/*! 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} Problem 8 How can an astronomer tell the d... [FREE SOLUTION] | 91Ó°ÊÓ

91Ó°ÊÓ

How can an astronomer tell the difference between a planetary nebula and a planet?

Short Answer

Expert verified
An astronomer can tell the difference between a planetary nebula and a planet based on their appearances, movements, and spectral signatures. A planetary nebula emits its own light, is diffused with intricate shapes and colors, appears fixed in relation to stars and produces unique emission lines in spectroscopic observation. A planet doesn't emit light but reflects its star's light, appears as a bright point that moves relative to stars, and presents a spectral signature similar to its star.

Step by step solution

01

Understanding what a Planetary Nebula is

A planetary nebula is an astronomical object consisting of a glowing shell of gas and plasma formed by certain types of stars when they die. These are usually quite colourful and visible via a telescope as glowing objects in the sky.
02

Understanding what a Planet is

A planet, on the other hand, is a celestial body that orbits a star, is spherical in shape, and has cleared its orbit of other debris. It may be visible from Earth as a bright point in the night sky but does not emit its own light.
03

Differentiating between a Planetary Nebula and a Planet

There are multiple ways an astronomer can tell the difference between a planetary nebula and a planet. Firstly by their appearance, as a planet doesn't emit its own light, it will look like a bright point in the sky, while a planetary nebula emits light and gas, so it will have a more diffused appearance with intricate shapes and colors. Secondly, through spectral observation. Planets generally reflect the light of their star, so their spectroscopic signature is similar to that of their star. A nebula has a completely different substance and produces a distinct emission spectrum with bright emission lines. Thirdly by their movement, Planets move relative to the stars in the sky since they are orbiting a star. In contrast, a nebula is much further away and appears fixed in relation to the stars.

Unlock Step-by-Step Solutions & Ace Your Exams!

  • Full Textbook Solutions

    Get detailed explanations and key concepts

  • Unlimited Al creation

    Al flashcards, explanations, exams and more...

  • Ads-free access

    To over 500 millions flashcards

  • Money-back guarantee

    We refund you if you fail your exam.

Over 30 million students worldwide already upgrade their learning with 91Ó°ÊÓ!

One App. One Place for Learning.

All the tools & learning materials you need for study success - in one app.

Get started for free

Most popular questions from this chapter

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.

See all solutions

Recommended explanations on Physics Textbooks

View all explanations

What do you think about this solution?

We value your feedback to improve our textbook solutions.

Study anywhere. Anytime. Across all devices.