Exam 13: Measuring the Properties of Stars

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The luminosity class of a star can be determined from the width of the spectral lines of the star.

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True

Analysis of ___ stars has shown that star masses are in the range of ___ to ____ solar masses.

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What is parallax?

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C

A star radiates most strongly at 600 nanometers. What is its surface temperature?

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In the above H-R diagram sketch, which star is a red giant?

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If Star A is twice as far as Star B, and they are identical in all other ways, then the brightness of Star A would be

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Lines from molecules are strongest in ___ type stars.

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What distinguishes the spectral type of a star?

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A star of apparent magnitude ____ appears 2.51 times brighter than a star of apparent magnitude 4.

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How can we explain the fact that hydrogen Balmer lines are essentially absent in the hot O type and the cool M stars?

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The star Aldebaran is a red giant, and is much more luminous than the Sun. What conclusions can be drawn from this fact?

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Star A is located at the top left of the H-R diagram and has the same luminosity as Star B which is located at the top right of the H-R diagram. How must these stars differ?

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Nearby stars have larger parallax angles, therefore their distance in parsecs is smaller.

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Parallax measurements of the distances to the nearest stars use _____ as a baseline.

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A star radiates most strongly at 400 nm. What is its surface temperature?

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Measuring stellar masses using binary stars is difficult because binary stars are rare.

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A star's parallax can reveal its distance. Stars with larger parallaxes are _______.

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Star A and Star B have same temperatures, but Star A is more luminous than Star B. Based on this information, which of the following must be the case?

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An M type star 1,000 times more luminous than the Sun will be located near the ___ part of the H-R diagram.

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A 10th magnitude star is ____________ than a 5th magnitude star.

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