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Physics & Astronomy
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Discovering the Universe
Exam 12: Characterizing Stars
Path 4
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Question 181
Multiple Choice
If the intrinsically brightest stars in Earth's sky have absolute magnitudes of -10, how bright (in terms of total energy output per second) are these stars compared with the Sun, whose absolute magnitude is +4.8?
Question 182
Multiple Choice
For MOST stars, the
Question 183
Multiple Choice
What is a star's luminosity?
Question 184
Multiple Choice
The Hipparcos satellite was able to measure parallax for stars out to about 150 pc. This distance includes roughly 2.5 million stars. What is the average number of stars in 1 cubic parsec?
Question 185
Multiple Choice
Suppose the distance between an observer and a lightbulb is doubled. How does its final brightness compare with its initial brightness?
Question 186
Multiple Choice
What will be the intrinsic brightness or luminosity of a white dwarf star that has the same temperature as the Sun? See Figure 12-7 in the text.
Question 187
Multiple Choice
Why are Balmer absorption lines very weak in the spectra of stars with low surface temperatures-significantly below 10,000 K, for example?
Question 188
Multiple Choice
How many eleventh magnitude stars are required to equal the brightness of one first magnitude?
Question 189
Multiple Choice
When comparing two stars, the one with the _____ must have the greater luminosity.
Question 190
Multiple Choice
Absolute magnitude is defined as the apparent magnitude that a star would have if
Question 191
Multiple Choice
A particular star is at a distance of 20 pc from Earth. For this star, the apparent magnitude will have
Question 192
Multiple Choice
How many times brighter than a magnitude +4.0 star is a magnitude +3.0 star?
Question 193
Multiple Choice
What condition is necessary on Earth to see eclipses of stars in binary star systems?
Question 194
Multiple Choice
The absolute magnitude of a star is the brightness the star would appear to have if it were placed at what distance from Earth?
Question 195
Multiple Choice
Astronomers originally classified the spectra of stars according to the strengths of their hydrogen lines. What new physical insight enabled a reinterpretation of these patterns in terms of surface temperature during the 1920s?