REVIEW: Astronomy 106 Test 5
Multiple
Choice
Identify
the letter of the choice that best completes the statement or answers the
question.
____ 1. Why
do main sequence stars have different surface temeperatures?
|
a. |
Their chemical compositions differ. Hot stars have more hydrogen than cool
stars |
|
b. |
They have different masses - hot stars
are more massive than cool stars |
|
c. |
They have different masses - cool stars
are more massive than hot stars |
|
d. |
neutrino production is different in stars
with different temperatures |
|
e. |
It depends on their age - new stars are
cooler because the thermonuclear reaction is just starting |
____ 2. In
what region of the galaxy do new stars form?
|
a. |
in the halo |
|
b. |
in globular star clusters |
|
c. |
the the
galactic disk |
|
d. |
near the center of the galaxy |
|
e. |
in the corona |
____ 3. Why
are most stars found on the main sequence?
|
a. |
main sequence stars are cooler than stars
off the main sequence. |
|
b. |
main sequence stars are more plentiful
at this stage of cosmic evolution |
|
c. |
other evolutionary stages - protostar and giant - are very short compared to the main
sequence. |
|
d. |
main sequence stars are much brighter
than stars off the main sequence and are, therefore, easier to see |
|
e. |
most main sequence stars are in
hydrostatic equilibrium |
____ 4. From
what type of objects do stars form?
|
a. |
giant molecular clouds |
|
b. |
Extremely hot gases ejected from
supernovae |
|
c. |
cometary materials from interstellar space |
|
d. |
planetary collisions |
|
e. |
intergalactic shock waves |
____ 5. What
is nucleosynthesis?
|
a. |
energy generation through the breakup of
large nuclei |
|
b. |
process of turning neutral atoms into ions |
|
c. |
the process of exciting nuclei in the
ground state so that they are ready to emit radiation |
|
d. |
the process of fusing two smaller nuclei
together to make larger nuclei |
|
e. |
also known as fission |
____ 6. In
what stage of a star's life does it become a red giant?
|
a. |
in the beginning, at the protostar stage |
|
b. |
in the middle, when it is in hydrostatic
equilibrium |
|
c. |
after its outer shell drifts away as a
planetary nebula |
|
d. |
right before its surface drops below the
event horizon |
|
e. |
in the later stages, when it moves off the
main sequence. |
____ 7. What
property of a star determines whether it ultimately becomes a white dwarf,
neutron star, or black hole?
|
a. |
its temperature |
|
b. |
its location in the galaxy |
|
c. |
its diameter |
|
d. |
its mass |
|
e. |
its chemical composition |
____ 8. Who
discovered pulsars (rapidly rotating neutron stars) in 1967
|
a. |
Vera Ruben |
|
b. |
Jocelyn Bell |
|
c. |
Cecilia Payne |
|
d. |
Annie Jump Canon |
|
e. |
Edwin Hubble |
____ 9. What
is the Chandrasekhar Limit?
|
a. |
The smallest that a body can be and
still ignite thermonuclear fusion |
|
b. |
The greatest mass that a white dwarf can
have without imploding into a neutron star or black hole |
|
c. |
The maximum number of stars that can be
seen from the northern hemisphere with the naked eye. |
|
d. |
The greatest mass a neutron star can
have before it implodes into a black
hole |
|
e. |
The largest nuclei that can be
synthesized in the core of massive stars |
____ 10. What
prevents a white dwarf from collapsing?
|
a. |
degenerate neutron pressure |
|
b. |
hydrostatic equilibrium |
|
c. |
degenerate electron pressure |
|
d. |
degernerate proton pressure |
|
e. |
nucelosynthesis |
____ 11. Who
discovered the thermonuclear reaction known as the proton-proton chain?
|
a. |
Arthur Eddington |
|
b. |
Vera Ruben |
|
c. |
Jocelyn Bell |
|
d. |
Edwin Hubble |
|
e. |
Hans Bethe |
____ 12. What
is the approximae main sequence lifetime of a star with the mass
of the sun?
|
a. |
10,000 years |
|
b. |
1,000,000 years |
|
c. |
10,000,000,000 years |
|
d. |
100,000,000,000 years |
|
e. |
1,000,000,000 years |
____ 13. What
is the nuclear reaction which powers the sun?
|
a. |
fission |
|
b. |
fusion |
|
c. |
the proton-proton chain |
|
d. |
a
and b |
|
e. |
b
and c |
____ 14. Why
is a temperature of at least ten million degrees requried
to ignite a thermonuclear reaction?
|
a. |
to overcome the electromagnatic
repulsion between protons |
|
b. |
to overcome the electromagnetic
repulsion between electrons |
|
c. |
to overcome the gravitational repulsion
between charges |
|
d. |
to slow down the naturtal
attraction between protons and electrons |
|
e. |
to split larger nuclei into smaller
nuclei |
____ 15. When
light from a star passes close to the sun, the position of that star on the
celestial sphere appears
|
a. |
to be further from the sun than when the
sun is not present |
|
b. |
to be closer to the sun than when the
sun is not present |
|
c. |
to disappear |
|
d. |
to be in the same place as it is when
the sun is not present |
|
e. |
to be closer or further from the sun,
depending on the spectral class of the star |
____ 16. Einstein's
___________ principle states that an observer cannot distinguish between the
force exerted on her due to an acceleration and force exerted on her by a massive body
|
a. |
uniformity |
|
b. |
relativity |
|
c. |
cosmological |
|
d. |
plenitude |
|
e. |
equivalence |
____ 17. According
to general relativity, what is gravity?
|
a. |
a force field |
|
b. |
a curvature of space-time |
|
c. |
equivalent to dark matter |
|
d. |
the same as energy |
|
e. |
depends on the frame of reference |
____ 18. What
happens to time in a gavitational field?
|
a. |
Time flows at the same rate in all graviational fields |
|
b. |
Time speeds up in a gravitational field.
The stronger the field, the faster
time flows |
|
c. |
Time slows down in a gravitational
field. The stronger the field, the slower time flows. |
|
d. |
The stronger the gravitational field, the
more difficult it is to measure time |
|
e. |
none of the above |
____ 19. Why
are astronauts orbiting the Earth weightless?
|
a. |
They are beyond the reach of Earth's
gravitational field |
|
b. |
The gravitational fields of Earth, the moon
and the sun pull in equal and opposite directions and cancel each other out. |
|
c. |
The acceleration of the spacecraft
produces a force that is equal and opposite to the
Earth's gravitational field. |
|
d. |
The astronauts are following the
curvature of space around a massive body (the Earth) |
|
e. |
They are weightless relative to the
spacecraft but not relative to the Earth |
____ 20. What
was the first test of general relativity that was widely viewed as confirming
the theory?
|
a. |
The precise measurement of the speed of
light in 1919 |
|
b. |
The detonation of the first atomic bomb
in 1945 |
|
c. |
The determination that time runs slower
in a gravitational field by comparing the elapsed time recorded by two
synchronized clocks, one on the ground floor, and one on the fifth
floor. |
|
d. |
The discovery of intese
radiation from a black hole |
|
e. |
The distortion of the star pattern
around the sun during an eclipse in 1919 |
____ 21. 
The above drawing shows
the positions of 5 stars on the celestial sphere when the sun is passing
through. If the sun were not there
|
a. |
the stars would be farther apart |
|
b. |
the stars would be closer together |
|
c. |
the position of the stars would be
exactly the same |
|
d. |
some stars would be closer together,
some farther apart, and some would be in the same place |
|
e. |
their positions would be different, but
it would depend on their spectral classifications |
____ 22. What
does the equation E=mc2 mean?
|
a. |
the speed of light is always the same |
|
b. |
a gravitational field cannot be
distinguished from an acceleration |
|
c. |
energy and mass are the same thing |
|
d. |
time slows down in a gravitational field |
|
e. |
mass increases as its velocity increases |
____ 23. Which
of the following would feel no gravitational force?
|
a. |
An astronaut in a spaceship orbiting
Jupiter |
|
b. |
An astronaut in a spaceship drifting in
interstellar space |
|
c. |
An astronaut in a spaceship accelerating in interstellar
space |
|
d. |
All of the above |
|
e. |
Only A and B |
____ 24. Arrange
the three stellar remnants in according to their diameters, largest to
smallest
|
a. |
black hole, neutron star, white dwarf |
|
b. |
white dwarf, neutron star, black hole |
|
c. |
neutron star, black hole, white dwarf |
|
d. |
white dwarf, black hole, neutron star |
|
e. |
black
hole, white dwarf, neutron star |
____ 25. Where
are nuclei larger than iron (Fe) synthesized?
|
a. |
In the cores of stars 8 tmes the mass of the sun or more |
|
b. |
In the cores of stars between 8 and 25
times the mass of the sun |
|
c. |
In the cores of stars 8 times the mass
of the sun or less |
|
d. |
In supernovae explosions |
|
e. |
In the cores of stars at least 20 times
the mass of the sun |
____ 26. The
event horizon is
|
a. |
equal to the diameter of a star whose
escape velocity just exceeds the speed of light |
|
b. |
the initation
of thermonuclear fusion in the cores of large stars |
|
c. |
the point at which a star exhusts its nuclear fuel |
|
d. |
the point at which a white dwarf becomes
a neutron star |
|
e. |
the moment at which a supernova explodes |
____ 27. A
star with a mass 10 times that of the sun will finish its life cycle as
|
a. |
a white dwarf from its core and a
planetary nebula |
|
b. |
a black hole from its core and a
planetary nebula |
|
c. |
a neutron star from its core and and widely scattered debris from the supernova |
|
d. |
a black hole from its core and widely scatterd debris from the supernova |
|
e. |
a neutron star from its core and a
planetary nebula |
____ 28. A
star with a mass 5 times that of the sun will finish its life cycle as
|
a. |
a white dwarf from its core and a
planetary nebula |
|
b. |
a black hole from its core and a
planetary nebula |
|
c. |
a neutron star from its core and and widely scattered debris from the supernova |
|
d. |
a black hole from its core and widely scatterd debris from the supernova |
|
e. |
a neutron star from its core and a
planetary nebula |
____ 29. A
star with a mass 26 times that of the sun will finish its life cycle as
|
a. |
a white dwarf from its core and a
planetary nebula |
|
b. |
a black hole from its core and a
planetary nebula |
|
c. |
a neutron star from its core and and widely scattered debris from the supernova |
|
d. |
a black hole from its core and widely scatterd debris from the supernova |
|
e. |
a neutron star from its core and a
planetary nebula |
____ 30. An
astronaut on a
spaceship traveling at 90% the speed of light is headed for a planet circling
the star Sirius. The time required to reach Sirius
|
a. |
will be shorter for the astronaut than for
an observer on the Earth monitoring the flight . |
|
b. |
will be longer for the astronaut than for an
observer on the Earth monitoring the flight . |
|
c. |
will be the same for the astronaut as for an
observer on the Earth monitoring the flight. |
|
d. |
will depend on the technique used to make
the measurement. |
|
e. |
will appear to be shorter for the astronaut,
but will actually be the same as for an observer on the Earth monitoring the
flight . |