A) the supergiant region
B) the main sequence
C) the white dwarf region
D) the visual region
E) the twilight zone
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Multiple Choice
A) its apparent brightness
B) its temperature
C) its chemical composition
D) its mass
E) you can't fool me, all of these are quite easy to measure directly
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Multiple Choice
A) double stars
B) main sequence stars
C) brown dwarf pairs
D) first contact stars
E) binary stars
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Multiple Choice
A) it must be a main sequence star
B) it must be quite small in size
C) it must be quite large in size
D) it must be brown dwarf and not a regular star
E) this must be an error in observations; no such star can exist
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Multiple Choice
A) among the white dwarfs
B) among the stars at the top left of the main sequence
C) among the stars at the bottom right of the main sequence
D) among the supergiants
E) stars with low mass can be located anywhere at all in the H-R diagram
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Multiple Choice
A) along the right (vertical axis)
B) along the bottom (the horizontal axis)
C) only in the red giant region
D) only on the main sequence
E) H-R diagrams have nothing to say about spectral types
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Multiple Choice
A) stars are so bright, their light burns out all the delicate instruments we would use to measure their diameters
B) all stars change their diameters regularly, growing alternately larger and smaller
C) stars are so far away, we cannot resolve (distinguish) their diameters
D) stars are all in binary systems, and we can only see the combined diameter of both stars
E) you can't fool me; measuring the diameter of any star is a relatively easy process
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Multiple Choice
A) that the lines in its spectrum get brighter
B) that the lines in its spectrum merge with the lines of the other star
C) that it is no longer possible to learn what elements are in the star
D) that the lines in its spectrum show a blue-shift
E) none of the above
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Multiple Choice
A) watching the body of the Moon go across the star
B) getting the light curve of an eclipsing binary star
C) comparing the color of a star seen high above our heads and then again when it's near the horizon
D) measuring the spectrum of a spectroscopic binary
E) more than one of the above
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Multiple Choice
A) only near the top of the diagram and never near the bottom
B) only near the left side of the diagram and never near the right
C) only on the right side of the diagram and never on the left
D) only near the bottom of the diagram and never near the top
E) anywhere in the diagram
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Multiple Choice
A) mass
B) diameter
C) surface temperature
D) age
E) location in the sky
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Multiple Choice
A) a brown dwarf
B) a planet
C) the Sun
D) the smallest mass star that can still have fusion of hydrogen to helium in its core
E) you can't fool me, all the above have roughly the same mass
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Multiple Choice
A) larger in diameter
B) smaller in diameter
C) the same size in diameter
D) younger in age
E) less massive
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Multiple Choice
A) Galileo saw through his early telescope that the Milky Way consisted of many stars
B) Herschel measured the two stars that make up the Castor system moved around each other
C) Cannon measured different lines in the spectra of different types of stars
D) Comet Halley returned after a 76-year absence
E) You can't fool me, we still don't know whether gravity around other stars works the same way as it does here
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Multiple Choice
A) Hubble
B) Humason
C) Hertzsprung
D) Huggins
E) Hoyle
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Multiple Choice
A) intrinsically fainter than the Sun
B) very close to us (among the closest stars)
C) more luminous (intrinsically brighter) than the Sun
D) only visible to our eyes because they actually consist of three or more stars blending their light together
E) undergoing some sort of explosion which makes their outer layers unusually bright
Correct Answer
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Multiple Choice
A) visual double stars
B) white dwarf stars
C) main sequence stars
D) eclipsing binary stars
E) any star that is not a brown dwarf
Section 18.4: The H-R Diagram
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Multiple Choice
A) because conditions in the "neighborhood" of the Sun only permit low-mass (low luminosity) stars to form
B) because such very luminous stars are extremely rare, and thus any small neighborhood in the Galaxy is unlikely to contain one of them
C) because all stars in the vicinity of the Sun have planets, and planets rob a star of its brightness
D) because such superstars only give off a lot of energy for a year or so, before they die
E) because such superstars are really several hundred stars blending their light together (but so far away we can't distinguish individual stars) ; nearby stars are easy to separate
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Multiple Choice
A) low luminosity compared to the Sun
B) spectra that show they contain mostly carbon
C) enormous masses compared to the Sun
D) diameters thousands of times greater than the Sun's
E) a dozen or more stars in close orbit around them
Section 18.2: Measuring Stellar Masses
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Multiple Choice
A) among the supergiants, in the upper right
B) a little bit below the Sun on the main sequence
C) among the most brilliant of the white dwarfs, in the lower left
D) near the very top of the main sequence, in the upper left
E) it could be anywhere on the diagram; we would need more information to determine its place
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