The role of planetary formation and evolution in shaping the composition of exoplanetary atmospheres

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• 作者：D. Turrini ; R. P. Nelson ; M. Barbieri
• 关键词：Planetary formation ; Migration ; Atmospheres ; Giant planets ; Space missions ; Extrasolar planets
• 刊名：Experimental Astronomy
• 出版年：2015
• 出版时间：December 2015
• 年：2015
• 卷：40
• 期：2-3
• 页码：501-522
• 全文大小：1,055 KB
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• 作者单位：D. Turrini (1)
  R. P. Nelson (2)
  M. Barbieri (3)
  
  1. Istituto di Astrofisica e Planetologia Spaziali INAF-IAPS, Via Fosso del Cavaliere 100, 00133, Rome, Italy
  2. School of Physics and Astronomy, Queen Mary University of London, Mile End Road, London, E1 4NS, U.K.
  3. Centro Interdipartimentale di Studi e Attività Spaziali CISAS, Università di Padova, Via Venezia 15, 35131, Padova, Italy
  
• 刊物类别：Physics and Astronomy
• 刊物主题：Physics
  Astronomy
  Statistics for Engineering, Physics, Computer Science, Chemistry and Geosciences
  
• 出版者：Springer Netherlands
• ISSN：1572-9508

文摘

Over the last twenty years, the search for extrasolar planets has revealed the rich diversity of outcomes from the formation and evolution of planetary systems. In order to fully understand how these extrasolar planets came to be, however, the orbital and physical data we possess are not enough, and they need to be complemented with information about the composition of the exoplanets. Ground-based and space-based observations provided the first data on the atmospheric composition of a few extrasolar planets, but a larger and more detailed sample is required before we can fully take advantage of it. The primary goal of a dedicated space mission like the Exoplanet Characterization Observatory (EChO) proposal is to fill this gap and to expand the limited data we possess by performing a systematic survey of extrasolar planets. The full exploitation of the data that space-based and ground-based facilities will provide in the near future, however, requires knowledge about the sources and sinks of the chemical species and molecules that will be observed. Luckily, the study of the past history of the Solar System provides several indications about the effects of processes like migration, late accretion and secular impacts, and on the time they occur in the life of planetary systems. In this work we will review what is already known about the factors influencing the composition of planetary atmospheres, focusing on the case of gaseous giant planets, and what instead still need to be investigated. Keywords Planetary formation Migration Atmospheres Giant planets Space missions Extrasolar planets