower amount of condensable materials in the temperature conditions that existed in the interior Solar System, with and estimated range of time between 50 and 100 million years to have the interior Solar System fully formed. This formation of the interior solar system was dominated by violent collisions between thousands of protoplanets and billions of much smaller planetesimals. In this conference we will make special emphasis on the details of the formation of the terrestrial planets, and the Earth-Moon system in particular, which was formed as a consequence of one of those planetary impacts.