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Planets Are Not Points: The Profound Effect of Planetary Structure on Exoplanet System Architectures
Planets Are Not Points: The Profound Effect of Planetary Structure on Exoplanet System Architectures
상세정보
- 자료유형
- 학위논문 서양
- 최종처리일시
- 20260202103012
- ISBN
- 9798286443857
- DDC
- 520
- 저자명
- Lu, Tiger C.
- 서명/저자
- Planets Are Not Points: The Profound Effect of Planetary Structure on Exoplanet System Architectures
- 발행사항
- [Sl] : Yale University, 2025
- 발행사항
- Ann Arbor : ProQuest Dissertations & Theses, 2025
- 형태사항
- 209 p
- 주기사항
- Source: Dissertations Abstracts International, Volume: 86-12, Section: B.
- 주기사항
- Advisor: Rice, Malena.
- 학위논문주기
- Thesis (Ph.D.)--Yale University, 2025.
- 초록/해제
- 요약The quantity and quality of astronomical data has advanced to the point in which truly detailed and nuanced theoretical models are necessary. In the field of exoplanetary dynamics, it has become increasingly clear that we must account for the effects of planetary structure when considering the dynamics of the system. In other words, Planets are not Points. This dissertation details my contributions to the field of exoplanet dynamics, split into three subcategories:• Part I (Chapters 2 - 3): Numerical Methods & the N-Body Problem. These chapters discusses the numerical methods I have developed to study the analytically unsolvable N-Body problem, and details their implementation into the popular open-source software REBOUND.• Part II (Chapters 4 - 5): Spin-Orbit Dynamics. These chapters explore my work into the complex interplay between a planet's spin and it's motion, driven by tidal forces. I present an origin story for the large obliquity of the planet Uranus, and I show that such large obliquity can also explain the anomalously low density of the super-puff planet HIP-41378 f.• Part III (Chapter 6). Coupled Planetary Structure and Dynamical Evolution. This chapter details my work into self-consistent evolution of a planet's interior structure and the system's dynamical evolution. I present a case study of the intriguing HAT-P-11 system, a dynamical puzzle that can only be explained via truly self-consistent evolution.
- 일반주제명
- Astronomy
- 일반주제명
- Astrophysics
- 일반주제명
- Physics
- 키워드
- Planets
- 키워드
- N-Body problem
- 기타저자
- Yale University Astronomy
- 기본자료저록
- Dissertations Abstracts International. 86-12B.
- 전자적 위치 및 접속
- 로그인 후 원문을 볼 수 있습니다.
MARC
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■00520260202103012
■006m o d
■007cr#unu||||||||
■020 ▼a9798286443857
■035 ▼a(MiAaPQ)AAI31842717
■040 ▼aMiAaPQ▼cMiAaPQ
■0820 ▼a520
■1001 ▼aLu, Tiger C.
■24510▼aPlanets Are Not Points: The Profound Effect of Planetary Structure on Exoplanet System Architectures
■260 ▼a[Sl]▼bYale University▼c2025
■260 1▼aAnn Arbor▼bProQuest Dissertations & Theses▼c2025
■300 ▼a209 p
■500 ▼aSource: Dissertations Abstracts International, Volume: 86-12, Section: B.
■500 ▼aAdvisor: Rice, Malena.
■5021 ▼aThesis (Ph.D.)--Yale University, 2025.
■520 ▼aThe quantity and quality of astronomical data has advanced to the point in which truly detailed and nuanced theoretical models are necessary. In the field of exoplanetary dynamics, it has become increasingly clear that we must account for the effects of planetary structure when considering the dynamics of the system. In other words, Planets are not Points. This dissertation details my contributions to the field of exoplanet dynamics, split into three subcategories:• Part I (Chapters 2 - 3): Numerical Methods & the N-Body Problem. These chapters discusses the numerical methods I have developed to study the analytically unsolvable N-Body problem, and details their implementation into the popular open-source software REBOUND.• Part II (Chapters 4 - 5): Spin-Orbit Dynamics. These chapters explore my work into the complex interplay between a planet's spin and it's motion, driven by tidal forces. I present an origin story for the large obliquity of the planet Uranus, and I show that such large obliquity can also explain the anomalously low density of the super-puff planet HIP-41378 f.• Part III (Chapter 6). Coupled Planetary Structure and Dynamical Evolution. This chapter details my work into self-consistent evolution of a planet's interior structure and the system's dynamical evolution. I present a case study of the intriguing HAT-P-11 system, a dynamical puzzle that can only be explained via truly self-consistent evolution.
■590 ▼aSchool code: 0265.
■650 4▼aAstronomy
■650 4▼aAstrophysics
■650 4▼aPhysics
■653 ▼aPlanets
■653 ▼aPlanetary structure
■653 ▼aExoplanet dynamics
■653 ▼aN-Body problem
■690 ▼a0606
■690 ▼a0596
■690 ▼a0605
■71020▼aYale University▼bAstronomy.
■7730 ▼tDissertations Abstracts International▼g86-12B.
■790 ▼a0265
■791 ▼aPh.D.
■792 ▼a2025
■793 ▼aEnglish
■85640▼uhttp://www.riss.kr/pdu/ddodLink.do?id=T17356658▼nKERIS▼z이 자료의 원문은 한국교육학술정보원에서 제공합니다.
