Deck 10: The Interstellar Medium

Question 1

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

A) density; volume
B) temperature; density
C) temperature; mass
D) temperature; volume
E) density; mass

Answer 1

temperature; density

Question 2

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

Answer 2

True

Question 3

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.

Answer 3

False

Question 4

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

Question 5

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

A) atoms and molecules in the ISM
B) only  atoms in the ISM
C) only molecules in the ISM
D) only dust in the ISM
E) dust, atoms and molecules of the ISM

Question 6

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.

A) unique lines
B) unresolved lines
C) forbidden lines
D) unseen lines
E) "fathom" lines

Question 7

H II Regions are also called emission nebulae.

Question 8

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

Question 9

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

A) oxygen III
B) oxygen II
C) helium II
D) carbon monoxide
E) carbon dioxide

Question 10

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

Question 11

H I clouds can be observed using _____.

A) optical telescopes above the earth's atmosphere
B) 21-cm radiation
C) x-ray radiation
D) infrared radiation
E) ultraviolet radiation

Question 12

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

Question 13

The interstellar medium is composed of mainly _____.

A) equal parts of gas and dust
B) mostly dust and some gas
C) mostly gas and some dust
D) dust only
E) gas only

Question 14

Stars are born in reflection nebulae.

Question 15

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

Question 16

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

Question 17

What is the most abundant element in the interstellar medium?

A) carbon
B) iron dust
C) carbon dust
D) helium
E) hydrogen

Question 18

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.

Question 19

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

A) 10
B) 20
C) 50
D) 100
E) 150

Question 20

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

A) 21 centimeters
B) 21 millimeters
C) 21 meters
D) 22.2 centimeters
E) 22.2 millimeters

Question 21

Which mission passed the bow shock in the Universe?

A) Cassini-Huygens
B) Interstellar Boundary Explorer
C) Voyager I
D) Voyager II
E) Kepler

Question 22

The _______________ is a high temperature, low density region in the interstellar medium around the Sun.

Question 23

Coronal gas radiates energy at ______________ wavelengths.

Question 24

To an observer on Earth, dust in the interstellar medium will cause a star to appear _______________ and_______________than it really is.

Question 26

The type of radiation that is emitted when the electron in a hydrogen atom experiences a spin flip is a (n) _______________.

Question 27

Large molecular clouds will form into protostars because of ____.

A) the thermal motions of the atoms in the gas cloud
B) gravitational contraction
C) radiation pressure from nearby stars
D) the temperature reaching a critical point
E) condensation of dust and gas

Question 28

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

A) K o r higher
B) more than K but less than K
C) 5000 K
D) between1000 K to 5000 K
E) less than 500K

Question 29

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

A) emission nebulae
B) H I
C) reflection nebulae
D) dark nebulae
E) spectral type B6

Question 30

Distinguish between pressure and density .   How are they related to each other?

Question 31

What observations indicate the presence of dust in the interstellar medium?

Question 32

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?

A) Spitzer Space Telescope
B) infrared telescope
C) European Southern Observatory
D) X-ray telescope
E) radio telescope

Question 33

What produces the coronal gas?

Question 34

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

A) emission nebulae
B) H I
C) reflection nebulae
D) dark nebulae
E) spectral type B6

Question 35

Interstellar dust scatters _____________light more than _____________light.

Question 36

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?

A) emission nebulae
B) H I
C) reflection nebulae
D) dark nebulae
E) spectral type B6

Question 37

The interstellar reddening does not shift the _______________ of spectral lines, as does the Doppler effect.

Question 38

Molecules in the interstellar medium emit radiation at what wavelengths?

A) radio
B) microwave
C) visible light
D) ultraviolet
E) X-ray

Question 39

What observations demonstrate the existence of an interstellar medium?

Question 40

Which mission is mapping the heliosphere's boundary?

A) Cassini-Huygens
B) Interstellar Boundary Explorer
C) Voyager I
D) Voyager II
E) Kepler

Question 41

Describe three ways in which astronomers can distinguish between interstellar absorption lines and stellar absorption lines.

Question 42

What are "forbidden lines"? Briefly describe how they form.

Question 43

If hydrogen (H₂) gas is the most common molecule found within the interstellar medium, then why do astronomers measure the amount of carbon monoxide (CO) gas to map molecular clouds?

Question 44

_______________ is believed to be produced by supernova explosions.

Question 45

Briefly discuss the gas-stars-gas cycle.

Question 46

Why doesn't warm, dense hydrogen emit 21-cm radiation?

Question 47

______________ are cool, with temperatures of about 100 K and densities of ten to a few hundreds of atoms per cubic centimeter.

Question 48

_______________ require that a young hot star (T ≥ 25,000 K) be relatively nearby.

Question 49

Why is the sky blue during the day?

Question 50

List the three types of nebulae in the Interstellar Medium.

Question 51

H II emission nebula regions are found around _____________.