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DTSTART:20171029T010000
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DTSTART:20180325T010000
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DTSTART;TZID=Europe/Paris:20180329T130000
DTEND;TZID=Europe/Paris:20180329T140000
DTSTAMP:20260408T154841
CREATED:20180131T211858Z
LAST-MODIFIED:20180324T213728Z
UID:314-1522328400-1522332000@www.naxys.be
SUMMARY:Jean Teyssandier (Cornell University\, USA)
DESCRIPTION:Title: Orbital evolution during planet-⁠disc interactions \nAbstract: The origin and wide distribution of eccentricities and inclinations in planetary systems remains to be explained\, in particular in the context of planet-disc interactions. In this talk I will present a study of the evolution of eccentricity in discs and planets that combines methods from celestial mechanics and hydrodynamics\, and takes the form of a linear secular theory. I will compare the predictions of this linear theory against direct hydrodynamical simulations and show how eccentricity can grow. I will discuss what these results imply for the orbital structure of protoplanetary discs and young planetary systems. I will also discuss how moderate inclinations can be generated via similar mechanisms.
URL:https://www.naxys.be/event/jean-teyssandier-cornell-university-usa/
LOCATION:E25
CATEGORIES:NAXYS Seminar
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