NMC Library
Image from Google Jackets

How do you find an exoplanet? / John Asher Johnson

By: Series: Princeton frontiers in physicsPublisher: Princeton, New Jersey : Princeton University Press, [2016]Description: xv, 178 pages : illustrations ; 21 cmContent type:
  • text
Media type:
  • unmediated
Carrier type:
  • volume
ISBN:
  • 9780691156811 (hbk)
  • 0691156816 (hbk)
Subject(s): LOC classification:
  • QB820 .J64 2016
Contents:
Introduction. My brief history -- The human activity of watching the sky -- Asking why the planets move as they do -- Exoplanets and completing the Copernican revolution -- Stellar wobbles. At the telescope -- For every action -- Eccentric orbits -- Measuring precise radial velocities -- Stellar jitter -- Design considerations for a Doppler survey -- Concluding remarks -- Seeing the shadows of planets. Measuring and reading transit signals -- The importance of a/R* -- Transit timing variations -- Measuring the brightness of a star -- Radial velocities first, transits second -- Transit first, radial velocities second -- From close in to further out -- Planets bending space-time. The geometry of microlensing -- The microlensing light curve -- The microlensing signal of a planet -- Microlensing surveys -- Directly imaging planets. The problem of angular resolution -- The problem of contrast -- The problem of chance alignment -- Measuring the properties of an imaged planet -- The future of planet hunting. Placing the solar system in context -- Learning how planets form -- Finding life outside the solar system -- Giant planets as the tip of the iceberg -- The future of the Doppler method : moving to dedicated instrumentation -- The future of transit surveys -- The future of microlensing -- The future of direct imaging -- Concluding remarks
Summary: An authoritative primer on the four key techniques that today's planet hunters use to detect the feeble signals of planets orbiting distant stars.-- Source other than the Library of Congress
Holdings
Item type Current library Shelving location Call number Copy number Status Date due Barcode
Book Book NMC Library Stacks QB820 .J64 2016 (Browse shelf(Opens below)) 1 Available 33039001402253

Includes bibliographical references (pages 163-169) and index

Introduction. My brief history -- The human activity of watching the sky -- Asking why the planets move as they do -- Exoplanets and completing the Copernican revolution -- Stellar wobbles. At the telescope -- For every action -- Eccentric orbits -- Measuring precise radial velocities -- Stellar jitter -- Design considerations for a Doppler survey -- Concluding remarks -- Seeing the shadows of planets. Measuring and reading transit signals -- The importance of a/R* -- Transit timing variations -- Measuring the brightness of a star -- Radial velocities first, transits second -- Transit first, radial velocities second -- From close in to further out -- Planets bending space-time. The geometry of microlensing -- The microlensing light curve -- The microlensing signal of a planet -- Microlensing surveys -- Directly imaging planets. The problem of angular resolution -- The problem of contrast -- The problem of chance alignment -- Measuring the properties of an imaged planet -- The future of planet hunting. Placing the solar system in context -- Learning how planets form -- Finding life outside the solar system -- Giant planets as the tip of the iceberg -- The future of the Doppler method : moving to dedicated instrumentation -- The future of transit surveys -- The future of microlensing -- The future of direct imaging -- Concluding remarks

An authoritative primer on the four key techniques that today's planet hunters use to detect the feeble signals of planets orbiting distant stars.-- Source other than the Library of Congress

There are no comments on this title.

to post a comment.

Powered by Koha