Exam 5: Radiation and Spectra
Exam 1: Science and the Universe: a Brief Tour20 Questions
Exam 2: Observing the Sky: the Birth of Astronomy37 Questions
Exam 3: Orbits and Gravity35 Questions
Exam 4: Earth, Moon, and Sky47 Questions
Exam 5: Radiation and Spectra59 Questions
Exam 6: Astronomical Instruments45 Questions
Exam 7: Other Worlds: an Introduction to the Solar System36 Questions
Exam 8: Earth As a Planet36 Questions
Exam 9: Cratered Worlds: the Moon and Mercury34 Questions
Exam 10: Earthlike Planets: Venus and Mars45 Questions
Exam 11: The Giant Planets37 Questions
Exam 12: Rings, Moons, and Pluto41 Questions
Exam 13: Comets and Asteroids: Debris of the Solar System41 Questions
Exam 14: Cosmic Samples and the Origin of the Solar System46 Questions
Exam 15: The Sun: a Garden-Variety Star30 Questions
Exam 16: The Sun: a Nuclear Powerhouse36 Questions
Exam 17: Analyzing Starlight27 Questions
Exam 18: The Stars: a Celestial Census29 Questions
Exam 19: Celestial Distances31 Questions
Exam 20: Between the Stars37 Questions
Exam 21: The Birth of Stars and the Discovery of Planets Outside the Solar System34 Questions
Exam 22: Stars From Adolescence to Old Age35 Questions
Exam 23: The Death of Stars48 Questions
Exam 24: Black Holes and Curved Space-Time33 Questions
Exam 25: The Milky Way Galaxy31 Questions
Exam 26: Galaxies33 Questions
Exam 27: Active Galaxies, Quasars, and Supermassive Black Holes27 Questions
Exam 28: The Evolution and Distribution of Galaxies35 Questions
Exam 29: The Big Bang39 Questions
Exam 30: Life in the Universe36 Questions
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The Balmer Series of lines in the hydrogen atom was very important in the history of physics and astronomy. What made it so important?
(Multiple Choice)
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We observe a glowing cloud of gas in space with a spectroscope. We note that many of the familiar lines of hydrogen that we know on Earth seem to be in a different place. They are shifted toward the blue or violet end of the spectrum compared to their positions in the spectrum of glowing hydrogen gas on Earth. From this we can conclude that:
(Multiple Choice)
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The light which allows you to see this very interesting exam is made up of waves. In these waves, the distance between crests is called the:
(Multiple Choice)
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Two stars have the same diameter and are at the same distance from us (but in different parts of the sky.) Star A has a temperature of 4000 K, while star B has a temperature of 8000K. Which of the following statements is true:
(Multiple Choice)
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Which of the following is not a type of electromagnetic wave with lower energy than visible light waves?
(Multiple Choice)
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You are alone in a large, completely dark auditorium on Earth. What kind of telescope should I use from the other side of the auditorium to detect the electromagnetic radiation emitted by your body?
(Multiple Choice)
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An idealized object that does not reflect or scatter any radiation that hits it, but simply absorbs every bit of radiation that falls on it is called:
(Multiple Choice)
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The idea that atoms radiate energy only when their electrons move from higher to lower energy levels was first advanced by:
(Multiple Choice)
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(In the absence of a strong magnetic field), what is the chief factor that determines what type of electromagnetic radiation objects give off:
(Multiple Choice)
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Of the following, which consists of electro-magnetic waves with the shortest wavelength?
(Multiple Choice)
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What happens as an electron falls from a higher level to a lower level in an atom?
(Multiple Choice)
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Which of the following statements about electromagnetic radiation is FALSE?
(Multiple Choice)
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One reason that human eyes evolved to detect visible light is:
(Multiple Choice)
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Most ultraviolet radiation does not penetrate to the Earth's surface. Instead it is absorbed in:
(Multiple Choice)
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An astronomer discovers a new star and wants to measure its temperature. She would typically do this by:
(Multiple Choice)
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When a star or galaxy is moving away from us, we observe the Doppler effect by seeing the lines in its spectrum
(Multiple Choice)
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