Questions

Review Questions

Question 12.1

What are the important thermonuclear reactions leading up to the formation of iron?

Question 12.2

Describe the steps leading up to a core-collapse supernova.

Question 12.3

How do neutron stars form?

Question 12.4

What are the differences between degenerate-electron pressure and degenerate-neutron pressure?

Question 12.5

How is a neutron star similar to a coastal lighthouse?

Question 12.6

What determines if a core-collapse supernova will form a neutron star or a black hole?

Question 12.7

What is the difference between a black hole’s event horizon and its Schwarzschild radius?

Question 12.8

When we say that the Moon has a radius of 1080 miles (1737 km), we mean that this is the smallest radius that encloses all of the Moon’s material. In this sense, is it correct to think of the Schwarzschild radius as the radius of a black hole? Why or why not?

Question 12.9

Astronomers cannot actually see the black hole candidates in close binary systems. How, then, do they know that these candidates are not white dwarfs or neutron stars?

Question 12.10

What are the differences between a Type Ia and a Type II supernova?

Question 12.11

What are the similarities between a nova and a Type Ia supernova? What are the differences?

Question 12.12

What is the similarity between a nova and an X-ray burster? How are they different?

Web Chat Questions

Question 12.1

Imagine that our Sun was somehow replaced by a 1-M white-dwarf star and that Earth continued in an orbit of semimajor axis 1 AU around this star. Discuss what effects this would have on our planet. What would the white dwarf look like as seen from Earth? Could you look at it safely with the unaided eye? Would Earth’s surface temperature remain the same as it is now?

Question 12.2

The similar names white dwarf, red dwarf, and brown dwarf describe three very different kinds of objects. Suggest better names for these three kinds of objects, and describe how your names more accurately describe the objects’ properties.

Question 12.3

Describe the kinds of observations you might make in order to locate and identify black holes.

Collaborative exercises

Question 12.1

Imagine that a supernova originating from a close binary star system, both of whose stars have less than 4 solar masses, began (as seen from Earth) on the most recent birthday of the youngest person in your group. Using the light curves in Figure 12-18, what would its new luminosity be today and how bright would it appear in the sky (apparent magnitude) if it were located 32.6 light-years away? How would your answers change if you were to discover that the supernova actually originated from an isolated star with a mass 15 times greater than our Sun?

Question 12.2

Consider the graph showing a recording of a pulsar in Figure 12-9. Sketch and label similar graphs that your group estimates for: (1) a rapidly spinning, professional ice skater holding a flashlight; (2) an emergency signal on an ambulance; and (3) a rotating beacon at an airport.

Question 12.3

As stars go, pulsars are tiny, only about 12 miles (20 km) across. Name three specific things or places that have a size or a separation of about 12 miles.

Observing Questions

Question 12.1

The red supergiant Betelgeuse in the constellation Orion will explode as a supernova at some time in the future. Use the Starry Night™ program to investigate how the supernova might appear if the light from this explosion were to arrive at Earth tonight. Click the Home button in the toolbar to show the sky as seen from your location at the present time. Use the Find pane to locate Betelgeuse. If Betelgeuse is below the horizon, allow the program to reset the time to show this star.

  • a) At what time does Betelgeuse rise on today’s date? At what time does it set?
  • b) What is the apparent magnitude (mV) of Betelgeuse? (Hint: Use the HUD or the Info pane to find this information.)
  • c) If Betelgeuse became a supernova today, then at peak brightness it would be 11 magnitudes brighter than it is now. (Note: Magnitudes increase as brightness decreases for stars.) For comparison, mV = −4 for Venus at its brightest and mV = −12.6 for the full moon. Would Betelgeuse be visible in the daytime? How would it appear at night? Do you think it would cast shadows?

Question 12.2

Use the Starry Night™ program to examine the Veil Nebula, a large supernova remnant. Open Favourites > Explorations > Veil Nebula to see a view of the nebula high in the sky of Calgary, Canada, at midnight on August 1, 2013.

  1. a) What significant feature do you notice about this supernova remnant in this 5-degree field of view?
  2. b) Use the angular separation tool to measure the approximate angular distance between the components of this nebula. What angular distance separates these components? What form of optical aid is best suited to observing this object?

300

Question 12.3

Use the Starry Night™ program to observe the sky in July 1054, when the supernova that spawned the Crab Nebula (M1) would have been visible, probably even in daylight, from North America and may have been recorded as a pictograph at this time by inhabitants of Chaco Canyon, New Mexico. Open Favourites > Explorations > Crab-Pictograph to position yourself in Chaco Canyon, at latitude 36°N and longitude 108°W at 5 a.m. on July 5, 1054, looking toward the east, just before sunrise. Zoom in to display a field of view of about 10° centered on the Crab Nebula, where you can see the position of the Moon near to the nebula. You may find it helpful to turn daylight on or off (select Show Daylight or Hide Daylight in the View menu).

  • a) What is the phase of the Moon?
  • b) Investigate how the relative positions of the Moon and the Crab Nebula change when you set the date to July 4, 1054, or July 6, 1054. On which date do the relative positions of the Moon and the Crab Nebula give the best match to the pictograph shown in the textbook? You can now investigate the nebula more closely by zooming in to see a ground-based view of this expanding gas cloud from the violent supernova explosion.

Question 12.4

Use the Starry Night™ program to investigate the X-ray source and probable black hole, Cygnus X-1. This region of space is one of the brightest in the sky at X-ray wavelengths. Click the Home button in the toolbar and then use the Find pane to center the field of view on Cygnus X-1. If Cygnus X-1 is below the horizon, allow the program to reset the time to when it can best be seen. Click the checkbox to the left of the listing for Cygnus X-1 to apply a label to this object. Use the Zoom controls to set the field of view to 100 degrees. Use the Time controls in the toolbar to determine when Cygnus X-1 rises and sets on today’s date from your location.