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The Transits of Extrasolar Planets with Moons
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...
| Clasificación: | Libro Electrónico |
|---|---|
| Autor principal: | |
| Autor Corporativo: | |
| Formato: | Electrónico eBook |
| Idioma: | Inglés |
| Publicado: |
Berlin, Heidelberg :
Springer Berlin Heidelberg : Imprint: Springer,
2011.
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| Edición: | 1st ed. 2011. |
| Colección: | Springer Theses, Recognizing Outstanding Ph.D. Research,
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| Temas: | |
| Acceso en línea: | Texto Completo |
MARC
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| 001 | 978-3-642-22269-6 | ||
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| 005 | 20220207082728.0 | ||
| 007 | cr nn 008mamaa | ||
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| 020 | |a 9783642222696 |9 978-3-642-22269-6 | ||
| 024 | 7 | |a 10.1007/978-3-642-22269-6 |2 doi | |
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| 100 | 1 | |a Kipping, David M. |e author. |4 aut |4 http://id.loc.gov/vocabulary/relators/aut | |
| 245 | 1 | 4 | |a The Transits of Extrasolar Planets with Moons |h [electronic resource] / |c by David M. Kipping. |
| 250 | |a 1st ed. 2011. | ||
| 264 | 1 | |a Berlin, Heidelberg : |b Springer Berlin Heidelberg : |b Imprint: Springer, |c 2011. | |
| 300 | |a XVII, 200 p. 42 illus., 2 illus. in color. |b online resource. | ||
| 336 | |a text |b txt |2 rdacontent | ||
| 337 | |a computer |b c |2 rdamedia | ||
| 338 | |a online resource |b cr |2 rdacarrier | ||
| 347 | |a text file |b PDF |2 rda | ||
| 490 | 1 | |a Springer Theses, Recognizing Outstanding Ph.D. Research, |x 2190-5061 | |
| 505 | 0 | |a 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. | |
| 520 | |a 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. | ||
| 650 | 0 | |a Astronomy-Observations. | |
| 650 | 0 | |a Planetary science. | |
| 650 | 0 | |a Astrobiology. | |
| 650 | 0 | |a Astrophysics. | |
| 650 | 1 | 4 | |a Astronomy, Observations and Techniques. |
| 650 | 2 | 4 | |a Planetary Science. |
| 650 | 2 | 4 | |a Astrobiology. |
| 650 | 2 | 4 | |a Astrophysics. |
| 710 | 2 | |a SpringerLink (Online service) | |
| 773 | 0 | |t Springer Nature eBook | |
| 776 | 0 | 8 | |i Printed edition: |z 9783642271205 |
| 776 | 0 | 8 | |i Printed edition: |z 9783642222689 |
| 776 | 0 | 8 | |i Printed edition: |z 9783642222702 |
| 830 | 0 | |a Springer Theses, Recognizing Outstanding Ph.D. Research, |x 2190-5061 | |
| 856 | 4 | 0 | |u https://doi.uam.elogim.com/10.1007/978-3-642-22269-6 |z Texto Completo |
| 912 | |a ZDB-2-PHA | ||
| 912 | |a ZDB-2-SXP | ||
| 950 | |a Physics and Astronomy (SpringerNature-11651) | ||
| 950 | |a Physics and Astronomy (R0) (SpringerNature-43715) | ||