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SUMMARY:Dynamics of dust and gas in protoplanetary disks with massive embe
 dded planets - Hannah Petrovic (University of Cambridge)
DTSTART:20221109T131500Z
DTEND:20221109T134000Z
UID:TALK192584@talks.cam.ac.uk
CONTACT:Hannah Uebler
DESCRIPTION:Whilst the formation of planets continues to have many unknown
 s\, the recent theory of pebble accretion has unveiled a pathway through w
 hich the formation of planets can be accelerated compared to the standard 
 core accretion model. These pebbles are of particular interest given recen
 t imaging with ALMA\, highlighting rings and other disk substructures in t
 he dust. Here I explore the motion of dust and gas in protoplanetary disks
  with massive embedded planets using 3D hydrodynamic simulations. In parti
 cular\, I investigate the consequences of planetary masses above the so-ca
 lled pebble isolation mass on the dust and gas behaviour. I will go on to 
 broadly speak about the importance of these results on resulting disk and 
 planet compositions.
LOCATION:The Hoyle Lecture Theatre + Zoom 
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