How do you find an exoplanet?:
An authoritative primer on the four key techniques that today's planet hunters use to detect the feeble signals of planets orbiting distant stars
Gespeichert in:
| 1. Verfasser: | |
|---|---|
| Format: | Buch |
| Sprache: | English |
| Veröffentlicht: |
Princeton ; Oxford
Princeton University Press
[2016]
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| Schlagworte: | |
| Zusammenfassung: | An authoritative primer on the four key techniques that today's planet hunters use to detect the feeble signals of planets orbiting distant stars |
| Beschreibung: | xv, 178 Seiten Illustrationen, Diagramme |
Internformat
MARC
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| 020 | |z 9780691156811 |9 978-0-691-15681-1 | ||
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| 100 | 1 | |a Johnson, John Asher |e Verfasser |0 (DE-588)1113032480 |4 aut | |
| 245 | 1 | 0 | |a How do you find an exoplanet? |c John Asher Johnson |
| 264 | 1 | |a Princeton ; Oxford |b Princeton University Press |c [2016] | |
| 264 | 4 | |c © 2016 | |
| 300 | |a xv, 178 Seiten |b Illustrationen, Diagramme | ||
| 336 | |b txt |2 rdacontent | ||
| 337 | |b n |2 rdamedia | ||
| 338 | |b nc |2 rdacarrier | ||
| 505 | 8 | |a Includes bibliographical references (pages 163-169) and index | |
| 505 | 8 | |a 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 | |
| 520 | |a An authoritative primer on the four key techniques that today's planet hunters use to detect the feeble signals of planets orbiting distant stars | ||
| 650 | 4 | |a Extrasolar planets / Detection | |
| 650 | 4 | |a Extrasolar planets / Research / Methodology | |
| 650 | 0 | 7 | |a Extrasolarer Planet |0 (DE-588)4456110-6 |2 gnd |9 rswk-swf |
| 689 | 0 | 0 | |a Extrasolarer Planet |0 (DE-588)4456110-6 |D s |
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Datensatz im Suchindex
| _version_ | 1804176165518180352 |
|---|---|
| any_adam_object | |
| author | Johnson, John Asher |
| author_GND | (DE-588)1113032480 |
| author_facet | Johnson, John Asher |
| author_role | aut |
| author_sort | Johnson, John Asher |
| author_variant | j a j ja jaj |
| building | Verbundindex |
| bvnumber | BV043519821 |
| classification_rvk | US 7600 |
| contents | 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 |
| ctrlnum | (OCoLC)954339736 (DE-599)BVBBV043519821 |
| discipline | Physik |
| format | Book |
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| id | DE-604.BV043519821 |
| illustrated | Illustrated |
| indexdate | 2024-07-10T07:27:51Z |
| institution | BVB |
| language | English |
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| oclc_num | 954339736 |
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| owner_facet | DE-83 DE-20 |
| physical | xv, 178 Seiten Illustrationen, Diagramme |
| publishDate | 2016 |
| publishDateSearch | 2016 |
| publishDateSort | 2016 |
| publisher | Princeton University Press |
| record_format | marc |
| spelling | Johnson, John Asher Verfasser (DE-588)1113032480 aut How do you find an exoplanet? John Asher Johnson Princeton ; Oxford Princeton University Press [2016] © 2016 xv, 178 Seiten Illustrationen, Diagramme txt rdacontent n rdamedia nc rdacarrier 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 Extrasolar planets / Detection Extrasolar planets / Research / Methodology Extrasolarer Planet (DE-588)4456110-6 gnd rswk-swf Extrasolarer Planet (DE-588)4456110-6 s DE-604 |
| spellingShingle | Johnson, John Asher How do you find an exoplanet? 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 Extrasolar planets / Detection Extrasolar planets / Research / Methodology Extrasolarer Planet (DE-588)4456110-6 gnd |
| subject_GND | (DE-588)4456110-6 |
| title | How do you find an exoplanet? |
| title_auth | How do you find an exoplanet? |
| title_exact_search | How do you find an exoplanet? |
| title_full | How do you find an exoplanet? John Asher Johnson |
| title_fullStr | How do you find an exoplanet? John Asher Johnson |
| title_full_unstemmed | How do you find an exoplanet? John Asher Johnson |
| title_short | How do you find an exoplanet? |
| title_sort | how do you find an exoplanet |
| topic | Extrasolar planets / Detection Extrasolar planets / Research / Methodology Extrasolarer Planet (DE-588)4456110-6 gnd |
| topic_facet | Extrasolar planets / Detection Extrasolar planets / Research / Methodology Extrasolarer Planet |
| work_keys_str_mv | AT johnsonjohnasher howdoyoufindanexoplanet |