行星形成和揮發性原材流落到類地行星



本文章最後由 iheby 於 2016-11-25 23:01 編輯

iheby 發表於 2016-11-20 01:33
脈衝星狀態切換,脈衝輪廓不穩定性和計時噪聲 @香港大學物理學系

行星形成和揮發性原材流落到類地行星 @香港大學 物理學系+地科科學系
 
 
Joint SEMINAR:- Planet Formation and Volatile Delivery to Terrestrial Planets 
 
Due to the enormous discovery of exoplanets, planet formation theory is changing. This talk will present current understanding and discuss difficulty of planet formation. Formation of planetesimals – the building blocks of planets - and orbital migration of planets are the most serious problems. Based on these, the speaker will discuss the delivery of water(H2O), Carbon(C) and Nitrogen(N) to the Earth. Life is made of C and N and they may have been formed by chemical evolution in liquid water. Because these compounds are volatile, they would not be included in planetesimals around Earth‘s orbit, so that they must be condensed in outer regions and delivered to the Earth by some mechanism. Although there could be many planets in the so-called "habitable zones", in which ocean can exist on their surface, they cannot really harbor life unless H2O, C and N are delivered to the planets. 
 
時間:2016.12.02(五) 16:00 
地點:香港大學 莊月明物理樓522室 
講者:井田 茂 教授 Prof. Shigeru Ida (東京工業大學 地球生命研究所) 
語言:英語 

免費會議,歡迎參加

【訊息由張詠倫提供】

此活動由香港大學物理學系主辦。

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