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A star's apparent magnitude is a measure of


A) how bright it appears to us if it is at its actual distance.
B) how bright it appears to us at a standard distance of 10 pc.
C) its energy output per second compared to the Sun.
D) its mass in solar masses.
E) its surface temperature in Kelvin.

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Some giants and/or supergiants are less dense than air.

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The diagram below illustrates two stars in a visual binary system and the center of mass of this system. Based on this diagram, what is the ratio of the mass of star A to the mass of star B The diagram below illustrates two stars in a visual binary system and the center of mass of this system. Based on this diagram, what is the ratio of the mass of star A to the mass of star B   A) 2 to 1 B) 1 to 2 C) 2 to 3 D) 3 to 2 E) 1 to 3


A) 2 to 1
B) 1 to 2
C) 2 to 3
D) 3 to 2
E) 1 to 3

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Proxima Centauri has an absolute visual magnitude of 15.5 and an apparent visual magnitude of 11.0. What is the distance to Proxima Centauri in units of pc


A) 0.1
B) 100.1
C) 10-0.1
D) None of the other choices are correct.

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How do the spectra of giants, supergiants, and main-sequence stars differ

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Supergiants have very narrow s...

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  Which statement is incorrect about the above spectra  A) Hα line strength increases with decreasing stellar surface temperature from 05 to about F0 and decreases in line strength with decreasing stellar surface temperature from about F0 to M0. B) Hβ line strength increases with decreasing stellar surface temperature from 05 to about A1 and decreases in line strength with decreasing stellar surface temperature from about A1 to K0. C) Hγ line strength increases with decreasing stellar surface temperature from 05 to about K0 and decreases in line strength with decreasing stellar surface temperature from about K0 to M5. D) Hδ line strength increases with decreasing stellar surface temperature from 05 to about A1 and decreases in line strength with decreasing stellar surface temperature from about A1 to K0. Which statement is incorrect about the above spectra


A) Hα line strength increases with decreasing stellar surface temperature from 05 to about F0 and decreases in line strength with decreasing stellar surface temperature from about F0 to M0.
B) Hβ line strength increases with decreasing stellar surface temperature from 05 to about A1 and decreases in line strength with decreasing stellar surface temperature from about A1 to K0.
C) Hγ line strength increases with decreasing stellar surface temperature from 05 to about K0 and decreases in line strength with decreasing stellar surface temperature from about K0 to M5.
D) Hδ line strength increases with decreasing stellar surface temperature from 05 to about A1 and decreases in line strength with decreasing stellar surface temperature from about A1 to K0.

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Why don't we see hydrogen Balmer lines in the spectra of stars with temperatures of 3,200 K


A) There is no hydrogen in stars this cool.
B) The stars are hot enough that most of the hydrogen is ionized and the atoms cannot absorb energy.
C) These stars are so cool that nearly all of the hydrogen atoms are in the ground state.
D) Stars of this temperature are too cool to produce an absorption spectrum.
E) Stars of this temperature are too hot to produce an absorption spectrum.

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If a star is located at 10 pc, which of the following statements is correct


A) The star's apparent and absolute visual magnitudes are equal.
B) The star's apparent and absolute visual magnitudes are 0.
C) The star's apparent visual magnitude is -1.1 whereas the absolute visual magnitude is -5.
D) Two of the other choices are correct.

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How do absolute visual magnitude and luminosity differ

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Absolute visual magnitude of a star is t...

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We know the white dwarf star Sirius B has a mass comparable to the Sun because


A) of its measured color.
B) of its measured temperature compared to Sirius A.
C) it is part of binary star system with Sirius A.

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The best sample of the true numbers of the different types of stars consists of


A) stars that appear brightest in the sky to an observer on Earth.
B) all of the stars within our solar system.
C) all the stars within a given distance from Earth.

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What is the correct order of densities from least to most


A) supergiant, main sequence, white dwarf
B) main sequence, white dwarf, supergiant
C) white dwarf, main sequence, giant
D) main sequence, giant, supergiant

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We know that the numbers of stars _________ from _______ to ________ on the H-R diagram.


A) increases, upper right, lower left
B) decreases, upper left, lower right
C) increases, upper left, lower right
D) decreases, upper right, lower left

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Absolute visual magnitude is


A) the apparent magnitude of a star observed from Earth.
B) the luminosity of a star observed from a distance of 1000 pc.
C) the apparent magnitude of a star observed from a distance of 10 pc.
D) the luminosity of a star observed from Earth.
E) the apparent magnitude of a star observed from a distance of 10 pc and the luminosity of a star observed from Earth.

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A star's luminosity depends only on the star's


A) distance and diameter.
B) temperature and distance.
C) distance.
D) temperature and diameter.
E) apparent magnitude.

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Main-sequence stars have about the same density as the Sun but giant stars have very low densities.

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The method of spectroscopic parallax cannot be applied to stars beyond about 100 pc.

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Parallax would be easier to measure if


A) Earth's orbit was larger.
B) the stars were farther away.
C) Earth moved faster along its orbit.
D) Earth's orbit was larger, the stars were further away, and Earth moved faster along its orbit.
E) None of the other choices are correct.

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Arcturus has an mV = -0.04 and MV = -0.3. Its distance is 10-3.4 pc.

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For what kinds of stars are the masses of stars in the H-R diagram "orderly" For what kinds of stars are they disorderly In other words, could you guess the mass of a star from its location (luminosity, temperature) on the H-R diagram

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The masses of main-sequence st...

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