Astronomy 102, Midterm Exam #3
Thursday December 11, 2003
2.00 pm Ð 3.15 pm
Do not turn the pages of the exam
until you are instructed to do so.
You are responsible for reading the following
rules carefully before beginning.
Exam
rules: You may use only a writing instrument and a calculator while taking
this test. You may not consult
any computers, books, notes Ð neither on paper nor stored in a calculator Ð nor
each other. All of your work must
be written on the attached pages, using the reverse sides if necessary. Important equations, numbers and
conversion factors, used in the problems, are found in the last pages of the
exam, in the form of the Useful Equations sheet and the How Big Is That sheet. The final answers must be indicated
clearly. Exams are due at 3.15 pm.
The
questions are each worth five (5) points.
Partial credit is available
for those questions involving essays, short answers, drawings or explicit
calculations, and for multiple-choice questions indicated possibly to have more
than one correct answer (e.g. Òcheck all answers that applyÓ).
Note:
select only one answer for each question, except if the problem
explicitly indicates to Òcheck all that applyÒ.
Name: ___________________________________
ID number:
_______________________________
Recitation:
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1. A quasar is observed to have a spectral redshift corresponding to a speed of 8.6 x 108 cm/s. How far away is the quasar?
c 4.3 x 1013 ly.
c 4.3 x 108 ly.
c 4.3 x 103 ly.
c 4.3 x 106 ly.
c None of the above.
2. You measure a galaxy as being 4.9 x 108 ly away. What redshift (in terms of its velocity) will the galaxy's spectrum display?
c 9.8 x 108 cm/s.
c 9.8 x 106 cm/s.
c 9.8 x 1014 cm/s.
c 9.8 x 103 cm/s.
c None of the above.
3. This would be good ways to generate strong gravitational radiation (check all that apply):
c Sudden merger of two large black holes.
c Produce a large amount of exotic matter near a black holeÕs horizon.
c Cause a black hole to rotate at a large, constant rate.
c Move a black hole through space at a constant speed close to that of light.
c None of above.
4. Suppose we were to find that our previous measurements of the Hubble constant are wrong, and that the true value is 2 times the old value. In this case, our estimate of the age of the Universe would change to a value
c 0.2 times the previously-accepted age.
c 0.5 times the previously-accepted age.
c 2 times the previously-accepted age.
c 5 times the previously-accepted age.
5. In one incarnation of Star Trek, a Federation-run space station guards one end of a wormhole that connects two opposite quadrants of the Milky Way Galaxy. Using the wormhole, one can travel a distance equal to 0.45 times the diameter of the Galaxy and back in 98 minutes according to a clock on the space station. By what factor shorter is the apparent time of traveling through the wormhole compared to traveling without it according to the space station?
c 1.4 x 107
c 4.1 x 108
c 8.2 x 108
c 4.9 x 1010
6. HubbleÕs Law expresses the observed fact that:
c All distant galaxies are receding from us at speeds approaching the speed of light.
c All distant galaxies are approaching us at speeds proportional to their distance from us.
c All distant galaxies are approaching us at speeds approaching the speed of light.
c All distant galaxies are receding at speeds proportional to their distance from us.
c None of above.
7. Consider our discussion about
vacuum fluctuations, Hawking radiation, and exotic matter, and indicate which
of following statements are true (check all that apply):
c
It is possible, though
extremely unlikely, for black holes to emit television sets and leather-bound
copies of the works of Proust, via Hawking radiation.
c
Because virtual electrons and
virtual positrons are made in equal numbers by vacuum fluctuations, black holes
emit electrons and positrons equally.
c
According to the uncertainty
principle, a virtual particle-antiparticle pair can be generated out of
nothing, for a brief time.
c
It is possible for one member
of a virtual pair to be swallowed by a black hole while the other member
escapes.
c
Hawking radiation by the
black holes in active galaxy nuclei explains the large luminosities seen in
these objects.
8. The following statements describe exotic matter (check all that apply):
c Exotic matter has a negative mass.
c A stable wormhole must contain exotic matter.
c Vacuum fluctuations in strongly warped space-time are exotic.
c All antimatter is exotic.
c Exotic matter and regular matter annihilate each other when placed in contact.
9. Which of the following are examples of exotic matter (check all that apply):
c Vacuum fluctuations far from any source of gravity.
c Vacuum fluctuations near the surface of a white dwarf.
c Vacuum fluctuations near the surface of a neutron star
c Vacuum fluctuations near the decoupling surface of the Big Bang.
c None of above.
10. Consider our discussion of the temperature
and entropy of a black hole, and indicate which of following statements are
true (check all that apply):
c
The laws of thermodynamics do
not permit black holes to have positive entropy.
c
The temperature of the earth
is equal to absolute zero.
c
The entropy of the earth is
greater than zero.
c
A black hole must have large
entropy, or it would represent a violation of the second law of thermodynamics.
c
The temperature of a black
hole is less than absolute zero.
11. A certain galaxy is seen to be receding from us at a speed 10% of the speed of light. Its distance from us is approximately
c 0.15 light years.
c 15 light years.
c 1500 light years.
c 15 million light years.
c 1500 million light years.
12. Consider the apparent and absolute
horizons of black holes and indicate which of the following statements are true
(check all that apply):
c
A photon emitted from the
core of a collapsing star at the moment the absolute horizon is formed would
forever remain on the surface of the horizon.
c
A photon emitted from within
the absolute horizon of a collapsing star would be able to escape, if the star
could stop collapsing.
c
The absolute horizon grows
from a point to a final size of the Schwarzschild Singularity.
c
The absolute horizon is never
larger than the apparent horizon.
c
A star in the process of
collapsing has two horizons, one inside the other.
13. Consider what we discussed about wormholes
and time machines and indicate which of following statements are true (check
all that apply):
c
If wormhole time machines are
indeed stable, paradoxical situations such as the matricide paradox are allowed
to happen.
c
A wormhole can be created by
two black holes that overlap in hyperspace and are in the 'black hole'
(collapsing) configuration.
c
Wormhole time machines are
particularly stable and long-lived forms of wormholes.
c
A time machine can be created
by moving one of a wormhole's 'openings' through space at relativistic speeds
with respect to the other one.
c
In physical space, a wormhole
appears as a cylindrical tunnel connecting widely separated locations.
14. Wormhole time machines may not be possible because (check all
that apply)
c Cosmic censorship: the singularities they require may always be surrounded by event horizons.
c Circulation and build-up of vacuum fluctuations at the mouths of the wormhole, which causes one or the other of the wormholeÕs component singularities to evaporate.
c The matricide paradox; a time machine would allow one to travel backward in time, kill oneÕs mother, preventing oneÕs own birth, and thereby prevent one from travelling back in time. This is paradoxical, and is forbidden by known laws of physics.
c Circulation and build-up of light within the wormhole, which leads very quickly to an extremely large energy, the gravity of which causes the wormhole to collapse.
c None of above.
15. Consider the effects of exotic matter on
space-time in the vicinity of a black hole and indicate which of the following
statements are true (check all that apply):
c
Vacuum fluctuations near a
black hole horizon can lead to the evaporation of the black hole.
c
A black hole deflects light
less if it has exotic matter around it than if it does not.
c
Since mass can never be
negative, and since mass is equivalent to energy, there is no such thing as
matter with negative energy density.
c
Suppose it were possible for
a star to be made up completely of exotic matter. No planets could orbit this star.
c
A wormhole can exist longer
if exotic matter is added to it.
16. Consider Hubble's law and cosmological expansion of the Universe and detemine which of the following statements are (check all that apply):
c The expansion of the universe is isotropic: galaxies seem to recede according to Hubble's law, no matter which direction you look.
c There is one spot in the universe from which all galaxies appear to be receding, which is the center of the universe, from which the big bang started.
c There is no observational evidence for cosmological homogeneity.
c As the universe expands, material is continually created to occupy the additional volume.
c The cosmological expansion of the universe is an expansion of spacetime itself, which carries objects along with it. In a sense, then, the galaxies we observe to be receding are really at rest with respect to the space-time, which is dragging them along.
17. Consider the big bang and the current state of the Universe and detemine which of the following statements are true (check all that apply):
c The Big Bang is a gravitational singularity, and according to cosmic censorship all such singularities are surrounded by an event horizon. Thus, if Cosmic Censorship is true, our own Universe could appear as a black hole in another, larger Universe.
c The best estimates, from observations of galaxy motion and of small anisotropies in the cosmic background, indicate that the Universe is open.
c The wavelengths of light at which the early universe is brightest have been Doppler shifted into the microwave range.
c The Universe is apparently flat, and thus marginal: the observed expansion will slow down and stop.
c The decoupling surface is the earliest part of the universe's life that we can observe, using light.
18. The lifetime of a black hole (the time it takes it to evaporate by emission of Hawking radiation) with a mass of 2 Msun is
c Extremely short, which is why very few of them are observed.
c Slightly shorter than the present age of the Universe.
c Longer than the present age of the Universe, but much shorter than the lifetimes of the longest-lived stars.
c Longer than the present age of the Universe, but about the same as the lifetimes of 2 Msun stars.
c A great deal longer than the age of the Universe or the lifetimes of stars.
19. The age of the Universe is approximately
c 1.6«108 years.
c 1.6«109 years.
c 1.6«1010 years.
c Infinity (it has no known beginning).
c None of above.
20. The radius of the observable Universe is approximately
c 1.6«108 light years.
c 1.6«109 light years.
c 1.6«1010 light years.
c Infinity (it has no known limits).
c None of above.
21. Four distant galaxies are seen by their Doppler-shifted spectra to be receding from us at a speeds 1218 km s-1, 2436 km s-1, 3654 km s-1, and 4872 km s-1. The distances to these galaxies have a ratio of
c 1:0.93:0.6:0.3
c 1:1.5:2.0:2.5
c 1:2:3:4
c 1:4:9:16
c 1:10:100:1000
22. Inflationary models of the early Universe were motivated primarily by the following observational result(s) (check all that apply):
c The very long wavelengths at which the Cosmic Microwave Background is observed.
c The extreme smoothness of the Cosmic Microwave Background.
c The extremely large luminosity represented by the Cosmic Microwave Background.
c The high-velocity recession of stars and planets from the Cosmic Microwave Background.
c None of above.
23. A brick, illustrated below, encounters a strong gravity wave, traveling from left to right. Draw a sequence of sketches, indicating the changes in the brickÕs appearance as one cycle of the gravity wave passes.
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24. From our viewpoint in the Milky Way, the Universe appears to be expanding at the same speed for a given distance away, no matter which direction we look; in other words, it appears as if we are at the center of the expansion. From another, distant galaxy, the Universe would appear to
c Expand from a center in the vicinity of the Milky Way Galaxy.
c Expand from a center located at that galaxy.
c Expand from a center halfway between that galaxy and the Milky Way.
c All of above.
c None of above.
25. The following is experimental support for the Big Bang:
c The detection of the Cosmic Microwave Background, by Penzias and Wilson.
c The finding by Ryle et al. that the number of galaxies per unit volume in the Universe was larger in the past than in the present.
c The discovery by Hubble that the Universe expands.
c All of the above
c None of above.
26. A distant galaxy is seen by its Doppler-shifted spectrum to be
receding from us at a speed V, which is
small compared to the speed of light.
Another galaxy, twice as far away as the first, is seen. What is its recession speed?
c V/2.
c V.
c 2V.
c 4V.
c None of above.
27. In observations of a certain galaxy, a spectral line that normally has wavelength of 0.5 x 10-4 cm appears instead at wavelength 0.55 x 10-4 cm. How far away is the galaxy, in millions of light years? (Show your work if you wish to qualify for partial credit.)
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28. The spectrum of the Large Magellanic Cloud, a galaxy visible from Earth's southern hemisphere, shows blue-shifted spectral lines. This means (check all that apply):
c That this galaxy recedes from us, as it should since the Universe is expanding.
c That this galaxy is extremely distant.
c That the black hole at the center of the Milky Way is tremendously more massive than this galaxy, resulting in its light suffering a gravitational blueshift on its way to us.
c That this galaxy is nearby and has substantial motion in response to its attraction to the Milky Way and other neighboring objects, in addition to its motion from the expansion of the Universe.
c None of above.
29. Suppose opacity within decoupling surfaces werenÕt a problem; would it then be possible in principle for us to see the Big Bang singularity? (Check all that apply)
c Yes, because the non-infinite speed of light allows us to look into the past, all the way to the beginning of time, just by looking far enough away.
c No, because the singularityÕs event horizon gets in the way.
c Yes, because the large abundance in space of primordial wormhole time machines allows light emitted by the singularity 1010 years ago to reach us in the present time.
c No, because it would require detection of light or other particles that arrived from the future.
c None of above.
30. At what time after the Big Bang did electrons decouple?
c 10-35 s.
c 1 s.
c 200 s.
c 2 x 105 s.
c None of above.
31. Einstein originally proposed that the cosmological constant be added to the equations of the general theory of relativity, in order that (check all that apply):
c Isotropic and homogeneous solutions of these equations could be produced.
c Expanding or contracting solutions of these equations could be produced.
c Static solutions of the equations, involving no singularities, could be produced.
c The singularities evident in his first solutions of the equations could not be realized in nature.
c His mathematical error in the original form of general relativity would be corrected.
32. The Cosmic Microwave Background has long wavelengths because (check all that apply):
c It was emitted so far away from us, the Universe is expanding, and thus the light is extremely redshifted.
c It was emitted from near the event horizon surrounding the Big Bang singularity, and suffers an extreme gravitational redshift.
c It was emitted after the Universe had expanded and cooled to a temperature of 2.7 degrees above absolute zero, far too cold to emit visible light.
c It was emitted from behind the decoupling surface, and the Universe was so opaque then that only the longest-wavelength light gets through.
c None of above.
33. The Cosmic Microwave Background is virtually isotropic because
c It is emitted from the new matter that is constantly being produced out of nothingness to give the Universe its steady-state appearance; this new matter is uniformly distributed in space.
c It is emitted from spacetime points fairly close to the Big Bang singularity, and since all light paths terminate in the singularity we see the Background in whatever direction we look.
c Its wavelengths are actually larger than the Universe, and thus its energy is uniformly distributed throughout the Universe.
c All of above.
c None of above.
34. Why might a positivist argue that the study of black hole interiors and their singularities is not important? Check all that apply.
c It has been proven mathematically that the interiors of black holes are simple and completely understood; no further work is required.
c All of the entropy of the black hole is represented by the surface area of the horizon rather than its interior.
c The real world is not accessible to the senses, nor to extensions of our senses such as experimental instruments.
c Anything inside an event horizon is inaccessible to experiments from the outside; no experimental check can be made on the validity of theories of the interior.
c None of above.
35. Despite the argument above, why might a positivistic scientist be persuaded of the importance of studies of black hole interiors and singularities?
c Black holes can in principle combine to become wormholes, so that their interiors may in some sense become accessible to measurements.
c Cosmic censorship might not be universally true; naked singularities might therefore exist, accessible to measurements.
c The large-scale structure of the Universe resembles in many respects the interior of an event horizon, since the Universe itself originated in a singularity; the Universe is of course observable.
c All of above.
c None of above.
36. An era of extraordinarily rapid expansion early in the Universe's life, called the inflationary era, took place for the following reason:
c The huge amount of energy available in the form of heat, and the small number of elementary particles it was possible to make when the Universe was so hot, led to a runaway energy "cost" in the production of these particles.
c The evaporation of small black holes, produced early in the Big Bang, by Hawking radiation led to a burst of gamma rays, pushing the already-expanding contents of the Universe apart even faster.
c Vacuum fluctuations were exotic in the early Universe, and during the inflationary era the vacuum produced higher-mass vacuum fluctuations than it does now; the "antigravity" effects of these vacuum fluctuations accelerated the expansion of the non-exotic matter.
c All of above.
c None of above.
37. Assume we are living a matter-dominated Universe with a mass density that this much less than the critical density (A = 1). Based on the current value of the Hubble constant, what will the age of this Universe be?
c 1.5 x 1010 yr.
c 1.0 x 1010 yr.
c 1.3 x 1010 yr.
c 1.6 x 1010 yr.
38. Assume we are living a matter-dominated Universe with a mass density equal to the critical density (A = 2/3). Based on the current value of the Hubble constant, what will the age of this Universe be?
c 1.5 x 1010 yr.
c 1.0 x 1010 yr.
c 1.3 x 1010 yr.
c 1.6 x 1010 yr.
39. Describe the history of the Universe before the Big Bang occurred.
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40. Is the Universe open, marginal or closed? In a few sentences, choose one of these answers and defend it by citing experimental and theoretical results we have discussed this semester.
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Useful Equations
Length contraction, time dilation and velocity addition:

Minkowski absolute interval:
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Useful rearrangements of the Absolute Interval formula:

Mass-energy equivalence:
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Mass of a moving object:

Doppler shift:
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Schwarzschild circumference:
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Circumference of a spherical object of diameter d:
C = p d
HubbleÕs Law:
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Age of a matter-dominated
universe:
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How big is that?
|
Diameter of hydrogen atom |
1.06 « 10-8 cm |
|
Diameter of the Moon |
3.5 « 103 km |
|
Diameter of the Earth |
1.3 « 104 km |
|
Diameter of the Sun |
1.4 « 106 km |
|
Diameter of the Milky Way galaxy |
1.7 « 105 ly |
|
|
|
|
Distance to the Moon |
3.8 « 105 km |
|
Distance to the Sun |
1.5 « 108 km |
|
Distance to the next nearest star |
4 ly |
|
Distance to the center of the Milky Way |
2.7 « 104 ly |
|
Distance to the nearest galaxy |
1.7 « 105 ly |
|
|
|
|
Mass of hydrogen atom |
1.67 « 10-24 gm |
|
Mass of the Moon |
7.4 « 1025 gm |
|
Mass of the Earth |
6.0 « 1027 gm |
|
Mass of the Sun |
2.0 « 1033 gm (1 Msun) |
|
Mass of the Milky Way galaxy |
5 « 1010 MO |
|
|
|
|
Luminosity of the Sun |
3.8 « 1033 erg/s (1 Lsun) |
|
Luminosity of the largest stars |
105 LO |
|
Luminosity of the Milky Way galaxy |
1010 LO |
|
Luminosity of quasar 3C 273 |
1012 LO |
|
|
|
|
EarthÕs rotation period |
8.64 « 104 s (1 day) |
|
MoonÕs revolution period |
28 days |
|
EarthÕs revolution period |
365.25 days (1 year) |
|
SunÕs revolution period within Milky Way |
2.4 « 108 years |
|
Age of the solar system |
4.6 « 109 years |
|
Expected life span of the Sun |
1.5 « 1010 years |
|
Age of the Universe |
1.6 « 1010 years |
|
|
|
|
EarthÕs equator rotation speed |
0.47 km/s |
|
EarthÕs revolution speed |
30 km/s |
|
SunÕs speed within the Milky Way |
220 km/s |
|
Milky WayÕs speed within the local Universe |
500 km/s |
|
Typical lengths: |
|
|
Normal star diameter |
106 km |
|
Distance between stars |
a few ly |
|
Normal galaxy diameter |
105 ly |
|
Distance between galaxies |
106 ly |
|
|
|
|
Typical masses: |
|
|
Smallest star |
0.1 Msun |
|
Normal star |
1 Msun |
|
Giant star |
10 Msun |
|
Normal galaxy |
1010 - 1011 Msun |
|
Galaxy cluster |
1014 - 1015 Msun |
|
|
|
|
Typical luminosities: |
|
|
Normal star |
1 Lsun |
|
Giant star |
103 - 105 Lsun |
|
Normal galaxy |
109 - 1010 Lsun |
|
Quasar |
1012 - 1013 Lsun |
|
|
|
|
Typical time spans: |
|
|
Planetary revolution |
1 year |
|
Galaxy rotation |
107 - 109 years |
|
Life of giant stars |
106 - 109 years |
|
Life of normal star |
1010 years |
|
|
|
|
Typical speeds: |
|
|
Planetary orbits |
10 km/s |
|
Stellar motion in galaxy |
100 km/s |
|
Between nearby galaxies |
100 km/s |
|
|
|
|
Other important constants: |
|
|
1 ly = 9.46 « 1012 km = 9.46 « 1017 cm |
1 Mly = 106 ly |
|
1 km = 105 cm |
1 erg = 1 gm cm2/s2 |
|
1 hour = 3600 seconds |
1 year = 3.16 « 107 seconds |
|
¹ = 3.14159265359 |
HubbleÕs constant: H0 = 20 km/(sec Mly) |
|
Speed of light: c = 2.99792458 « 105 km/s = 2.99792458 « 1010 cm/s = 1 ly/year |
NewtonÕs gravitational constant: G = 6.67 « 10-8 cm3/(gm s2) |
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