NSCI 111 ASTRONOMY TEST #4 6/30/2007 Dr. Holmes NAME

ANSWER ALL THE QUESTIONS. THE WORTH OF EACH QUESTION IS IN () AFTER THE QUESTION.

 

1. (10) Fill in the following for two stars (excluding the sun)

Name of star

Constellation in which star is found

Absolute Magnitude

Apparent Magnitude

Distance from Earth

Spectral Class

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2. (16) Draw an H-R diagram, labeling both axes and indicating where the main sequence, giants, supergiants and white dwarfs are located. Also, place the sun and the two stars of problem #1 on the diagram.

 

3. (a) (4) What is a sunspot?

(b) (4) What is the solar wind? 

 

4. (6) Name and briefly describe two ways distances to the stars are determined.

1.

2.

 

5. (6) Name and briefly describe two of the ways of detecting binary stars:

1.

2.

 

6. (5) Why are binary stars important (i.e., how do they help us determine stellar properties) ?

 

7. a) (3) Distinguish between brightness and luminosity:

b) (3) Distinguish between apparent magnitude and absolute magnitude:

 

8.  (9)  Name three possible ways a star will end up after it has finished burning its fuel:

            1.

 

 

 

            2.

 

 

 

            3.

 

 

9. (4) What property of a star determines which of the above ways that star will end up?

 

10. a) (3) What is a Cephied variable star?

b) (3) Why is this type of star important?

 

11. (10) Draw another H-R diagram, labeling the axes and showing the position of the main sequence, and then draw in the life cycle of a star like the sun, and explain what is happening at each stage of the cycle.

 

12.  a) (2) What is a neutron star?

 

 

 

 

       b) (2)  When is a neutron star formed?

 

 

13. TRUE or FALSE: (+1 points each if correct, 0 if left blank, -1 if wrong)

                                    (or subtracting from 100: -0 if correct, -1 if blank, -2 if wrong)

__T___ a) The diameter of the sun is about 1% of the earth-sun distance (about means within a range from 0.5% to 5%).  Therefore it is larger than the earth to moon distance.

 

__F___ b) The sun should last a total of about 10 million years on the main sequence (about means within a range from 1 million to 100 million).

 

__T___ c) The average power from the sun falling on one square meter on the earth’s surface is about 250 Watts (about means within a range from 100 to 1000).

__F___ d) Binary star systems are relatively rare. Most stars that we see are single stars like the sun.

__F__  e) Some nebulae appear to be the result of exploding planets while others appear to be the result of exploding stars.

 

__T___ f) While the distance to the sun is several light minutes, the distance to the nearest star (excluding the sun) is several light years.

 

__F__  g) Sunspots are permanent spots on the sun’s surface.  They have lasted as long as we have been able to observe the sun.  Galileo saw the exact same spots we see today.

 

__F___ h) When the sun's hydrogen in its core is used up, the outer parts of the sun will probably expand to beyond the orbit of Pluto as the sun becomes a red giant star.

 

__F___ i) A supernova is when a star literally explodes and blows itself apart.  The energy output during the explosion is equivalent to that of around a hundred normal stars.

 

__F___ j) More massive stars last longer on the main sequence than less massive stars because they have more fuel (mass).

 

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