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University of Cambridge

The Structure of Extrasolar Planetesimal Belts in Images

Abstract

dc:description.abstract

Solid bodies in the form of planets and planetesimal belts familiar to us in the Solar System are also a prevalent feature around other stars. Their great diversity highlights a lack of complete theories for how they formed, which is further complicated by observational challenges to understand their full architecture in the first place. Currently, our best observational constraints on the outer planetary system come from imaging the planetesimal belts that population this region, known as debris disks. As planets dynamically interact with the disk throughout their formation and evolution, structures reflecting their history are imprinted on the disk. In this thesis, I develop systematic and unbiased methods to recover the three-dimensional structure of debris disks from their images applicable to a versatile range of imaging modes. By removing assumptions on the functional form of the disk structure, this method provides unbiased constraints on disk substructures with realistic uncertainties that enable us to interpret dynamical interactions shaping the planetary system. I apply this method to a sample of debris disks with resolved imaging to infer general three-dimensional structures of debris disks and their implications for planetary system formation. For the archetypal edge-on debris disk of β Pictoris for which multiple epochs of high-resolution mid-infrared and millimetre images are available, I model in detail its vertical structure for different grain sizes and any variations in azimuthal substructures across time, constraining dynamical scenarios that could be shaping the evolution of the system. The approaches developed in this work to model debris disk structures from images will be important for interpreting upcoming observations with ALMA, JWST and the next generation of observatories at high sensitivity and resolution.

Degree

thesis:*
Name dc:type.qualificationname
Doctor of Philosophy (PhD)
Level dc:type.qualificationlevel
Doctoral
Grantor dc:publisher.institution
University of Cambridge
Year dc:date.issued
2024

Author and committee

dc:creator, dc:contributor.*
Author dc:creator
  • Han, Yinuo
Advisor dc:contributor.advisor
  • Wyatt, Mark

Subjects

dc:subject × 10

Rights

dc:rights
Language dc:language
eng

Identifiers

dc:identifier.*
DOI dc:identifier.doi
https://doi.org/10.17863/CAM.112947
OAI identifier oai:identifier
oai:www.repository.cam.ac.uk:1810/375181

Chain of custody

source
Harvested from
Cambridge University
Base URL
api.repository.cam.ac.uk/server/oai/request
Last updated
2026-07-24
Source record
OAI-PMH GetRecord
citation

Han, Yinuo. The Structure of Extrasolar Planetesimal Belts in Images. Doctoral thesis, University of Cambridge, 2024. https://doi.org/10.17863/CAM.112947