Exam 25: Galaxies and Dark Matter: The Large-Scale Structure of the Cosmos

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How massive are the largest known galaxies?

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A radio galaxy whose lobes are swept back as if forming a tail.This probably indicates that:

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Describe how gravitational lensing works.What can it tell us about a quasar? What can it tell us about the galaxy that is doing the lensing? How is lensing valuable to the study of dark matter?

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Infall of ________ may explain the higher than expected star formation rates in galaxies.

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While our Milky Way's black hole is not massive enough to have once been quasar,it must have passed through its Seyfert phase by 3.5 billion years ago.Explain how we know this.

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What is the Great Wall?

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While we know of thousands of quasars,it is likely none of them still exist today.Explain.

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The ________ phenomenon is an extremely energetic event which apparently occurs in the nuclei of massive galaxies during an early stage of their evolution.

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Spiral galaxies are much more common in the centers of rich clusters than in the universe as a whole.

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A red supergiant is observed in a globular cluster in another galaxy (located 150,000 light years away).It is predicted,based on its mass and age of the star that it will supernova in about 10,000 years.When will this supernova be visible on Earth?

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The peak of the quasar epoch was:

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What is a galaxy's rotation curve? To which galaxies is it best applied,and what does it tell us about the distribution of dark matter?

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Voids contain about what percentage of the universe's mass?

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From studies of the masses of individual galaxies and the masses of clusters of galaxies,it is now apparent that up to ________ of the universe is composed of dark matter.

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The energy radiated from a typical quasar requires that its black hole accrete about:

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A galaxy is at a distance of one billion light years.Which of the following is true?

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Giant elliptical galaxies may be the result of ________ in the centers of rich clusters.

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For nearby spirals,their rotation curves help measure both light and dark matter.

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The type of radio galaxy that reveals its motion through the intergalactic medium is called a:

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Rotation curves for spiral galaxies show:

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