Filters
Question type

Study Flashcards

Who first used RR Lyrae variable stars to determine distances in our Milky Way Galaxy?


A) Henrietta Leavitt
B) Edwin Hubble
C) John Glenn
D) Carl Sagan
E) Harlow Shapley

Correct Answer

verifed

verified

Pulsating variable stars are useful in determining


A) the mass of a star for which the distance is known.
B) the temperature of a star for which we know the luminosity.
C) the radius of the bulge of our galaxy.
D) the distance to globular clusters.
E) the mass of the Milky Way galaxy.

Correct Answer

verifed

verified

Describe the central 25 pc of our galaxy.

Correct Answer

Answered by ExamLex AI

Answered by ExamLex AI

The central 25 pc of our galaxy, the Mil...

View Answer

In the edge-on sketch of a spiral galaxy, pick the letter corresponding most nearly to the location of globular clusters. In the edge-on sketch of a spiral galaxy, pick the letter corresponding most nearly to the location of globular clusters.   A)  A B)  B C)  C D)  D


A) A
B) B
C) C
D) D

Correct Answer

verifed

verified

What is the difference between an open cluster, an association, and a globular cluster? In which components of the galaxy does each lie?

Correct Answer

Answered by ExamLex AI

Answered by ExamLex AI

Open clusters, also known as galactic cl...

View Answer

Spiral tracers tend to be old, luminous stars.

Correct Answer

verifed

verified

Figure 12-1 Figure 12-1   -Refer to Figure 12-1. A Type I Cepheid has been located in an open cluster. The period of the Cepheid variable is 30 days and the variables apparent visual magnitude, m, is 10. First, use 12-1 to estimate the absolute visual magnitude, M . Calculate the distance to this open cluster? Hint: d<sub>pc</sub> = 10<sup>(</sup><sup>m</sup><sup> - </sup><sup>M</sup><sup> + 5) /5 </sup> A)  100 pc B)  10,000 pc C)  20 pc D)  300 pc E)  2500 pc -Refer to Figure 12-1. A Type I Cepheid has been located in an open cluster. The period of the Cepheid variable is 30 days and the variables apparent visual magnitude, m, is 10. First, use 12-1 to estimate the absolute visual magnitude, M . Calculate the distance to this open cluster? Hint: dpc = 10(m - M + 5) /5


A) 100 pc
B) 10,000 pc
C) 20 pc
D) 300 pc
E) 2500 pc

Correct Answer

verifed

verified

Shapley found the distance to the center of the galaxy by studying the distance to open clusters.

Correct Answer

verifed

verified

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.

Correct Answer

verifed

verified

The rotation curve of the galaxy provides evidence for the existence of the ____________________ which extends beyond the halo of the galaxy.

Correct Answer

verifed

verified

____________________ are groups of 100,000 to 1,000,000 population II stars firmly bound by gravity.

Correct Answer

verifed

verified

Giant molecular cloud complexes are located in spiral arms.

Correct Answer

verifed

verified

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.

Correct Answer

verifed

verified

The traditional "top-down" hypothesis of the formation of our galaxy cannot explain


A) why not all globular clusters are the same age.
B) why the youngest globular clusters are in the outer halo.
C) why the oldest stars are metal poor but not completely metal free.
D) streams and rings of scattered stars in the halo.
E) all of the above.

Correct Answer

verifed

verified

Discuss how Harlow Shapley determined the structure of the Milky Way galaxy from his study of globular clusters.

Correct Answer

verifed

verified

Radio maps of our galaxy show spiral arms because


A) the arms have larger Doppler shifts.
B) the gas in the spiral arms is very hot.
C) the dust in spiral arms is denser.
D) the gas in spiral arms is denser.
E) the stars in the spiral arms emit most of their energy at radio wavelengths.

Correct Answer

verifed

verified

Old stars are poor in heavy elements because there were very few previous generations of stars before the old stars formed.

Correct Answer

verifed

verified

Why are all spiral tracers young?

Correct Answer

verifed

verified

In the diagram below, the approximate absolute magnitude of a Type II Cepheid with a period of 30 days is ____________________. In the diagram below, the approximate absolute magnitude of a Type II Cepheid with a period of 30 days is ____________________.

Correct Answer

verifed

verified

The center of our galaxy lies in the direction of (but far beyond) the stars in the constellation of


A) Ursa Minor.
B) Ursa Major.
C) Sagittarius.
D) Orion.
E) Monoceros.

Correct Answer

verifed

verified

Showing 41 - 60 of 79

Related Exams

Show Answer