System Geometries and Transit/Eclipse Probabilities

Transiting exoplanets provide access to data to study the mass-radius relation and internal structure of extrasolar planets. Long-period transiting planets allow insight into planetary environments similar to the Solar System where, in contrast to hot Jupiters, planets are not constantly exposed...

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Main Authors: Howard A., Mahadevan S., Laughlin G., Kane S. R., von Braun K., Ciardi D. R.
Format: Article
Language:English
Published: EDP Sciences 2011-02-01
Series:EPJ Web of Conferences
Online Access:http://dx.doi.org/10.1051/epjconf/20101106006
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author Howard A.
Mahadevan S.
Laughlin G.
Kane S. R.
von Braun K.
Ciardi D. R.
author_facet Howard A.
Mahadevan S.
Laughlin G.
Kane S. R.
von Braun K.
Ciardi D. R.
author_sort Howard A.
collection DOAJ
description Transiting exoplanets provide access to data to study the mass-radius relation and internal structure of extrasolar planets. Long-period transiting planets allow insight into planetary environments similar to the Solar System where, in contrast to hot Jupiters, planets are not constantly exposed to the intense radiation of their parent stars. Observations of secondary eclipses additionally permit studies of exoplanet temperatures and large-scale exo-atmospheric properties. We show how transit and eclipse probabilities are related to planet-star system geometries, particularly for long-period, eccentric orbits. The resulting target selection and observational strategies represent the principal ingredients of our photometric survey of known radial-velocity planets with the aim of detecting transit signatures (TERMS).
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spelling doaj.art-98ac4dd092654fdfa0230cc35972cc572022-12-21T23:15:49ZengEDP SciencesEPJ Web of Conferences2100-014X2011-02-01110600610.1051/epjconf/20101106006System Geometries and Transit/Eclipse ProbabilitiesHoward A.Mahadevan S.Laughlin G.Kane S. R.von Braun K.Ciardi D. R.Transiting exoplanets provide access to data to study the mass-radius relation and internal structure of extrasolar planets. Long-period transiting planets allow insight into planetary environments similar to the Solar System where, in contrast to hot Jupiters, planets are not constantly exposed to the intense radiation of their parent stars. Observations of secondary eclipses additionally permit studies of exoplanet temperatures and large-scale exo-atmospheric properties. We show how transit and eclipse probabilities are related to planet-star system geometries, particularly for long-period, eccentric orbits. The resulting target selection and observational strategies represent the principal ingredients of our photometric survey of known radial-velocity planets with the aim of detecting transit signatures (TERMS).http://dx.doi.org/10.1051/epjconf/20101106006
spellingShingle Howard A.
Mahadevan S.
Laughlin G.
Kane S. R.
von Braun K.
Ciardi D. R.
System Geometries and Transit/Eclipse Probabilities
EPJ Web of Conferences
title System Geometries and Transit/Eclipse Probabilities
title_full System Geometries and Transit/Eclipse Probabilities
title_fullStr System Geometries and Transit/Eclipse Probabilities
title_full_unstemmed System Geometries and Transit/Eclipse Probabilities
title_short System Geometries and Transit/Eclipse Probabilities
title_sort system geometries and transit eclipse probabilities
url http://dx.doi.org/10.1051/epjconf/20101106006
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