Exam 8: The Family of Stars

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

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The absorption lines in the infrared portion of the spectrum of a star that are produced by hydrogen are from the

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Binary (double) stars can be detected by

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E

Of the three units of astronomical distances, _________ is shorter than _________, which is shorter than _________.

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The amount of light received at Earth from a star is called luminosity.

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What is the total mass of a binary star system with P = 20 yr and a = 10 AU?

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Groombridge 34 is an M1 V star. Based on this information, which of the following are true? I. Groombridge 34 has a surface temperature that is less than the Sun. II. Groombridge 34 has a mass that is greater than that of the Sun. III. Groombridge 34 is less luminous than the Sun. IV. Groombridge 34 is located near the middle of the H-R diagram.

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Consider a two-body system of the Earth orbiting the Sun. The center of mass would be located near the _________.

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  Based upon the information given in the above color photographs, what would you predict to see in a spectra class L0 color photo? Based upon the information given in the above color photographs, what would you predict to see in a spectra class L0 color photo?

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Why would parallaxes be easier to observe if Earth were farther from the Sun?

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Polaris is 10 times larger than Capella A and both are the same color. How much brighter or dimmer is Polaris to Capella?

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To observe a spectroscopic binary, we must be able to see both stars individually.

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If the orbital velocity of an eclipsing binary is 97 km/s and the smaller star is completely eclipsed in 2 hours, what is the diameter of the smaller star?

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You want to find a mass of a star on the main sequence of the H-R diagram. What do you need?

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  The concept the picture above is trying to get across is _______. The concept the picture above is trying to get across is _______.

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Describe the measurements needed to determine the orbit of a visual binary star.

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If a star's spectrum does not contain spectral lines characteristic of a certain element, can we conclude that the star does not contain that element? Why or why not?

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Why are the Balmer lines weak in the spectra of hot and cool stars, but strong in the spectra of intermediate-temperature stars?

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The most common stars are

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

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