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It is possible for a galaxy to have an apparent velocity greater than the speed of light.This means that the galaxy


A) has an active nucleus capable of producing relativistic jets.
B) is approaching us and the measured speed is a mere artifact of projecting its velocity along the line of sight.
C) has been ejected at tremendous speed by the Big Bang.
D) is being temporarily accelerated by large numbers of simultaneous supernovae blasts.
E) is being carried by the expansion of the universe.

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If the Hubble constant were equal to 50 km/s/Mpc, what would the approximate age of the universe (the Hubble time) be, assuming that the expansion rate has stayed approximately constant over time? Note that 1 Mpc = 3.086 * 1019 km and 1 year = 3.154 * 107 s.

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The age of the universe would ...

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The COBE and WMAP satellites detected fluctuations in the CMB.On average, how big were these fluctuations, and what do they that tell us about the universe at a redshift of z = 1,000?

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After correcting for the Milky Way's mot...

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Explain how the figure below shows evidence supporting the Big Bang theory. Explain how the figure below shows evidence supporting the Big Bang theory.

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The Big Bang theory predicts that only c...

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If a scientist in the distant Andromeda Galaxy studies the hydrogen gas in that galaxy, they will measure ________ what a scientist in our galaxy would measure, studying hydrogen gas In the Milky Way.


A) a larger mass per atom than
B) a smaller mass per atom than
C) a different set of spectral lines than
D) different possible chemical bonds with other elements than
E) the same properties as

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Galaxy peculiar velocities are typically about 300 km/s.How far away do you have to look in order to see recessional velocities that are 10 times this peculiar velocity? Note that the Hubble constant has a value of 70 km/s/Mpc.


A) 12 Mpc
B) 25 Mly
C) 37 Mpc
D) 43 Mpc
E) 52 Mpc

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If you measured the distances and recessional velocities for a sample of galaxies and plotted the data to get the figure shown below, what value would you derive for the Hubble constant? If you measured the distances and recessional velocities for a sample of galaxies and plotted the data to get the figure shown below, what value would you derive for the Hubble constant?   A)  10 km/s/Mpc B)  50 km/s/Mpc C)  70 km/s/Mpc D)  100 km/s/Mpc E)  500 km/s/Mpc


A) 10 km/s/Mpc
B) 50 km/s/Mpc
C) 70 km/s/Mpc
D) 100 km/s/Mpc
E) 500 km/s/Mpc

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Why did Big Bang nucleosynthesis only produce elements less massive than beryllium?


A) The laws of physics do not allow the formation of massive nuclei outside stars.
B) The universe was never hot enough for nucleosynthesis by fusion before stars formed.
C) There was no black hole to provide sufficient energy for advanced nucleosynthesis.
D) The universe expanded and cooled rapidly.
E) More massive elements did form, but they decayed very rapidly into lighter ones.

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The apparent recessional velocities of galaxies at large distances are due mainly to


A) the actual motions of the galaxies through space.
B) the motion of our Sun around the galactic center.
C) a continuously increasing scaling factor of the universe.
D) the relativistic jets launched by supermassive black holes.
E) incorrect interpretation of spectra from galaxies.

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If the distance of a galaxy is 5 Mpc, what is its recessional velocity if the Hubble constant is 70 km/s/Mpc?


A) 70 km/s
B) 100 km/s
C) 350 km/s
D) 500 km/s
E) 700 km/s

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In the early 1960s, physicists Penzias and Wilson detected a persistent noise at a wavelength of about 1 mm in their radio telescope that came from all directions in the sky due to


A) synchrotron emission from the Crab Nebula.
B) emission from newly formed stars in the Orion Nebula.
C) cellphone usage.
D) photons left over from the Big Bang.
E) television and radio broadcasting.

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Briefly explain how an accurate determination of Hubble constant has improved our understanding of cosmology.

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With an accurate determination of the Hu...

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The existence of the cosmic background radiation tells us that the early universe was


A) much hotter than it is today.
B) much colder than it is today.
C) composed entirely of radiation at early times.
D) composed entirely of stars at early times.
E) about the same temperature as today but much more dense.

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Distant galaxies we can see today with a redshift of z Distant galaxies we can see today with a redshift of z   6 emitted their light when the universe was A)  5 times smaller than it is today. B)  6 times smaller than it is today. C)  7 times smaller than it is today. D)  8 times smaller than it is today. E)  the same size as it is today. 6 emitted their light when the universe was


A) 5 times smaller than it is today.
B) 6 times smaller than it is today.
C) 7 times smaller than it is today.
D) 8 times smaller than it is today.
E) the same size as it is today.

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The CMB is a snapshot of the radiation in the universe at a redshift of z The CMB is a snapshot of the radiation in the universe at a redshift of z   1,000 when the universe was about A)  1,000 times smaller than it is today. B)  10 times smaller than it is today. C)  2 times smaller than it is today. D)  the same size as it is today. E)  10 times larger than it is today. 1,000 when the universe was about


A) 1,000 times smaller than it is today.
B) 10 times smaller than it is today.
C) 2 times smaller than it is today.
D) the same size as it is today.
E) 10 times larger than it is today.

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The oldest photons we detect in the universe come from


A) distant quasars.
B) the first generations of stars.
C) the most distant galaxies.
D) the epoch of recombination.
E) the first supernovae.

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If the distance of a galaxy at a redshift z = 0.05 is 220 Mpc, how many years back into the past are we looking when we observe this galaxy?


A) 5 million years
B) 220 million years
C) 720 million years
D) 6 billion years
E) 10 billion years

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If we lived in a galaxy 1 billion light-years from our own, what would we see?


A) a universe 1 billion years younger than ours
B) a universe 1 billion years older than ours
C) much the same universe as we see here
D) a universe expanding at a slower rate than we see from Earth
E) a universe expanding at a faster rate than we see from Earth

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