Exam 16: Galaxies

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Giant spirals are the largest galaxies in the Universe.

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How have elliptical and spiral galaxies developed differently through interactions with other galaxies?

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The velocity dispersion method can be used to find the _______________ of a galaxy.

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Hubble's Law is only effective in measuring the distance to nearby galaxies.

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The rotation curve of a galaxy is important in determining the galaxy's ____.

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At the longest look-back times, we see ____.

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A supermassive black hole in the center of a galaxy typically represents ____ of the galaxy's total mass.

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In general, ____.

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The structure of most galaxies is most apparent using near-infrared images that show the locations of ____.

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Because the Hubble constant has a value of 70 km/s/Mpc, a galaxy 50 Mpc away would have a recession velocity of _______________ km/s. (Round your answer to the nearest 1 km/s).

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When spiral nebulae were first discovered, astronomers quickly identified them as distant groupings of stars.

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Galactic _______________ describes the process of a large galaxy absorbing a smaller one.

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Spiral galaxies are mostly found ____.

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The Milky Way and other spiral galaxies ____.

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Because the Hubble constant equals 70 km/s/Mpc, a galaxy with a recession velocity of 4,900 km/s would be a distance of ____ Mpc from Earth.

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Gravitational _______________ can be used to detect dark matter.

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Compared to other spiral galaxies, the Milky Way is ____.

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The _______________ time is the amount of time it took light to travel from a celestial object to Earth.

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The range of diameters and luminosities displayed by elliptical galaxies is ____.

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Spiral and irregular galaxies have active star formation.

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