Spiral Structure of Galaxies
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Questions and Answers

What is the primary reason why we do not observe the mass in the outer regions of galaxies in visible light?

  • It is obscured by the visible stellar systems.
  • It is too far away from the center of the galaxy.
  • It is not very luminous. (correct)
  • It is not in the plane of our Milky Way.
  • What would happen to the spiral arms of galaxies if they consisted of the same material?

  • They would wind up very tightly. (correct)
  • They would disappear over time.
  • They would remain straight and unwound.
  • They would change into elliptical galaxies.
  • Why do the orbital periods of stars in galactic disks vary?

  • Because of the age of the stars in the galaxy.
  • Because of the density of stars in the galaxy.
  • Because of the uniform rotation of the galaxy.
  • Because of the differential rotation of the galaxy. (correct)
  • What is the implication of not observing tightly wound spiral arms in galaxies?

    <p>Spiral structure is a transient phenomenon, or it is a wave phenomenon, or both.</p> Signup and view all the answers

    What is the name of the scientist who described the orbits of stars in self-gravitating stellar disks?

    <p>Per Olaf Lindblad</p> Signup and view all the answers

    What type of motion do stars in self-gravitating stellar disks exhibit?

    <p>Epicyclic motion</p> Signup and view all the answers

    What is the shape of the distribution of globular clusters in the galaxy according to Shapley's findings?

    <p>Spherical</p> Signup and view all the answers

    What was the significance of Shapley's discovery of the globular cluster distribution?

    <p>It showed we are not at the center of the universe</p> Signup and view all the answers

    What advantage did Shapley have over Kapteyn in determining the distribution of globular clusters?

    <p>He looked at objects located out of the plane of our galaxy</p> Signup and view all the answers

    What did Jan Oort measure to determine the dynamics of the galactic disk near the sun?

    <p>The Doppler shifts of the stars</p> Signup and view all the answers

    What was the model of the disk of our galaxy near the sun according to Jan Oort's research?

    <p>A circular shape with circular orbits</p> Signup and view all the answers

    What was the shape of the distribution of bright, giant stars observed by Jan Oort?

    <p>Flattened</p> Signup and view all the answers

    What is thought to be responsible for the strength and beauty of the spiral in the Whirlpool Galaxy, M51?

    <p>The passage of the companion galaxy</p> Signup and view all the answers

    What was the limitation of the computer simulation of the passage of the smaller galaxy past M51?

    <p>It was unable to reproduce the very prominent spiral structure in the inner regions of M51</p> Signup and view all the answers

    What is the purpose of using computer simulations in astronomy?

    <p>To test theoretical models of galaxy formation and evolution</p> Signup and view all the answers

    What is the predicted outcome of the passage of the companion galaxy by M51?

    <p>The exhibition of a very strong spiral structure in M51</p> Signup and view all the answers

    What is the main difficulty in using General Relativity to calculate the behavior of two very compact massive objects in close proximity?

    <p>The complexity of the calculations</p> Signup and view all the answers

    What is the focus of the discussion of General Relativity in this context?

    <p>The principle of equivalence and the definition of a straight line</p> Signup and view all the answers

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