In this book, renowned scientists describe the various techniques used to detect and characterize extrasolar planets, or exoplanets, with a view to unveiling the “tricks of the trade” of planet detection to a wider community. The radial velocity method, transit method, microlensing method, and direct imaging method are all clearly explained, drawing attention to their advantages and limitations and highlighting the complementary roles that they can play in improving the characterization of exoplanets’ physical and orbital properties. By probing the planetary frequency at different distances and in different conditions, these techniques are helping astrophysicists to reconstruct the scenarios of planetary formation and to give robust scientific answers to questions regarding the frequency of potentially habitable worlds. Twenty years have passed since the discovery of a Jupiter-mass companion to a main sequence star other than the Sun, heralding the birth of extrasolar planetary research; this book fully conveys the exciting progress that has been achieved during the intervening period.
Les informations fournies dans la section « Synopsis » peuvent faire référence à une autre édition de ce titre.
Valerio Bozza is a researcher in the "E.R. Caianiello" Department of Physics at the University of Salerno, Italy. Dr. Bozza gained his doctorate from Salerno University in 2002 for a thesis on "Pre-Big Bang cosmology: initial conditions and brane-worlds" and subsequently undertook research at CERN's TH Unit. His fields of interest include cosmology (string cosmology, bouncing cosmologies, cosmological perturbations, brane worlds, and transplanckian effects), gravitational lensing by black holes, and microlensing (the search for extrasolar planets, binary microlensing modeling, and microlenses surrounded by gas clouds). He is the author of more than 90 scientific publications.
Luigi Mancini works as a Research Staff Scientist in the Planet and Star Formation Department of the Max Planck Institute for Astronomy in Heidelberg, Germany. As a member of the HATSouth project team, his research is currently focused primarily on the search for extrasolar planets transiting nearby brightstars in the Southern Hemisphere. Dr. Mancini is also leading a project for accurate measurements of the properties of extrasolar planets via photometric observations and is involved in the GAPS (Characterizing the Global Architectures of Planetary Systems) project. He holds the Italian National Academic Qualification as an Associate Professor and is the author of approaching 100 papers in peer-reviewed journals.Les informations fournies dans la section « A propos du livre » peuvent faire référence à une autre édition de ce titre.
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Taschenbuch. Etat : Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -In this book, renowned scientists describe the various techniques used to detect and characterize extrasolar planets, or exoplanets, with a view to unveiling the 'tricks of the trade' of planet detection to a wider community. The radial velocity method, transit method, microlensing method, and direct imaging method are all clearly explained, drawing attention to their advantages and limitations and highlighting the complementary roles that they can play in improving the characterization of exoplanets' physical and orbital properties. By probing the planetary frequency at different distances and in different conditions, these techniques are helping astrophysicists to reconstruct the scenarios of planetary formation and to give robust scientific answers to questions regarding the frequency of potentially habitable worlds. Twenty years have passed since the discovery of a Jupiter-mass companion to a main sequence star other than the Sun, heralding the birth of extrasolar planetary research; this book fully conveys the exciting progress that has been achieved during the intervening period. 268 pp. Englisch. N° de réf. du vendeur 9783319801469
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Taschenbuch. Etat : Neu. Methods of Detecting Exoplanets | 1st Advanced School on Exoplanetary Science | Valerio Bozza (u. a.) | Taschenbuch | xv | Englisch | 2018 | Springer | EAN 9783319801469 | Verantwortliche Person für die EU: Springer Verlag GmbH, Tiergartenstr. 17, 69121 Heidelberg, juergen[dot]hartmann[at]springer[dot]com | Anbieter: preigu. N° de réf. du vendeur 114236210
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Taschenbuch. Etat : Neu. This item is printed on demand - Print on Demand Titel. Neuware -In this book, renowned scientists describe the various techniques used to detect and characterize extrasolar planets, or exoplanets, with a view to unveiling the ¿tricks of the trade¿ of planet detection to a wider community. The radial velocity method, transit method, microlensing method, and direct imaging method are all clearly explained, drawing attention to their advantages and limitations and highlighting the complementary roles that they can play in improving the characterization of exoplanets¿ physical and orbital properties. By probing the planetary frequency at different distances and in different conditions, these techniques are helping astrophysicists to reconstruct the scenarios of planetary formation and to give robust scientific answers to questions regarding the frequency of potentially habitable worlds. Twenty years have passed since the discovery of a Jupiter-mass companion to a main sequence star other than the Sun, heralding the birth of extrasolar planetary research; this book fully conveys the exciting progress that has been achieved during the intervening period.Springer-Verlag KG, Sachsenplatz 4-6, 1201 Wien 268 pp. Englisch. N° de réf. du vendeur 9783319801469
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Taschenbuch. Etat : Neu. Druck auf Anfrage Neuware - Printed after ordering - In this book, renowned scientists describe the various techniques used to detect and characterize extrasolar planets, or exoplanets, with a view to unveiling the 'tricks of the trade' of planet detection to a wider community. The radial velocity method, transit method, microlensing method, and direct imaging method are all clearly explained, drawing attention to their advantages and limitations and highlighting the complementary roles that they can play in improving the characterization of exoplanets' physical and orbital properties. By probing the planetary frequency at different distances and in different conditions, these techniques are helping astrophysicists to reconstruct the scenarios of planetary formation and to give robust scientific answers to questions regarding the frequency of potentially habitable worlds. Twenty years have passed since the discovery of a Jupiter-mass companion to a main sequence star other than the Sun, heralding the birth of extrasolar planetary research; this book fully conveys the exciting progress that has been achieved during the intervening period. N° de réf. du vendeur 9783319801469
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