The Transits of Extrasolar Planets with Moons

2011
ISBN: 978-3-642-27120-5
Verlag: Springer

Buch, Englisch, 200 Seiten, Previously published in hardcover, Format (B × H): 155 mm x 235 mm, Gewicht: 341 g

Reihe: Springer Theses

Can we detect the moons of extrasolar planets? For two decades, astronomers have made enormous progress in the detection and characterisation of exoplanetary systems but the identification of an "exomoon" is notably absent.
In this thesis, David Kipping shows how transiting planets may be used to infer the presence of exomoons through deviations in the time and duration of the planetary eclipses. A detailed account of the transit model, potential distortions, and timing techniques is covered before the analytic forms for the timing
variations are derived. It is shown that habitable-zone exomoons above 0.2 Earth-masses are detectable with the Kepler space telescope using these new timing techniques.

Zielgruppe

Research

Autoren/Hrsg.

Kipping, David M.

Fachgebiete

• Naturwissenschaften Astronomie Astrophysik
• Naturwissenschaften Physik Angewandte Physik Astrophysik
• Naturwissenschaften Astronomie Galaxien und Sterne
• Naturwissenschaften Astronomie Astronomische Beobachtung: Observatorien, Instrumente, Methoden

Inhaltsverzeichnis

1 Introduction.- 2 Extrasolar Moons.- 3 The Transiting Planet.- 4 Timing the Transit.- 5 Transit Distortions.- 6 Transit Timing Effects due to an Exomoon.- 7 Detectability of Habitable Exomoons with Kepler-Class Photometry.- 8 Conclusions & Future Work.- A Notations & Acronyms.

Über Autor(innen)

Dr. Kipping got his PhD in Astrophysics from University College London in 2011. He is Carl Sagan Fellow at Harvard College Observatory.