Exam 4: Atomic Physics and Spectra
Exam 1: Discovering the Night Sky374 Questions
Exam 2: Gravitation and the Motion of the Planets356 Questions
Exam 3: Light and Telescopes275 Questions
Exam 4: Atomic Physics and Spectra223 Questions
Exam 5: Exoplanets and the Formation of Planetary Systems98 Questions
Exam 6: Formation of the Solar System121 Questions
Exam 7: Earth and the Moon305 Questions
Exam 8: The Other Terrestrial Planets265 Questions
Exam 9: The Outer Planets360 Questions
Exam 10: Vagabonds of the Solar System198 Questions
Exam 11: The Sun: Our Extraordinary Star248 Questions
Exam 12: Characterizing Stars254 Questions
Exam 13: The Lives of Stars From Birth Through Middle Age325 Questions
Exam 14: The Death of Stars235 Questions
Exam 15: Black Holes: Matters of Gravity178 Questions
Exam 16: The Milky Way Galaxy157 Questions
Exam 17: Galaxies207 Questions
Exam 18: Quasars and Other Active Galaxies118 Questions
Exam 19: Cosmology217 Questions
Exam 20: Astrobiology71 Questions
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What overall effect on the visible spectrum of the light from a star results from the light's passage through Earth's atmosphere?
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What is the approximate peak wavelength of radiation emitted by (live) human beings, who are (normally) at a temperature of about 310 K?
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Atoms in a thin, hot gas (such as a neon advertising sign), according to Kirchhoff's laws, emit light at
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A typical but very cool star might have a temperature of 3100°C. On the Kelvin scale, this is about
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A spectrum produced by heating a gaseous sample of a single element consists of a series of bright lines. If a solid composed of this element is heated, the result will be that
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The gas in the interstellar space between stars is very tenuous (thin) but can be heated to a very high temperature in the vicinity of a hot star. This hot, tenuous gas will emit
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The star P Cygni (in the constellation Cygnus, the Swan) is surrounded by an extensive low-density atmosphere. It has a bright, continuous spectrum with many narrow, dark absorption lines and a few bright emission lines. The bright emission lines are produced by
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The specific colors of light emitted by an atom in a hot, thin gas (e.g., in a neon tube, a fluorescent bulb, or a gas cloud in space) are caused by
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The isotope 15N has an atomic number of 7. The nucleus of this isotope contains
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The radial velocity of a star or other object is measured by
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According to Kirchhoff's laws, the continuous spectrum of light from a hot star, after passing through a cool gas cloud,
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The star Vega has a higher surface temperature than the Sun. With IR indicating infrared and UV indicating ultraviolet, Vega emits _____ IR and _____ UV flux than the Sun.
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What changes should an observer expect to see in the resulting spectrum of emitted light from a piece of metal when it is heated slowly in an intense flame from 500 K to 1500 K?
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An astronomer, examining two photographs of a small area of sky taken 20 years apart, notices that some of the stars have moved slightly across the sky, relative to most of the other stars in the photographs. This displacement of the stars across the sky is an example of
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When an object is moving toward an observer, the visible light it emits is Doppler-shifted toward the
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An astronomer finds a source of light in space that emits light only in specific, narrow emission lines. Kirchhoff's laws lead him to which conclusion?
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