Exam 24: Galaxies: Building Blocks of the Universe

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The expansion of the universe means that stars in our Milky Way Galaxy are getting increasingly farther apart.

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Most of the galaxies in the Local Group are:

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Explain as exactly as possible the way in which the central engine of active galaxies and quasars actually works.Why is the orientation so important?

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Type I supernovae can be used to determine distances to galaxies much better than type II supernovae.

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The huge lobe radio galaxy at the center of the Virgo Supercluster is:

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Discuss the population,size,and types of galaxies we find in our Local Group.

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A supernova that occurred 30,000 years ago in a galaxy 100,000 light years away will be observed on Earth:

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M-87,the giant elliptical at the heart of the Virgo Supercluster,shows a(n)________ extending outward from its core,moving at relativistic velocities.

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Distinguish an Sa from an Sc galaxy.

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How did Hubble use the cosmological redshift to determine distance?

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What type of galaxy are the two Magellanic Clouds? How do we know this visually?

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How does the modern value of Hubble's constant compare to Hubble's original published value?

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What lines of evidence show that the Milky Way Galaxy is indeed a spiral galaxy?

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Quasars usually have their distances measured by what technique?

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Not only does the central engine of active galaxies and quasars require a black hole,but also ________ to provide the radiate energy.

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________ galaxies seem to represent a transition between quasars and similar active nuclei compared to more normal spirals.

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Within the boundaries of the constellations Coma and Virgo are found:

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Quasar's spectral lines are:

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The Magellanic Clouds are good examples of the ________ type of galaxy.

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If we are directly in the line of a jet coming out of the lobe galaxy's core,we see a:

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