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UID:37@osups.universite-paris-saclay.fr
DTSTART;TZID=Europe/Paris:20251204T110000
DTEND;TZID=Europe/Paris:20251204T120000
DTSTAMP:20251114T130226Z
URL:https://osups.universite-paris-saclay.fr/calendrier/forming-giant-plan
 ets-in-protoplanetary-disks/
SUMMARY:Forming giant planets in protoplanetary disks
DESCRIPTION:par Camille Bergez-Casalou (IAS)\n\nAbstract: Planets are forme
 d from the dust and gas in rotation around newborn stars\, called protopla
 netary disks. In particular\, gaseous giant planets (like Jupiter or Satur
 n) must have acquired their gaseous envelop during the lifetime of the pro
 toplanetary disk. Understanding how planets interact with their surroundin
 g disk is primordial to understand how they formed and lead to the populat
 ion of exoplanets that we observe today. In this talk\, I will present how
  we link hydrodynamical simulations of growing giant planets to the observ
 ations of disks\, with both ALMA and JWST. Gas accreting planets will have
  an impact on the global disk structure\, forming gaps. These ones can be 
 observed with ALMA and be indirectly linked to the characteristics of the 
 planet. Moreover\, the JWST has the sensitivity to observe disks around lo
 w mass objects and characterize how it accretes from its disk. I will disc
 uss in which framework these objects can be seen as scaled up versions of 
 planetary mass objects.\n\nLieu : salle 1-2-3 (Bât.121)
CATEGORIES:Séminaires
LOCATION:IAS\, Bât. 121 rue Jean Teillac\, Orsay\, 91400\, France
X-APPLE-STRUCTURED-LOCATION;VALUE=URI;X-ADDRESS=Bât. 121 rue Jean Teillac\
 , Orsay\, 91400\, France;X-APPLE-RADIUS=100;X-TITLE=IAS:geo:0,0
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TZID:Europe/Paris
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