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Exploring the Architecture of Transiting Exoplanetary Systems with High-Precision Photometry

  • Kento Masuda

Part of the Springer Theses book series (Springer Theses)

About this book

Introduction

This thesis develops and establishes several methods to determine the detailed geometric architecture of transiting exoplanetary systems (planets orbiting around, and periodically passing in front of, stars other than the sun) using high-precision photometric data collected by the Kepler space telescope. It highlights the measurement of stellar obliquity – the tilt of the stellar equator with respect to the planetary orbital plane(s) – and presents methods for more precise obliquity measurements in individual systems of particular interest, as well as for measurements in systems that have been out of reach of previous methods. Such information is useful for investigating the dynamical evolution of the planetary orbit, which is the key to understanding the diverse architecture of exoplanetary systems. The thesis also demonstrates a wide range of unique applications of high-precision photometric data, which expand the capability of future space-based photometry.

Keywords

Transiting Exoplanet Formation of Hot Jupiters Kepler Space Telescope Stellar Obliquity The Rossiter-Mclaughlin Effect Gravity Darkening Asteroseismology Transit Timing Variations Exoplanetary Systems Stellar Spin and Planetary Orbital Axes

Authors and affiliations

  • Kento Masuda
    • 1
  1. 1.Department of Astrophysical SciencesPrinceton UniversityPrincetonUSA

Bibliographic information

  • DOI https://doi.org/10.1007/978-981-10-8453-9
  • Copyright Information Springer Nature Singapore Pte Ltd. 2018
  • Publisher Name Springer, Singapore
  • eBook Packages Physics and Astronomy
  • Print ISBN 978-981-10-8452-2
  • Online ISBN 978-981-10-8453-9
  • Series Print ISSN 2190-5053
  • Series Online ISSN 2190-5061
  • Buy this book on publisher's site
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