Loose Leaf For Explorations:  Introduction To Astronomy
Loose Leaf For Explorations: Introduction To Astronomy
9th Edition
ISBN: 9781260432145
Author: Thomas T Arny, Stephen E Schneider Professor
Publisher: McGraw-Hill Education
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Chapter 14, Problem 2P
To determine

The amount of cold interstellar cloud in cubic meters required to build the sun, the ratio of volume of cold interstellar cloud to the volume of the sun, and the volume of cold interstellar cloud in cubic light years.

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Models of the first star-forming clouds indicate that they had a temperature of roughly 150 K and a particle density of roughly 400,000 particles per cubic centimeter at the time they started trapping their internal thermal energy. ▼ Part A Estimate the mass at which thermal pressure balances gravity for these values of pressure and temperature. Express your answer in kilograms. —| ΑΣΦ Mcloud Submit Part B = Mcloud How does that mass compare with the Sun's mass? Express your answer in solar masses. Submit Request Answer = ΤΙ ΑΣΦ Request Answer ? ? kg MSun Review
Absorption lines produced by interstellar gas   a. are wider than the lines from stars because the gas is hotter than most stars.   b. are more narrow than the lines from stars because the gas has a lower pressure than stars.   c. indicate that the interstellar medium contains dust.   d. indicate that the interstellar medium is expanding away from the sun.   e. indicate nothing; none of the above statements are true.
Let us imagine that the spectrum of a star is collected and we find the absorption line of Hydrogen-Alpha (the deepest absorption line of hydrogen in the visible part of the electromagnetic spectrum) to be observed at 656.5 nm instead of 656.3 nm as measured in a lab here on Earth. What is the velocity of this star in m/s? (Hint: speed of light is 3*10^8 m/s; leave the units off of your answer)
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