Exploring the architecture of transiting exoplanetary systems with high-precision photometry /
General Material Designation
[Book]
First Statement of Responsibility
by Kento Masuda.
.PUBLICATION, DISTRIBUTION, ETC
Place of Publication, Distribution, etc.
Singapore :
Name of Publisher, Distributor, etc.
Springer,
Date of Publication, Distribution, etc.
2018.
PHYSICAL DESCRIPTION
Specific Material Designation and Extent of Item
1 online resource (XIV, 160 pages) :
Other Physical Details
illustrations
SERIES
Series Title
Springer Theses, Recognizing Outstanding Ph. D. Research,
ISSN of Series
2190-5053
INTERNAL BIBLIOGRAPHIES/INDEXES NOTE
Text of Note
Includes bibliographical references.
CONTENTS NOTE
Text of Note
Diversity of the Extrasolar Worlds -- Measurements of Stellar Obliquities -- Origin of the Misaligned Hot Jupiters: Nature or Nurture? -- Three-dimensional Stellar Obliquities of HAT-P-7 and Kepler-25 from Joint Analysis of Asteroseismology, Transit Light Curve, and the Rossiter-McLaughlin E.
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SUMMARY OR ABSTRACT
Text of Note
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.