Deck 15: The Milky Way Galaxy

ملء الشاشة (f)
exit full mode
سؤال
The age of the Milky Way galaxy has been estimated to be at least 13 billion years based on

A) observations of globular clusters.
B) observations of open clusters.
C) 21cm radiation from H I regions.
D) the rotation curve of the galaxy.
E) the energy produced by Sagittarius A*
استخدم زر المسافة أو
up arrow
down arrow
لقلب البطاقة.
سؤال
Halo stars located in the disk are easy to detect because they

A) are the only low mass stars in the disk.
B) are only found in globular clusters.
C) are primarily O and B supergiants.
D) move at an angle across the disk.
E) emit cosmic rays.
سؤال
Population II stars <strong>Population II stars  </strong> A) III & IV B) I & II C) II D) IV E) I,II,& III <div style=padding-top: 35px>

A) III & IV
B) I & II
C) II
D) IV
E) I,II,& III
سؤال
The orbits of population I stars <strong>The orbits of population I stars  </strong> A) I B) IV C) I & IV D) II & IV E) I & III <div style=padding-top: 35px>

A) I
B) IV
C) I & IV
D) II & IV
E) I & III
سؤال
The traditional monolithic collapse theory for the formation of the Milky Way Galaxy suggests that our galaxy formed

A) as material accreted around a massive black hole currently at the center of our galaxy.
B) from a large cloud of material that formed stars and star clusters and slowly flattened to a disk.
C) from material that had been ejected in the violent explosion of a dying galaxy.
D) as a result of mergers between several smaller groups of gas,dust,and stars.
E) as two massive galaxies collided.
سؤال
The magnetic field of the galaxy

A) is stronger than the magnetic field of the sun.
B) traps cosmic rays in the disk of the galaxy.
C) creates the spiral density waves that initiate star formation.
D) forces the halo stars to follow highly inclined orbits.
E) produces 21-cm radiation that allows us to map the spiral arms.
سؤال
The first stars to form in our galaxy

A) had circular orbits.
B) had highly elliptical orbits.
C) were population I stars.
D) all had orbits in the same plane.
سؤال
Galaxy spiral arms are traced out (outlined)by stars which are <strong>Galaxy spiral arms are traced out (outlined)by stars which are  </strong> A) I & III B) I & IV C) II & III D) II & IV E) I,III,& IV <div style=padding-top: 35px>

A) I & III
B) I & IV
C) II & III
D) II & IV
E) I,III,& IV
سؤال
Diagram 15-1 <strong>Diagram 15-1    -Refer to Diagram 15-1.A type II Cepheid has been located in a distant globular cluster with a period of 10 days.What is the star's absolute magnitude?</strong> A) (-1) B) 0 C) (-4) D)( -6) E) The absolute magnitude of a Cepheid variable cannot be determined unless its distance is known. <div style=padding-top: 35px>

-Refer to Diagram 15-1.A type II Cepheid has been located in a distant globular cluster with a period of 10 days.What is the star's absolute magnitude?

A) (-1)
B) 0
C) (-4)
D)( -6)
E) The absolute magnitude of a Cepheid variable cannot be determined unless its distance is known.
سؤال
Our galaxy is suspected to be surrounded by a galactic corona because the disk of the galaxy

A) rotates faster than expected in its outer region.
B) rotates more slowly than expected in its outer region.
C) rotates faster than expected in its inner region.
D) rotates more slowly than expected in its inner region.
E) is much flatter than expected.
سؤال
The nuclear bulge of our galaxy

A) contains stars that are primarily population I stars.
B) contains relatively large amounts of gas and dust.
C) contains stars primarily associated with the spherical component of our galaxy.
D) contains stars primarily associated with the disk component of our galaxy.
E) a,b,and d
سؤال
Which of the following is not a characteristic of the stars of the disk component of our galaxy?

A) circular orbits
B) randomly inclined orbits
C) higher metal abundance
D) young stars
E) star formation regions
سؤال
Herschel's grindstone and Kapteyn's star system were too small because

A) they did not count the brightest stars.
B) they did not study the southern sky.
C) they did not have large enough telescopes.
D) they only observed stars in the disk of the galaxy and not the halo.
E) they did not know about interstellar dust clouds.
سؤال
Younger stars formed not so long ago have more heavy elements than stars formed early in the history of our Galaxy because

A) old stars destroy heavy elements as they age.
B) young stars burn their nuclear fuels faster.
C) heavy elements were made in previous generations of stars.
D) all of the above
E) heavy elements haven't had time to settle to the core of these younger stars.
سؤال
Nucleosynthesis

A) is the process by which energy is produced at the center of the galaxy.
B) is the process by which hydrogen and helium are converted into heavier elements.
C) describes the structure of a globular cluster.
D) describes how the magnetic field of the galaxy traps cosmic rays.
E) describes the method by which neutral hydrogen produces 21 cm radiation.
سؤال
The center of our galaxy lies in the direction of the constellation of

A) Ursa Minor.
B) Ursa Major.
C) Sagittarius.
D) Orion.
E) Monoceros.
سؤال
A group of 10 to 100 stars that formed at the same time but are so widely scattered in space their mutual gravity cannot hold them together is called

A) a globular cluster.
B) an open cluster.
C) an association.
D) a spherical component.
E) an accretion disk.
سؤال
Compared to population II,the larger abundance of atoms more massive than hydrogen and helium in population I stars

A) indicates that they were formed before the population II stars.
B) indicates that the material they formed from had been enriched with material from supernovae.
C) indicates that they contain very few heavy metals compared to halo stars.
D) depends on the temperature of the star.
E) depends on the mass of the star.
سؤال
The first scientific attempt to map the Milky Way galaxy

A) showed that the Sun was located in the center of the system of planets making up our Galaxy.
B) showed that our Galaxy is a round ball on which we live.
C) showed that our Galaxy has 9 stars
D) used globular clusters to determine the location of the center of the galaxy.
E) was completed by William and Caroline Herschel.
سؤال
Diagram 15-1 <strong>Diagram 15-1   Refer to Diagram 15-1.A type I Cepheid has been located in an open cluster.The period of the Cepheid variable is 30 days,and the variable's apparent visual magnitude is 10.What is the distance to this open cluster?</strong> A) 100 pc B) 10,000 pc C) 20 pc D) 300 pc E) 2500 pc <div style=padding-top: 35px>
Refer to Diagram 15-1.A type I Cepheid has been located in an open cluster.The period of the Cepheid variable is 30 days,and the variable's apparent visual magnitude is 10.What is the distance to this open cluster?

A) 100 pc
B) 10,000 pc
C) 20 pc
D) 300 pc
E) 2500 pc
سؤال
The energy source at the center of our galaxy

A) is not visible at optical wavelengths.
B) produces gamma rays.
C) must be less than 10 AU in diameter.
D) all of the above
E) none of the above
سؤال
How is the age of the galaxy determined?

A) Measuring the metallicity of Population II stars.
B) Finding the turnoff point in the H-R diagram of globular clusters.
C) From the motion of stars in the galactic halo.
D) Counting the number of open clusters in the spiral arms.
سؤال
How did Harlow Shapley determine where the center of the galaxy lies?

A) He plotted the distribution of open clusters.
B) He plotted the distribution of globular clusters.
C) He made star counts in every direction of the galactic disk.
D) He measured the amount of dust obscuration in every direction of the galactic disk.
سؤال
Shapley found the distance to the center of the galaxy by studying the distance to open clusters.
سؤال
How did Harlow Shapley use the period-luminosity relationship of Cepheid variables to determine the size of the Milky Way galaxy?

A) He determined the proper motion of globular clusters in the outer disk of the galaxy.
B) He found the distance to individual Cepheid variables free floating in the halo.
C) He found the distance to open clusters found throughout the disk of the galaxy.
D) He found the distance to globular clusters distributed about the center of the galaxy.
سؤال
Radio maps of our galaxy show spiral arms because the

A) arms have high Doppler shifts.
B) gas in the spiral arms is hot enough to emit photons.
C) dust in spiral arms is more dense than it is between the spiral arms.
D) gas in spiral arms is more dense than it is between the spiral arms.
E) stars in the spiral arms emit most of their energy at radio wavelengths.
سؤال
What behavior do galactic rotation curves exhibit to suggest the existence of dark matter?

A) Small velocities are seen at large distances from the galactic center.
B) Small velocities are seen at distances close to the galactic center.
C) Large velocities are seen at large distances from the galactic center.
D) Large velocities are seen at distances close to the galactic center.
سؤال
Astronomers before Shapely underestimated the size of the Milky Way galaxy because they lacked large enough telescopes.
سؤال
In the edge-on sketch of a spiral galaxy,pick the letter corresponding most nearly to the location of globular clusters. <strong>In the edge-on sketch of a spiral galaxy,pick the letter corresponding most nearly to the location of globular clusters.  </strong> A) A B) B C) C D) D <div style=padding-top: 35px>

A) A
B) B
C) C
D) D
سؤال
If the spiral density wave were the only thing producing spiral arms,it would be expected that

A) all spiral arms would be dust free.
B) all galaxies would have grand design spiral patterns.
C) the Milky Way would be more massive than observed.
D) the Milky Way wouldn't have any spiral arms.
E) the halo component of the Milky way would show spiral arms as well.
سؤال
The disk of our galaxy consists of

A) the nine known planets
B) only stars
C) stars,dust,and gas
D) quasars
E) only black holes
سؤال
Radio maps of the spiral arms of our galaxy

A) reveal that our galaxy is a grand design spiral.
B) map the location of Hot O and B stars by the radio radiation they emit.
C) reveal that the spiral arms are winding up and growing closer together.
D) reveal that the sun is currently located in the center of a spiral arm.
E) map the location of dense neutral hydrogen clouds.
سؤال
How does the traditional monolithic collapse theory of the formation of the galaxy explain the origin of globular clusters?

A) They formed in the disk and later were ejected to the halo.
B) They formed in other galaxies and were captured by close interactions.
C) They build over time from the collision of stars in the halo.
D) They formed early on during the free-fall collapse of the proto-galactic material.
سؤال
A several million solar mass ____ is thought to be at the center of our galaxy.

A) spiral arm
B) globular cluster
C) planet
D) black hole
سؤال
The energy source at the center of our galaxy is called

A) Cygnus X-1.
B) the Orion arm.
C) the sun.
D) Sagittarius A*.
سؤال
Our Milky Way Galaxy is about...

A) 1 light year across
B) 10 light years across
C) 100 light years across
D) 1000 light years across
E) 100,000 light years across
سؤال
This is a "thought" question.Why are few galaxies outside our own galaxy seen in the circle around the sky where the Milky Way is located? This is because ...

A) there aren't any galaxies in those directions
B) dust in the Milky Way blots out our view of galaxies in those directions
C) the missing mass is in those directions
D) the Big Bang has blown galaxies away from those directions
سؤال
CO observations of the galaxy reveal

A) the location of dense neutral hydrogen clouds.
B) the location of population II stars.
C) the location of population I stars.
D) the location of the galactic corona.
E) the location of giant molecular clouds.
سؤال
The disk of the Milky Way is approximately 20,000 ly in diameter.
سؤال
If a star with a peculiar space motion with respect a typical disk star is found what other property would you expect it to have?

A) Low luminosity.
B) Poor metal content compared to the Sun.
C) Old age.
D) All of the above.
سؤال
The rotation curve of the galaxy provides evidence for the existence of the ____________________ which extends beyond the halo of the galaxy.
سؤال
____________________ are groups of 100,000 to 1,000,000 population II stars firmly bound by gravity.
سؤال
Population II stars contain more metals than Population I stars.
سؤال
The orbits of halo stars are typically circular and have a low inclination with respect to the disk.
سؤال
The ____________________ of the galaxy contains population I stars,open clusters,and gas clouds.
سؤال
Globular clusters are primarily found in the ____________________ component of the Galaxy.
سؤال
Henrietta Leavitt discovered the period-luminosity relationship for ____________________.
سؤال
Spiral tracers tend to be old,luminous stars.
سؤال
The center of our galaxy shows signs of past eruptions.
سؤال
The density wave theory explains spurs and branches along the spiral arms.
سؤال
Giant molecular cloud complexes are located in spiral arms.
سؤال
The rapid rotation in the outer disk suggests that our galaxy is more massive than previously thought.
سؤال
Old stars are poor in heavy atoms because there were no previous generations of stars.
سؤال
The disk of the galaxy is older than the halo.
فتح الحزمة
قم بالتسجيل لفتح البطاقات في هذه المجموعة!
Unlock Deck
Unlock Deck
1/54
auto play flashcards
العب
simple tutorial
ملء الشاشة (f)
exit full mode
Deck 15: The Milky Way Galaxy
1
The age of the Milky Way galaxy has been estimated to be at least 13 billion years based on

A) observations of globular clusters.
B) observations of open clusters.
C) 21cm radiation from H I regions.
D) the rotation curve of the galaxy.
E) the energy produced by Sagittarius A*
observations of globular clusters.
2
Halo stars located in the disk are easy to detect because they

A) are the only low mass stars in the disk.
B) are only found in globular clusters.
C) are primarily O and B supergiants.
D) move at an angle across the disk.
E) emit cosmic rays.
move at an angle across the disk.
3
Population II stars <strong>Population II stars  </strong> A) III & IV B) I & II C) II D) IV E) I,II,& III

A) III & IV
B) I & II
C) II
D) IV
E) I,II,& III
III & IV
4
The orbits of population I stars <strong>The orbits of population I stars  </strong> A) I B) IV C) I & IV D) II & IV E) I & III

A) I
B) IV
C) I & IV
D) II & IV
E) I & III
فتح الحزمة
افتح القفل للوصول البطاقات البالغ عددها 54 في هذه المجموعة.
فتح الحزمة
k this deck
5
The traditional monolithic collapse theory for the formation of the Milky Way Galaxy suggests that our galaxy formed

A) as material accreted around a massive black hole currently at the center of our galaxy.
B) from a large cloud of material that formed stars and star clusters and slowly flattened to a disk.
C) from material that had been ejected in the violent explosion of a dying galaxy.
D) as a result of mergers between several smaller groups of gas,dust,and stars.
E) as two massive galaxies collided.
فتح الحزمة
افتح القفل للوصول البطاقات البالغ عددها 54 في هذه المجموعة.
فتح الحزمة
k this deck
6
The magnetic field of the galaxy

A) is stronger than the magnetic field of the sun.
B) traps cosmic rays in the disk of the galaxy.
C) creates the spiral density waves that initiate star formation.
D) forces the halo stars to follow highly inclined orbits.
E) produces 21-cm radiation that allows us to map the spiral arms.
فتح الحزمة
افتح القفل للوصول البطاقات البالغ عددها 54 في هذه المجموعة.
فتح الحزمة
k this deck
7
The first stars to form in our galaxy

A) had circular orbits.
B) had highly elliptical orbits.
C) were population I stars.
D) all had orbits in the same plane.
فتح الحزمة
افتح القفل للوصول البطاقات البالغ عددها 54 في هذه المجموعة.
فتح الحزمة
k this deck
8
Galaxy spiral arms are traced out (outlined)by stars which are <strong>Galaxy spiral arms are traced out (outlined)by stars which are  </strong> A) I & III B) I & IV C) II & III D) II & IV E) I,III,& IV

A) I & III
B) I & IV
C) II & III
D) II & IV
E) I,III,& IV
فتح الحزمة
افتح القفل للوصول البطاقات البالغ عددها 54 في هذه المجموعة.
فتح الحزمة
k this deck
9
Diagram 15-1 <strong>Diagram 15-1    -Refer to Diagram 15-1.A type II Cepheid has been located in a distant globular cluster with a period of 10 days.What is the star's absolute magnitude?</strong> A) (-1) B) 0 C) (-4) D)( -6) E) The absolute magnitude of a Cepheid variable cannot be determined unless its distance is known.

-Refer to Diagram 15-1.A type II Cepheid has been located in a distant globular cluster with a period of 10 days.What is the star's absolute magnitude?

A) (-1)
B) 0
C) (-4)
D)( -6)
E) The absolute magnitude of a Cepheid variable cannot be determined unless its distance is known.
فتح الحزمة
افتح القفل للوصول البطاقات البالغ عددها 54 في هذه المجموعة.
فتح الحزمة
k this deck
10
Our galaxy is suspected to be surrounded by a galactic corona because the disk of the galaxy

A) rotates faster than expected in its outer region.
B) rotates more slowly than expected in its outer region.
C) rotates faster than expected in its inner region.
D) rotates more slowly than expected in its inner region.
E) is much flatter than expected.
فتح الحزمة
افتح القفل للوصول البطاقات البالغ عددها 54 في هذه المجموعة.
فتح الحزمة
k this deck
11
The nuclear bulge of our galaxy

A) contains stars that are primarily population I stars.
B) contains relatively large amounts of gas and dust.
C) contains stars primarily associated with the spherical component of our galaxy.
D) contains stars primarily associated with the disk component of our galaxy.
E) a,b,and d
فتح الحزمة
افتح القفل للوصول البطاقات البالغ عددها 54 في هذه المجموعة.
فتح الحزمة
k this deck
12
Which of the following is not a characteristic of the stars of the disk component of our galaxy?

A) circular orbits
B) randomly inclined orbits
C) higher metal abundance
D) young stars
E) star formation regions
فتح الحزمة
افتح القفل للوصول البطاقات البالغ عددها 54 في هذه المجموعة.
فتح الحزمة
k this deck
13
Herschel's grindstone and Kapteyn's star system were too small because

A) they did not count the brightest stars.
B) they did not study the southern sky.
C) they did not have large enough telescopes.
D) they only observed stars in the disk of the galaxy and not the halo.
E) they did not know about interstellar dust clouds.
فتح الحزمة
افتح القفل للوصول البطاقات البالغ عددها 54 في هذه المجموعة.
فتح الحزمة
k this deck
14
Younger stars formed not so long ago have more heavy elements than stars formed early in the history of our Galaxy because

A) old stars destroy heavy elements as they age.
B) young stars burn their nuclear fuels faster.
C) heavy elements were made in previous generations of stars.
D) all of the above
E) heavy elements haven't had time to settle to the core of these younger stars.
فتح الحزمة
افتح القفل للوصول البطاقات البالغ عددها 54 في هذه المجموعة.
فتح الحزمة
k this deck
15
Nucleosynthesis

A) is the process by which energy is produced at the center of the galaxy.
B) is the process by which hydrogen and helium are converted into heavier elements.
C) describes the structure of a globular cluster.
D) describes how the magnetic field of the galaxy traps cosmic rays.
E) describes the method by which neutral hydrogen produces 21 cm radiation.
فتح الحزمة
افتح القفل للوصول البطاقات البالغ عددها 54 في هذه المجموعة.
فتح الحزمة
k this deck
16
The center of our galaxy lies in the direction of the constellation of

A) Ursa Minor.
B) Ursa Major.
C) Sagittarius.
D) Orion.
E) Monoceros.
فتح الحزمة
افتح القفل للوصول البطاقات البالغ عددها 54 في هذه المجموعة.
فتح الحزمة
k this deck
17
A group of 10 to 100 stars that formed at the same time but are so widely scattered in space their mutual gravity cannot hold them together is called

A) a globular cluster.
B) an open cluster.
C) an association.
D) a spherical component.
E) an accretion disk.
فتح الحزمة
افتح القفل للوصول البطاقات البالغ عددها 54 في هذه المجموعة.
فتح الحزمة
k this deck
18
Compared to population II,the larger abundance of atoms more massive than hydrogen and helium in population I stars

A) indicates that they were formed before the population II stars.
B) indicates that the material they formed from had been enriched with material from supernovae.
C) indicates that they contain very few heavy metals compared to halo stars.
D) depends on the temperature of the star.
E) depends on the mass of the star.
فتح الحزمة
افتح القفل للوصول البطاقات البالغ عددها 54 في هذه المجموعة.
فتح الحزمة
k this deck
19
The first scientific attempt to map the Milky Way galaxy

A) showed that the Sun was located in the center of the system of planets making up our Galaxy.
B) showed that our Galaxy is a round ball on which we live.
C) showed that our Galaxy has 9 stars
D) used globular clusters to determine the location of the center of the galaxy.
E) was completed by William and Caroline Herschel.
فتح الحزمة
افتح القفل للوصول البطاقات البالغ عددها 54 في هذه المجموعة.
فتح الحزمة
k this deck
20
Diagram 15-1 <strong>Diagram 15-1   Refer to Diagram 15-1.A type I Cepheid has been located in an open cluster.The period of the Cepheid variable is 30 days,and the variable's apparent visual magnitude is 10.What is the distance to this open cluster?</strong> A) 100 pc B) 10,000 pc C) 20 pc D) 300 pc E) 2500 pc
Refer to Diagram 15-1.A type I Cepheid has been located in an open cluster.The period of the Cepheid variable is 30 days,and the variable's apparent visual magnitude is 10.What is the distance to this open cluster?

A) 100 pc
B) 10,000 pc
C) 20 pc
D) 300 pc
E) 2500 pc
فتح الحزمة
افتح القفل للوصول البطاقات البالغ عددها 54 في هذه المجموعة.
فتح الحزمة
k this deck
21
The energy source at the center of our galaxy

A) is not visible at optical wavelengths.
B) produces gamma rays.
C) must be less than 10 AU in diameter.
D) all of the above
E) none of the above
فتح الحزمة
افتح القفل للوصول البطاقات البالغ عددها 54 في هذه المجموعة.
فتح الحزمة
k this deck
22
How is the age of the galaxy determined?

A) Measuring the metallicity of Population II stars.
B) Finding the turnoff point in the H-R diagram of globular clusters.
C) From the motion of stars in the galactic halo.
D) Counting the number of open clusters in the spiral arms.
فتح الحزمة
افتح القفل للوصول البطاقات البالغ عددها 54 في هذه المجموعة.
فتح الحزمة
k this deck
23
How did Harlow Shapley determine where the center of the galaxy lies?

A) He plotted the distribution of open clusters.
B) He plotted the distribution of globular clusters.
C) He made star counts in every direction of the galactic disk.
D) He measured the amount of dust obscuration in every direction of the galactic disk.
فتح الحزمة
افتح القفل للوصول البطاقات البالغ عددها 54 في هذه المجموعة.
فتح الحزمة
k this deck
24
Shapley found the distance to the center of the galaxy by studying the distance to open clusters.
فتح الحزمة
افتح القفل للوصول البطاقات البالغ عددها 54 في هذه المجموعة.
فتح الحزمة
k this deck
25
How did Harlow Shapley use the period-luminosity relationship of Cepheid variables to determine the size of the Milky Way galaxy?

A) He determined the proper motion of globular clusters in the outer disk of the galaxy.
B) He found the distance to individual Cepheid variables free floating in the halo.
C) He found the distance to open clusters found throughout the disk of the galaxy.
D) He found the distance to globular clusters distributed about the center of the galaxy.
فتح الحزمة
افتح القفل للوصول البطاقات البالغ عددها 54 في هذه المجموعة.
فتح الحزمة
k this deck
26
Radio maps of our galaxy show spiral arms because the

A) arms have high Doppler shifts.
B) gas in the spiral arms is hot enough to emit photons.
C) dust in spiral arms is more dense than it is between the spiral arms.
D) gas in spiral arms is more dense than it is between the spiral arms.
E) stars in the spiral arms emit most of their energy at radio wavelengths.
فتح الحزمة
افتح القفل للوصول البطاقات البالغ عددها 54 في هذه المجموعة.
فتح الحزمة
k this deck
27
What behavior do galactic rotation curves exhibit to suggest the existence of dark matter?

A) Small velocities are seen at large distances from the galactic center.
B) Small velocities are seen at distances close to the galactic center.
C) Large velocities are seen at large distances from the galactic center.
D) Large velocities are seen at distances close to the galactic center.
فتح الحزمة
افتح القفل للوصول البطاقات البالغ عددها 54 في هذه المجموعة.
فتح الحزمة
k this deck
28
Astronomers before Shapely underestimated the size of the Milky Way galaxy because they lacked large enough telescopes.
فتح الحزمة
افتح القفل للوصول البطاقات البالغ عددها 54 في هذه المجموعة.
فتح الحزمة
k this deck
29
In the edge-on sketch of a spiral galaxy,pick the letter corresponding most nearly to the location of globular clusters. <strong>In the edge-on sketch of a spiral galaxy,pick the letter corresponding most nearly to the location of globular clusters.  </strong> A) A B) B C) C D) D

A) A
B) B
C) C
D) D
فتح الحزمة
افتح القفل للوصول البطاقات البالغ عددها 54 في هذه المجموعة.
فتح الحزمة
k this deck
30
If the spiral density wave were the only thing producing spiral arms,it would be expected that

A) all spiral arms would be dust free.
B) all galaxies would have grand design spiral patterns.
C) the Milky Way would be more massive than observed.
D) the Milky Way wouldn't have any spiral arms.
E) the halo component of the Milky way would show spiral arms as well.
فتح الحزمة
افتح القفل للوصول البطاقات البالغ عددها 54 في هذه المجموعة.
فتح الحزمة
k this deck
31
The disk of our galaxy consists of

A) the nine known planets
B) only stars
C) stars,dust,and gas
D) quasars
E) only black holes
فتح الحزمة
افتح القفل للوصول البطاقات البالغ عددها 54 في هذه المجموعة.
فتح الحزمة
k this deck
32
Radio maps of the spiral arms of our galaxy

A) reveal that our galaxy is a grand design spiral.
B) map the location of Hot O and B stars by the radio radiation they emit.
C) reveal that the spiral arms are winding up and growing closer together.
D) reveal that the sun is currently located in the center of a spiral arm.
E) map the location of dense neutral hydrogen clouds.
فتح الحزمة
افتح القفل للوصول البطاقات البالغ عددها 54 في هذه المجموعة.
فتح الحزمة
k this deck
33
How does the traditional monolithic collapse theory of the formation of the galaxy explain the origin of globular clusters?

A) They formed in the disk and later were ejected to the halo.
B) They formed in other galaxies and were captured by close interactions.
C) They build over time from the collision of stars in the halo.
D) They formed early on during the free-fall collapse of the proto-galactic material.
فتح الحزمة
افتح القفل للوصول البطاقات البالغ عددها 54 في هذه المجموعة.
فتح الحزمة
k this deck
34
A several million solar mass ____ is thought to be at the center of our galaxy.

A) spiral arm
B) globular cluster
C) planet
D) black hole
فتح الحزمة
افتح القفل للوصول البطاقات البالغ عددها 54 في هذه المجموعة.
فتح الحزمة
k this deck
35
The energy source at the center of our galaxy is called

A) Cygnus X-1.
B) the Orion arm.
C) the sun.
D) Sagittarius A*.
فتح الحزمة
افتح القفل للوصول البطاقات البالغ عددها 54 في هذه المجموعة.
فتح الحزمة
k this deck
36
Our Milky Way Galaxy is about...

A) 1 light year across
B) 10 light years across
C) 100 light years across
D) 1000 light years across
E) 100,000 light years across
فتح الحزمة
افتح القفل للوصول البطاقات البالغ عددها 54 في هذه المجموعة.
فتح الحزمة
k this deck
37
This is a "thought" question.Why are few galaxies outside our own galaxy seen in the circle around the sky where the Milky Way is located? This is because ...

A) there aren't any galaxies in those directions
B) dust in the Milky Way blots out our view of galaxies in those directions
C) the missing mass is in those directions
D) the Big Bang has blown galaxies away from those directions
فتح الحزمة
افتح القفل للوصول البطاقات البالغ عددها 54 في هذه المجموعة.
فتح الحزمة
k this deck
38
CO observations of the galaxy reveal

A) the location of dense neutral hydrogen clouds.
B) the location of population II stars.
C) the location of population I stars.
D) the location of the galactic corona.
E) the location of giant molecular clouds.
فتح الحزمة
افتح القفل للوصول البطاقات البالغ عددها 54 في هذه المجموعة.
فتح الحزمة
k this deck
39
The disk of the Milky Way is approximately 20,000 ly in diameter.
فتح الحزمة
افتح القفل للوصول البطاقات البالغ عددها 54 في هذه المجموعة.
فتح الحزمة
k this deck
40
If a star with a peculiar space motion with respect a typical disk star is found what other property would you expect it to have?

A) Low luminosity.
B) Poor metal content compared to the Sun.
C) Old age.
D) All of the above.
فتح الحزمة
افتح القفل للوصول البطاقات البالغ عددها 54 في هذه المجموعة.
فتح الحزمة
k this deck
41
The rotation curve of the galaxy provides evidence for the existence of the ____________________ which extends beyond the halo of the galaxy.
فتح الحزمة
افتح القفل للوصول البطاقات البالغ عددها 54 في هذه المجموعة.
فتح الحزمة
k this deck
42
____________________ are groups of 100,000 to 1,000,000 population II stars firmly bound by gravity.
فتح الحزمة
افتح القفل للوصول البطاقات البالغ عددها 54 في هذه المجموعة.
فتح الحزمة
k this deck
43
Population II stars contain more metals than Population I stars.
فتح الحزمة
افتح القفل للوصول البطاقات البالغ عددها 54 في هذه المجموعة.
فتح الحزمة
k this deck
44
The orbits of halo stars are typically circular and have a low inclination with respect to the disk.
فتح الحزمة
افتح القفل للوصول البطاقات البالغ عددها 54 في هذه المجموعة.
فتح الحزمة
k this deck
45
The ____________________ of the galaxy contains population I stars,open clusters,and gas clouds.
فتح الحزمة
افتح القفل للوصول البطاقات البالغ عددها 54 في هذه المجموعة.
فتح الحزمة
k this deck
46
Globular clusters are primarily found in the ____________________ component of the Galaxy.
فتح الحزمة
افتح القفل للوصول البطاقات البالغ عددها 54 في هذه المجموعة.
فتح الحزمة
k this deck
47
Henrietta Leavitt discovered the period-luminosity relationship for ____________________.
فتح الحزمة
افتح القفل للوصول البطاقات البالغ عددها 54 في هذه المجموعة.
فتح الحزمة
k this deck
48
Spiral tracers tend to be old,luminous stars.
فتح الحزمة
افتح القفل للوصول البطاقات البالغ عددها 54 في هذه المجموعة.
فتح الحزمة
k this deck
49
The center of our galaxy shows signs of past eruptions.
فتح الحزمة
افتح القفل للوصول البطاقات البالغ عددها 54 في هذه المجموعة.
فتح الحزمة
k this deck
50
The density wave theory explains spurs and branches along the spiral arms.
فتح الحزمة
افتح القفل للوصول البطاقات البالغ عددها 54 في هذه المجموعة.
فتح الحزمة
k this deck
51
Giant molecular cloud complexes are located in spiral arms.
فتح الحزمة
افتح القفل للوصول البطاقات البالغ عددها 54 في هذه المجموعة.
فتح الحزمة
k this deck
52
The rapid rotation in the outer disk suggests that our galaxy is more massive than previously thought.
فتح الحزمة
افتح القفل للوصول البطاقات البالغ عددها 54 في هذه المجموعة.
فتح الحزمة
k this deck
53
Old stars are poor in heavy atoms because there were no previous generations of stars.
فتح الحزمة
افتح القفل للوصول البطاقات البالغ عددها 54 في هذه المجموعة.
فتح الحزمة
k this deck
54
The disk of the galaxy is older than the halo.
فتح الحزمة
افتح القفل للوصول البطاقات البالغ عددها 54 في هذه المجموعة.
فتح الحزمة
k this deck
locked card icon
فتح الحزمة
افتح القفل للوصول البطاقات البالغ عددها 54 في هذه المجموعة.