chapter 10 py

studied byStudied by 1 person
5.0(1)
get a hint
hint

Nebula is just another name for the interstellar medium (ISM).

1 / 32

Tags and Description

33 Terms

1

Nebula is just another name for the interstellar medium (ISM).

true

New cards
2

Calculations of the Sun's future evolution indicate that it will blow away almost half of its mass in several relatively short episodes about 4 to 5 billion years from now before it is finally extinguished.

false

New cards
3

The composition of the interstellar dust suggests that it is formed primarily in the atmospheres of cool stars.

true

New cards
4

​Which type of nebulaeare twisted and distorted clouds of gas and dust dense enough to obstruct the view of the more distant stars?

\n ​dark nebulae

New cards
5

H I clouds can be observed using _____.

21 cm radiation

New cards
6

​Which telescope imaged the center of the Milky Way Galaxy at a wavelength of 8 microns to reveal the distribution of the dusty interstellar medium?

Spitzer Space Telescope

New cards
7

Coronal gas emits x-rays and has temperatures of ____.

10^6 K or higher

New cards
8

​Observing at a wide range of wavelengths, astronomers have detected more than ______ different molecules in the ISM.

150

New cards
9

At infrared wavelengths, the ISM glows with blackbody radiation emitted by the interstellar dust.

true

New cards
10

Elements such as carbon, silicon and oxygen have been produced in stars and expelled as stars age in the interstellar medium. This is most likely due to these elements having cooled and condensed from aging stars to form dust grains, and carried out by a powerful winds.

true

New cards
11

Because blue light has a shorter wavelength than red light, it will be more readily scattered.

true

New cards
12

H II Regions are also called emission nebulae.

true

New cards
13

​Which type of nebulae is produced when short-wavelength scatters from the dust and displays a blue hue?

reflection nebulae

New cards
14

​What is the most abundant element in the interstellar medium?

hydrogen

New cards
15

Interstellar extinction and the reddening of light by the interstellar medium (ISM) are both caused by _____.

only dust in the ISM

New cards
16

The intercloud medium is believed to make up 90 percent of the mass of the interstellar medium.

false

New cards
17

X-rays come from certain regions of the interstellar medium because gas molecules in those regions are at a very high density.

false

New cards
18

​Which type of nebula is produced when a star, hotter than 25,000 K, excites the gas near it to produce an emission spectrum producing a distinctive pink color?

emission nebulae

New cards
19

​Which mission passed the bow shock in the Universe?

Voyager I

New cards
20

​Large molecular clouds will form into protostars because of ____.

gravitational contraction

New cards
21

Stars are born in reflection nebulae.

false

New cards
22

Stars are born from the interstellar medium, and aging or dying stars return gas and dust back into the interstellar medium.

true

New cards
23

​The interstellar medium is composed of mainly _____.

mostly gas and some dust

New cards
24

The ground state of hydrogen has two closely-spaced energy levels, where one-electron is spinning up and the other is spinning down. This energy transition corresponds to releasing excess energy as a photon at what wavelength?

21 centimenters

New cards
25

The coronal gas in the interstellar medium has very high temperatures similar to the Sun's corona.

true

New cards
26

Molecular clouds are mapped using _____ gas instead of the most-abundant hydrogen because it radiates at radio wavelengths more efficiently.

carbon monoxide

New cards
27

​Which mission is mapping the heliosphere's boundary?

interstellar boundary explorer

New cards
28

The spacecraft ________ captured particles that scientists believe came from the ISM.

Stardust

New cards
29

The ISM is easily visible to human eyes.

false

New cards
30

Which molecule has not been detected in molecular clouds?

All of these have been detected

New cards
31

​The emission lines from O III are called ____ because they are not visible laboratories on Earth due to the much greater pressure of the gas on Earth.

forbidden lines

New cards
32

​The pressure of a gas depends on the ____ and ____ of the gas.

temperature; density

New cards
33

​Molecules in the interstellar medium emit radiation at what wavelengths?

radio

New cards

Explore top notes

note Note
studied byStudied by 6 people
Updated ... ago
5.0 Stars(1)
note Note
studied byStudied by 14 people
Updated ... ago
5.0 Stars(1)
note Note
studied byStudied by 36 people
Updated ... ago
5.0 Stars(3)
note Note
studied byStudied by 5 people
Updated ... ago
5.0 Stars(1)
note Note
studied byStudied by 8 people
Updated ... ago
5.0 Stars(1)
note Note
studied byStudied by 12 people
Updated ... ago
5.0 Stars(1)
note Note
studied byStudied by 1 person
Updated ... ago
5.0 Stars(1)
note Note
studied byStudied by 89159 people
Updated ... ago
4.9 Stars(507)

Explore top flashcards

flashcards Flashcard76 terms
studied byStudied by 1 person
Updated ... ago
5.0 Stars(1)
flashcards Flashcard87 terms
studied byStudied by 30 people
Updated ... ago
5.0 Stars(1)
flashcards Flashcard55 terms
studied byStudied by 27 people
Updated ... ago
5.0 Stars(2)
flashcards Flashcard207 terms
studied byStudied by 7 people
Updated ... ago
5.0 Stars(1)
flashcards Flashcard82 terms
studied byStudied by 2 people
Updated ... ago
5.0 Stars(1)
flashcards Flashcard94 terms
studied byStudied by 27 people
Updated ... ago
5.0 Stars(1)
flashcards Flashcard62 terms
studied byStudied by 1 person
Updated ... ago
5.0 Stars(1)
flashcards Flashcard86 terms
studied byStudied by 100 people
Updated ... ago
5.0 Stars(1)