Master thesis defense by Jacob Krag Nørgaard
Modeling Water Transport and Ice-Line Evolution in Protoplanetary Disks
Abstract
Recent observations of protoplanetary disks with telescopes and interferometers such as the James Webb Space Telescope (JWST) and the Atacama Large Millimeter/submillimeter Array (ALMA) reveal a wide range of water, carbon dioxide, and hydrocarbon abundances.
A luminosity burst-type heating event shows that temporary heating can shift the ice line outward and leave a long-lived, grain-size-dependent imprint as vapor recondenses mainly onto small grains. This work demonstrates that simplified descriptions of the volatile ice line as temperature-defined boundaries miss important aspects of disk evolution. The distribution of water ice and vapor is history-dependent, meaning that the volatile composition observed at a given time may reflect earlier stages of dust growth, transport, and heating. These results highlight the need to treat dust and volatile evolution self-consistently when assessing the volatile material available for planet formation.
Supervisors
Troels Haugbølle, Adrien Houge, Michael Küffmeier, and Giulia Perotti
Censor
Hans Kjeldsen, AU