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Methods of detecting exoplanets = 1s...
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SpringerLink (Online service)
Methods of detecting exoplanets = 1st Advanced School on Exoplanetary Science /
Record Type:
Language materials, printed : Monograph/item
Title/Author:
Methods of detecting exoplanets/ edited by Valerio Bozza, Luigi Mancini, Alessandro Sozzetti.
Reminder of title:
1st Advanced School on Exoplanetary Science /
other author:
Bozza, Valerio.
corporate name:
Workshop on the Preservation of Stability under Discretization
Published:
Cham :Springer International Publishing : : 2016.,
Description:
xv, 252 p. :ill. (some col.), digital ; : 24 cm.;
Contained By:
Springer eBooks
Subject:
Extrasolar planets - Congresses. - Detection -
Online resource:
http://dx.doi.org/10.1007/978-3-319-27458-4
ISBN:
9783319274584
Methods of detecting exoplanets = 1st Advanced School on Exoplanetary Science /
Methods of detecting exoplanets
1st Advanced School on Exoplanetary Science /[electronic resource] :edited by Valerio Bozza, Luigi Mancini, Alessandro Sozzetti. - Cham :Springer International Publishing :2016. - xv, 252 p. :ill. (some col.), digital ;24 cm. - Astrophysics and space science library,4280067-0057 ;. - Astrophysics and space science library ;v.351..
1st Advanced School on Exoplanetary Science: Methods of detecting Exoplantes -- The Radial Velocity Method -- The Transit method -- The Microlensing method -- Direct imaging of Exoplanets.
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.
ISBN: 9783319274584
Standard No.: 10.1007/978-3-319-27458-4doiSubjects--Topical Terms:
1108354
Extrasolar planets
--Detection--Congresses.
LC Class. No.: QB820
Dewey Class. No.: 523.24
Methods of detecting exoplanets = 1st Advanced School on Exoplanetary Science /
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1st Advanced School on Exoplanetary Science: Methods of detecting Exoplantes -- The Radial Velocity Method -- The Transit method -- The Microlensing method -- Direct imaging of Exoplanets.
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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.
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Physics and Astronomy (Springer-11651)
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