Homeworks 7

Homework 7 due on 10/26/09

Problem 1

Part 1

How long does it take a star with a mass of 1 M⊙ to form, from the beginning of its collapse from an gas cloud until its arrival on the main sequence? A star with a mass of 15 M⊙? Objects with masses less than 0.08 M⊙ never become hot enough in their cores to fuse hydrogen into helium. What happens to these low-mass objects?

Part 2

What observations give direct evidence for the existence of the following kinds of interstellar material?

1. Dust.
2. Massive, dense clouds with many molecules (molecular clouds).
3. Clouds of ionized hydrogen with temperatures near 10⁴ K (HII regions).
4. Clouds of neutral hydrogen with temperatures near 100 K (HI regions).
5. Extremely hot gas with temperatures near 10⁶ K (intercloud coronal gas).

Problem 2

Two hot, high-luminosity blue stars are embedded in an interstellar cloud. A picture of the stars and the cloud at visible wavelengths shows just one of the stars. It also shows that some parts of the cloud are blue and some parts have a green or red color.

1. What is the most likely reason that one star cannot be seen at visible wavelengths?
2. Why does part of the cloud look blue?
3. Why does part of the cloud look red?

Problem 3

Why is the chemical composition of the Earth and the other terrestrial planets so different from that of the sun? Why is the chemical composition of Jupiter and the other Jovian planets more similar to the sun’s?

Problem 4

Describe the evolution of a 1 solar mass star. Draw the HR-diagram and identify the significant phases of burning. Which events mark the ’transitions”? Provide the time scales for the various burning stages.