Chapter 20: Problem 8
How can an astronomer tell the difference between a planetary nebula and a planet?
/*! This file is auto-generated */ .wp-block-button__link{color:#fff;background-color:#32373c;border-radius:9999px;box-shadow:none;text-decoration:none;padding:calc(.667em + 2px) calc(1.333em + 2px);font-size:1.125em}.wp-block-file__button{background:#32373c;color:#fff;text-decoration:none}
Learning Materials
Features
Discover
Chapter 20: Problem 8
How can an astronomer tell the difference between a planetary nebula and a planet?
All the tools & learning materials you need for study success - in one app.
Get started for free
In what way does the structure of an aging supergiant resemble that of an onion?
Imagine that our Sun was somehow replaced by a \(1-\mathrm{M}_{\odot}\) white dwarf star, and that our Earth continued in an orbit of semimajor axis \(1 \mathrm{AU}\) 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 the Earth's surface temperature remain the same as it is now?
. Is our own Sun likely to become a supernova? Why or why not?
Use the Starry Night Enthusiast \({ }^{\text {TM }}\) program to show the location of Supernova \(1987 \mathrm{~A}\). In the menu, select Favourites \(>\) Deep Space \(>\) Local Universe to display the Milky Way and other nearby galaxies, conveniently labeled, against the background of distant galaxies, from a distance of \(0.282\) Mly from the Sun. (If the Milky Way does not appear immediately, click once on either of the Zoom buttons.) Remove the image of the astronaut's feet by clicking on View > Feet. You can rotate the Milky Way Galaxy and its neighbor galaxies by holding down both the Shift button and the mouse button while moving the mouse. (On a two-button mouse, hold down the left mouse button.) (a) Use the Find pane to locate and center the Sun in the field of view. Describe the position of the Large Magellanic Cloud (LMC), within which SN \(1987 \mathrm{~A}\) lies, relative to the Milky Way Galaxy and to our solar system. (b) Use the Find pane to center on the LMC. You should be able to locate the Tarantula Nebula, shown in Figure 20-17. Is SN 1987A near to the center or the edge of the LMC? (Note that, although Starry Night Enthusiast \({ }^{\mathrm{TM}}\) depicts the LMC as being rather flat, it is thought to be an irregular blob of stars with some thickness.)
The central star in a newly formed planetary nebula has a luminosity of \(1000 \mathrm{~L}_{\odot}\) and a surface temperature of \(100,000 \mathrm{~K}\). What is the star's radius? Give your answer as a multiple of the Sun's radius.
What do you think about this solution?
We value your feedback to improve our textbook solutions.