The Cosmic Perspective (9th Edition)
The Cosmic Perspective (9th Edition)
9th Edition
ISBN: 9780134874364
Author: Jeffrey O. Bennett, Megan O. Donahue, Nicholas Schneider, Mark Voit
Publisher: PEARSON
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Chapter 5, Problem 47EAP

(a)

To determine

To Explain: Studying an object’s spectrum can allow to determine its surface chemical composition.

(b)

To determine

To Explain: Studying an object’s spectrum can allow to determine its surface temperature.

(c)

To determine

To Explain: Studying an object’s spectrum can allow to determine whether it is low density cloud or something more substantial.

(d)

To determine

To Explain: Studying an object’s spectrum can allow to determine whether object has hot upper atmosphere.

(e)

To determine

To Explain: Studying an object’s spectrum can allow to determine whether object is reflecting blue light from a star.

(f)

To determine

To Explain: Studying an object’s spectrum can allow to determine whether object is moving away or towards earth.

(g)

To determine

To Explain: Studying an object’s spectrum can allow to determine object’srotation rate.

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The spectrum of a typical star shows absorption lines at different wavelengths than their laboratory values. If the observed wavelength is greater than its laboratory value of 656.3 nm, one can conclude that... A. The separation between Earth and the star is decreasing. B. The separation between Earth and the star is increasing. C. The separation between Earth and the star is unchanging D. No conclusion is possible.
What is the ratio of the light-gathering power of a 10-meter telescope to that of a 1‑meter telescope?   a. 10 to 1   b. 1 to 10   c. 100 to 1   d. 1 to 100   e. 3.2 to 1
Q / which type of spectral line broadening is less important compared to other type

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The Cosmic Perspective (9th Edition)

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