What is spectroscopic parallax?
A) apparent change in position of the absorption lines in a star's spectrum due to the Doppler shift caused by Earth's motion around the Sun
B) apparent change in position of a nearby star compared with distant background stars due to the motion of Earth around the Sun
C) change in position of the absorption lines in a star's spectrum due to the Doppler shift caused by the star's motion around the center of mass in a binary star system
D) distance to a star measured using the spectral luminosity class of the star and the inverse-square law
Correct Answer:
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Q204: Two stars in a binary system orbit
Q205: Which of these statements about measuring the
Q206: What is the only way to measure
Q207: See Figure 12-10 in the text.
Q208: The spectral luminosity class of the
Q210: Which of these is not a type
Q211: Two stars, one classified A4 V and
Q212: Which important stellar parameter can be derived
Q213: How do astronomers measure the masses of
Q214: Which of these spectral luminosity classes corresponds
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