Introduction to stars and planets [electronic resource] : an activities-based exploration / Alan Hirshfeld.

How do astronomers know what they know about the stars and planets? That is the question behind today's rapid pace of cosmic discovery, for every new finding rests upon a centuries-long foundation of astronomical practice. Introduction to Stars and Planets: An activities-based exploration reveals th...

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Bibliographic Details
Uniform Title:AAS-IOP astronomy. 2021 collection.
Main Author: Hirshfeld, Alan (Author)
Corporate Author: Institute of Physics (Great Britain) (Publisher)
Language:English
Published: Bristol [England] (Temple Circus, Temple Way, Bristol BS1 6HG, UK) : IOP Publishing, [2020]
Series:AAS-IOP astronomy. 2021 collection.
Subjects:
Online Access:
Variant Title:
Introduction to Stars and Planets: An activities-based exploration
Format: Electronic eBook

MARC

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245 1 0 |a Introduction to stars and planets  |h [electronic resource] :  |b an activities-based exploration /  |c Alan Hirshfeld. 
246 2 |a Introduction to Stars and Planets: An activities-based exploration 
264 1 |a Bristol [England] (Temple Circus, Temple Way, Bristol BS1 6HG, UK) :  |b IOP Publishing,  |c [2020] 
490 1 |a AAS-IOP astronomy. [2021 collection],  |x 2514-3433 
500 |a "Version: 20201201"--Title page verso. 
504 |a Includes bibliographical references. 
505 8 |a 26. The search for exoplanets : Doppler method -- 26.1. The Doppler effect -- 26.2. Center of mass -- 26.3. Detecting the solar system from afar -- 26.4. Weighing an exoplanet 
505 8 |a 27. The search for exoplanets : transit method (I) -- 27.1. Introduction -- 27.2. Planetary transit basics -- 27.3. Detecting the solar system from afar (redux) 
505 8 |a 28. The search for exoplanets : transit method (II) -- 28.1. Case study : the transit of a real exoplanet -- 28.2. Radius of Kepler 21b -- 28.3. Orbital radius of Kepler 21b -- 28.4. Mass and average density of Kepler 21b -- 28.5. Surface temperature of Kepler 21b. 
505 0 |a part I. The sun. 1. The Sun's distance I : the method of Aristarchus -- 1.1. Aristarchus's distance to the Sun -- 1.2. The Sun's diameter -- 1.3. The Sun's distance revisited 
505 8 |a 2. The Sun's distance II : transits and radar-ranging of Venus -- 2.1. Transits of Venus -- 2.2. The relative sizes of Earth's and Venus's orbits -- 2.3. The absolute distance from the Earth to Venus -- 2.4. Radar-ranging of Venus 
505 8 |a 3. The Sun's diameter and mass -- 3.1. The Sun's diameter -- 3.2. The Sun's mass -- 3.3. Implications 
505 8 |a 4. The sunspot cycle -- 4.1. Tracking sunspots through history 
505 8 |a 5. The solar constant -- 5.1. Basic concepts -- 5.2. Measuring the solar constant -- 5.3. The solar constant in practice 
505 8 |a 6. The Sun's luminosity -- 6.1. Introduction -- 6.2. Squares and spheres 
505 8 |a 7. The Sun's surface temperature -- 7.1. Taking the Sun's temperature -- 7.2. A pint-sized star 
505 8 |a 8. Spectral lines and the chemistry of the Sun -- 8.1. Dark lines and bright lines -- 8.2. The Sun's spectrum -- 8.3. Establishing the spectrum's wavelength scale -- 8.4. Computing the wavelengths of the dark lines -- 8.5. Identifying the Fraunhofer lines 
505 8 |a 9. Is the Sun on fire? -- 9.1. The energy enigma -- 9.2. Chemical combustion -- 9.3. Conclusion 
505 8 |a 10. How long will the Sun shine? -- 10.1. Thermonuclear fusion -- 10.2. Input data -- 10.3. Mass into energy -- 10.4. How long can fusion last? -- 10.5. The life span of the sun 
505 8 |a part II. The stars. 11. The distances of stars : stellar parallax -- 11.1. Stellar parallax -- 11.2. Parallax simulation -- 11.3. Bessel's star -- 11.4. The 3D cosmos 
505 8 |a 12. Weighing a star : binary stars and stellar mass -- 12.1. Binary stars -- 12.2. Orbital period -- 12.3. Orbital radius and combined mass of Sirius and Sirius B -- 12.4. Masses of the individual stars 
505 8 |a 13. The Hertzsprung-Russell diagram -- 13.1. Introduction -- 13.2. Stellar magnitudes and spectral types -- 13.3. Plotting and reading the HR diagram -- 13.4. Selection effects -- 13.5. Theory meets the HR diagram 
505 8 |a 14. The distance to a star cluster -- 14.1. The color-magnitude diagram -- 14.2. Main-sequence fitting -- 14.3. Caveat : interstellar dust 
505 8 |a 15. The evolution of the Sun -- 15.1. Programming the Sun -- 15.2. The life and death of our star 
505 8 |a 16. The evolution of massive stars -- 16.1. Cosmic beacons -- 16.2. Heavyweights 
505 8 |a 17. Supernovae : the expansion of the Crab Nebula -- 17.1. The Crab Nebula, then and now -- 17.2. Image scale -- 17.3. Measurement of the nebula -- 17.4. Expansion and age of the Crab Nebula -- 17.5. Distance of the Crab Nebula 
505 8 |a 18. The event horizon of black holes -- 18.1. Black hole basics -- 18.2. Escape velocity -- 18.3. John Michell's "dark star" -- 18.4. The event horizon 
505 8 |a 19. Kepler's Third law and the masses of black holes -- 19.1. Introduction -- 19.2. Inside the solar system -- 19.3. Beyond the solar system -- 19.4. Beyond the galaxy 
505 8 |a 20. Our place in the galaxy -- 20.1. Our view of the galaxy -- 20.2. Globular star clusters -- 20.3. Galactic coordinate system 
505 8 |a part III. The planets. 21. A slice of earth -- 21.1. The Earth in perspective 
505 8 |a 22. Geological time in perspective -- 22.1. Cosmic calendar 
505 8 |a 23. The comparative density of planets -- 23.1. Average density -- 23.2. Terrestrial versus Jovian planets 
505 8 |a 24. Planetary surface temperatures -- 24.1. Introduction -- 24.2. Earth's surface temperature -- 24.3. The surface temperature of other planets -- 24.4. The surface temperature of a comet 
505 8 |a 25. The habitable zone -- 25.1. Introduction -- 25.2. Replacing the Sun -- 25.3. Relocating the Earth 
520 3 |a How do astronomers know what they know about the stars and planets? That is the question behind today's rapid pace of cosmic discovery, for every new finding rests upon a centuries-long foundation of astronomical practice. Introduction to Stars and Planets: An activities-based exploration reveals the methods by which Earthbound observers have deduced the physical attributes of celestial bodies, whether situated within our solar neighborhood or at the far ends of the Galaxy. The book's 28 mildly mathematical activities invite readers to carry out the essential work of the astronomer by utilizing real observational data sets and high-quality celestial photographs to establish the innate properties of a range of cosmic systems. Taken in sequence, these activities illustrate the epic advancement of stellar and planetary astronomy over the past century, up to the present day. 
521 |a College-level introductory courses in astronomy, both classroom and online. Also first-year course in an astronomy/astrophysics major curriculum. 
538 |a Mode of access: World Wide Web. 
538 |a System requirements: Adobe Acrobat Reader, EPUB reader, or Kindle reader. 
545 |a Alan Hirshfeld, Professor of physics at the University of Massachusetts Dartmouth, is Chair of the American Astronomical Society's Historical Astronomy Division and a longtime Associate of the Harvard College Observatory. He is the author of Parallax: The Race to Measure the Cosmos; The Electric Life of Michael Faraday; Eureka Man: The Life and Legacy of Archimedes; Astronomy Activity & Laboratory Manual; and Starlight Detectives: How Astronomers, Inventors, and Eccentrics Discovered the Modern Universe. He is a regular book reviewer for The Wall Street Journal and writes and lectures frequently on science history and discovery. Visit the author's website at www.alanhirshfeld.com. 
650 0 |a Planets. 
650 0 |a Stars. 
710 2 |a Institute of Physics (Great Britain),  |e publisher. 
773 0 |t IOP eBooks AAS-IOP Astronomy 2021 Collection   |d IOP Publishing Limited 
776 0 8 |i Print version:  |z 9780750336895  |z 9780750336925 
830 0 |a AAS-IOP astronomy.  |p 2021 collection. 
856 4 0 |y Access Content Online(from IOP eBooks AAS-IOP Astronomy 2021 Collection)  |u https://ezproxy.msu.edu/login?url=https://iopscience.iop.org/book/mono/978-0-7503-3691-8  |z IOP eBooks AAS-IOP Astronomy 2021 Collection: 2020