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Dynamics of Orbiting Systems: Topics in Migration and Resonance
Dynamics of Orbiting Systems: Topics in Migration and Resonance
Dynamics of Orbiting Systems: Topics in Migration and Resonance

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자료유형  
 학위논문 서양
최종처리일시  
20260202104718
ISBN  
9798293826216
DDC  
520
저자명  
Laune, Jordan.
서명/저자  
Dynamics of Orbiting Systems: Topics in Migration and Resonance
발행사항  
[Sl] : Cornell University, 2025
발행사항  
Ann Arbor : ProQuest Dissertations & Theses, 2025
형태사항  
182 p
주기사항  
Source: Dissertations Abstracts International, Volume: 87-03, Section: B.
주기사항  
Advisor: Lai, Dong.
학위논문주기  
Thesis (Ph.D.)--Cornell University, 2025.
초록/해제  
요약A common class of astrophysical systems consists of smaller bodies orbiting a more massive central object. The orbits of the smaller bodies usually change over their lifetime, this is referred to as orbital migration. Resonance-where two system frequencies align-is one of the strongest indicators of smooth orbital migration, as the sweeping of frequencies over time enables capture. For example, many exoplanet systems have been observed to be in mean motion resonance, where their orbital periods are related by an integer ratio. This configuration is usually attributed to smooth, disk-driven migration. In this thesis, I investigate three topics concerning migration and resonance. The first topic I investigate is the effect of gas accretion on a migrating planet. I show that orbital migration is outward in my model, contrary to the classic picture of planet migration. Secondly, I determine the disk conditions which lead to apsidal alignment and antialignment in resonant exoplanet systems. I demonstrate that a force which drives eccentricities can potentially explain aligned systems. Lastly, I study the effect that differential apsidal precession has on resonance capture. I identify both a resonance overlap threshold and a secular resonance that can disrupt capture.
일반주제명  
Astronomy
일반주제명  
Astrophysics
일반주제명  
Planetology
키워드  
Accretion disks
키워드  
Planet migration
키워드  
Planetary systems
키워드  
Resonance
기타저자  
Cornell University Astronomy and Space Sciences
기본자료저록  
Dissertations Abstracts International. 87-03B.
전자적 위치 및 접속  
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MARC

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■020    ▼a9798293826216
■035    ▼a(MiAaPQ)AAI32120630
■040    ▼aMiAaPQ▼cMiAaPQ
■0820  ▼a520
■1001  ▼aLaune,  Jordan.▼0(orcid)0000-0002-0896-7393
■24510▼aDynamics  of  Orbiting  Systems:  Topics  in  Migration  and  Resonance
■260    ▼a[Sl]▼bCornell  University▼c2025
■260  1▼aAnn  Arbor▼bProQuest  Dissertations  &  Theses▼c2025
■300    ▼a182  p
■500    ▼aSource:  Dissertations  Abstracts  International,  Volume:  87-03,  Section:  B.
■500    ▼aAdvisor:  Lai,  Dong.
■5021  ▼aThesis  (Ph.D.)--Cornell  University,  2025.
■520    ▼aA  common  class  of  astrophysical  systems  consists  of  smaller  bodies  orbiting  a  more  massive  central  object.  The  orbits  of  the  smaller  bodies  usually  change  over  their  lifetime,  this  is  referred  to  as  orbital  migration.  Resonance-where  two  system  frequencies  align-is  one  of  the  strongest  indicators  of  smooth  orbital  migration,  as  the  sweeping  of  frequencies  over  time  enables  capture.  For  example,  many  exoplanet  systems  have  been  observed  to  be  in  mean  motion  resonance,  where  their  orbital  periods  are  related  by  an  integer  ratio.  This  configuration  is  usually  attributed  to  smooth,  disk-driven  migration.  In  this  thesis,  I  investigate  three  topics  concerning  migration  and  resonance.  The  first  topic  I  investigate  is  the  effect  of  gas  accretion  on  a  migrating  planet.  I  show  that  orbital  migration  is  outward  in  my  model,  contrary  to  the  classic  picture  of  planet  migration.  Secondly,  I  determine  the  disk  conditions  which  lead  to  apsidal  alignment  and  antialignment  in  resonant  exoplanet  systems.  I  demonstrate  that  a  force  which  drives  eccentricities  can  potentially  explain  aligned  systems.  Lastly,  I  study  the  effect  that  differential  apsidal  precession  has  on  resonance  capture.  I  identify  both  a  resonance  overlap  threshold  and  a  secular  resonance  that  can  disrupt  capture.
■590    ▼aSchool  code:  0058.
■650  4▼aAstronomy
■650  4▼aAstrophysics
■650  4▼aPlanetology
■653    ▼aAccretion  disks
■653    ▼aPlanet  migration
■653    ▼aPlanetary  systems
■653    ▼aResonance
■690    ▼a0606
■690    ▼a0596
■690    ▼a0590
■71020▼aCornell  University▼bAstronomy  and  Space  Sciences.
■7730  ▼tDissertations  Abstracts  International▼g87-03B.
■790    ▼a0058
■791    ▼aPh.D.
■792    ▼a2025
■793    ▼aEnglish
■85640▼uhttp://www.riss.kr/pdu/ddodLink.do?id=T17358548▼nKERIS▼z이  자료의  원문은  한국교육학술정보원에서  제공합니다.

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