Question 1
On a Hertzsprung-Russell diagram, where on the main sequence would you find stars that have the greatest mass?Selected Answer: 
 
upper leftCorrect Answer: 
 
Response Feedback: Correct, O stars have the largest massQuestion 2
When we see a region of a planet that is not as heavily cratered as other regions, we conclude thatSelected Answer: 
 
the surface in the region is younger than the surface in more heavily cratered regions.Correct Answer: 
 
Response Feedback: Correct, the regions that have been reformed via vulcanism, erosion, etc most recently have fewer cratersQuestion 3
Hydrostatic equilibrium means that:Selected Answer: 
 
stars have a higher temperature and pressure in their centers to support the mass of their outer layersCorrect Answer: 
 stars have a higher temperature and pressure in their centers to support the mass of their outer layersResponse Feedback: Correct, the concept of hydrostatic equilibrium implies that a star must have a higher pressure in its center to support the weight of the outer layers.Question 4
Remembering that the Sun has a surface temperature of approximately 5,800 K, a main sequence A star like Vega will have a temperature of approximately:Selected Answer: 
 
3,000 KCorrect Answer: 
 10,000KResponse Feedback: Incorrect, an A star is slightly hotter than the Sun, a star at ~50,000K is an O star (the hottest stars) and all of the other choices are as cool or cooler than the Sun so would not fit an A star.Question 5
The core of the Sun isSelected Answer: 
 
much hotter and much denser than its surface.Correct Answer: 
 
Response Feedback: Correct, remember our discussion based upon the average density and the luminosity relationship with temperature and radiusQuestion 6
Type II supernovae occur in evolved O and B stars because they:Selected Answer: 
 
form white dwarf stars in binary systemsCorrect Answer: 
 can fuse elements heavier than helium and thus have large iron coresResponse Feedback: Incorrect, remember that iron has the highest binding energy of all elements and so a star cannot extract energy from fusing iron into heavier elements.Question 7
You observe a star cluster with a main-sequence turn-off point at spectral type G2 (the same spectral type as the Sun). What is the age of this star cluster?Selected Answer: 
 
10 billion years.Correct Answer: 
 
Response Feedback: Correct, stars like the Sun live 10 billion yearsQuestion 8
Compared to stars like the Sun, B stars like RigeL have:Selected Answer: 
 
lifetimes much shorter than the SunCorrect Answer: 
 lifetimes much shorter than the SunResponse Feedback: Correct, hot, luminous massive stars like Rigel burn through there fuel much more quickly and thus have lifetimes much shorter than the Sun.Question 9
What happens to the core of a star after it ejects a planetary nebula?Selected Answer: 
 
It becomes a white dwarf.Correct Answer: 
 
Response Feedback: Correct, this is the path stars like the Sun take in becoming white dwarfsQuestion 10
If we see a high mass Ostar in the Andromeda galaxy tonight, we know that:Selected Answer: 
 
it will have already gone (Type II) supernovaCorrect Answer: 
 it will have already gone (Type II) supernovaResponse Feedback: Correct, remember that an O star has lifetime of order 1 million years, and so even before the light from an O star reaches us from Andromeda (2 million light years away) the star has been born, evolved, and exploded as a Type II SN before any being in the MIlky Way can see it.Question 11
About how old is the Solar System?Selected Answer: 
 
5 trillion yearsCorrect Answer: 
 5 billion yearsQuestion 12
You observe two stars over the course of a year (or more) and find that both stars have measurable parallax angles. Star X has a parallax angle of 1 arc-second. Star Y has a parallax angle of 1/4 of an arc-second. How do the distances to the two stars compare?Selected Answer: 
 
star Y is 4 times further awayCorrect Answer: 
 star Y is 4 times further awayResponse Feedback: Correct, the parallax angle is equal to (distance)-1, so the more distant star has a smaller parallax, and if the parallax is 4 times smaller then it is 4 times further away.Question 13
How thick are Saturn's rings from top to bottom?Selected Answer: 
 
a few hundred kilometersCorrect Answer: 
 
Response Feedback: Incorrect, the rings are incredibly thinQuestion 14
We currently know of approximately how many exo-planets?Selected Answer: 
 
900Correct Answer: 
 900 Response Feedback: Correct, and increasing steadily.Question 15
What do asteroids and comets have in common?Selected Answer: 
 
Most are unchanged since their formation in the solar nebula.Correct Answer: 
 
Response Feedback: Correct, both are left over from the formation of the Solar SystemQuestion 16
Why does the fusion of hydrogen release energy to power the Sun and stars?Selected Answer: 
b. 
fusion combines 4 hydrogen atoms into one helium which has less mass than 4 protonsCorrect Answer: 
b. fusion combines 4 hydrogen atoms into one helium which has less mass than 4 protonsResponse Feedback: Correct, this mass difference powers the stars, think Einstein's equation E = m c2, the energy released is proportional to the mass difference.Question 17
Consider two stars, A and B, with the following apparent and absolute magnitudes:
m(A) = -2 (apparent magnitude)
M(A) = 10 (absolute magnitude)
m(B) = 3 (apparent magnitude)
M(B) = 5 (absolute magnitude)
which is more luminous?Selected Answer: 
b. 
A appears brighter, but B is actually brighterCorrect Answer: 
c. A appears brighter, but B is actually brighterResponse Feedback: Correct, A's apparent magnitude of -2 (a smaller number) means it appears brighter but B's absolute magnitude of 5 (versus 10 for A) means it is in intrinsically brighter.Question 18
Pluto is now classified as a dwarf planet because:Selected Answer: 
 
it is in the Kuiper beltCorrect Answer: 
 it is in the Kuiper beltResponse Feedback: Correct, Pluto has not "cleared" its orbit as it is surrounded by similar sized bodies.Question 19
A main sequence star's luminosity comes from:Selected Answer: 
a. 
fusion of hydrogen into helium in the coreCorrect Answer: 
c. fusion of hydrogen into helium in the coreResponse Feedback: Correct, the main sequence is when a star uses nuclear fusion reactions to convert hydrogen into helium in the core of the star.Question 20
The MK-spectral types OBAFGKM must represent a sequence of:Selected Answer: 
 
decreasing temperaturesCorrect Answer: 
 decreasing temperaturesResponse Feedback: Correct, the first letter of the spectral type is related to the effective surface temperature of the star. Not that (for example) M stars can have a variety of radii and hence luminosities (as L=T4R2), and that a supergiant has a larger mass than a giant or main sequence M star.Question 21
Why do asteroids and comets differ in composition?Selected Answer: 
 
Asteroids formed inside the frost line, while comets formed outside.Correct Answer: 
 
Response Feedback: Correct, asteroids formed where the pre-Solar nebula was too hot for ices to formQuestion 22
If the Sun were to suddenly expand to be 10 times its current size of ~0.0047 AU but keep the same mass, the Earth would:Selected Answer: 
 
stay in the same orbitCorrect Answer: 
 stay in the same orbitResponse Feedback: Correct, the force on the Earth would be unchanged since the mass of the Sun is unchanged, so the orbit would not change.
Note this would not be true if the Sun were to expand to be larger than the Earth's orbit of course.
Also note that orbital distances are defined from both object's centers, so while the Earth in some sense is "closer" to the Sun's surface, its distance from the Sun's center and hence its orbital distance is unchanged.Question 23
How do the planets near the Sun differ from those farther out?Selected Answer: 
 
The ones nearest the Sun are generally smallest.Correct Answer: 
 The ones nearest the Sun are generally smallest.Question 24
Incandescent light bulbs have a temperature of ~2700 K, this means that their light is emitted mostly:Selected Answer: 
 
at infrared wavelengthsCorrect Answer: 
 at infrared wavelengthsResponse Feedback: Correct, the cooler temperature (relative to the Sun) means that these bulbs emit most of their light at longer - infrared - wavelengths. This is why they are so inefficient.Question 25
A G2V star and a K2V star have the same:Selected Answer: 
 
none of the aboveCorrect Answer: 
 none of the aboveResponse Feedback: Correct, remember for main sequence stars the mass, radius, luminosity and temperature are all related (and all are lower as you get to later spectral types).Question 26
The Sun will most likely never become a nova or type Ia supernova because such events only happen to stars thatSelected Answer: 
 
are in close binary systemsCorrect Answer: 
 are in close binary systemsResponse Feedback: Correct, novae and type Ia supernovae occur in binary systems where one member is a white dwarf.Question 27
Which of the following is not a characteristic of the inner planets?Selected Answer: 
 
They all have substantial atmospheres.Correct Answer: 
 
Response Feedback: Correct, only Venus and Earth have significant atmospheresQuestion 28
Imagine a star which has the same luminosity as the Sun but which has a surface temperature that is twice that of the Sun. You would then expect that a planet identical to Earth orbiting at 1 AU from this star would:Selected Answer: 
 
be approximately the same temperature as the EarthCorrect Answer: 
 be approximately the same temperature as the EarthQuestion 29
On a Hertzsprung-Russell diagram, where would you find red giant stars?Selected Answer: 
 
upper rightCorrect Answer: 
 
Response Feedback: Correct, red giants are cool (to the right) and bright (toward the top)Question 30
Remembering that the surface temperature of the Sun is ~6000K, a red giant would have a temperature of:Selected Answer: 
 
3000 KCorrect Answer: 
 3000 KResponse Feedback: Correct, a red giant like Arcturus is ~1/2 the (surface) temperature of the SunQuestion 31
Type-II supernovae occur when:Selected Answer: 
d. 
a massive star collapses after running out of fuelCorrect Answer: 
c. a massive star collapses after running out of fuelResponse Feedback: Correct, a Type II supernova is when the core of a massive star collapses, releasing energy that explodes the rest of the starQuestion 32
After the collapse began were all parts of the Solar Nebula the same temperature, and if not which part was hottest?Selected Answer: 
 
Not all the same temperature, and the inner parts were the hottest.Correct Answer: 
 Not all the same temperature, and the inner parts were the hottest.Question 33
A constellation isSelected Answer: 
a. 
stars at varying distances in the same part of the skyCorrect Answer: 
a. stars at varying distances in the same part of the skyResponse Feedback: Correct, the stars in a constellation are not necessarily members of a single star cluster. stars in a single cluster are approximately the same age and distance.Question 34
A star like the Sun will:Selected Answer: 
a. 
become a white dwarfCorrect Answer: 
a. become a white dwarfResponse Feedback: Correct, after it uses all of its hydrogen fuel a star like the Sun will expand into a red giant, then eventually after running out of its core helium become a planetary nebula and then a white dwarfQuestion 35
Approximately how many Earth's fit inside the Sun:Selected Answer: 
b. 
1,000,000Correct Answer: 
a. 1,000,000Response Feedback: Correct, the volume of the Sun is ~1,000,000 times that of the Earth.Question 36
An M-star which is 1/1000th the luminosity of the Sun an 1/10th its mass should live approximatelySelected Answer: 
c. 
1 trillion yearsCorrect Answer: 
b. 1 trillion yearsResponse Feedback: Correct, since the amount of energy it puts out is 1/1000th that of the Sun but it has only 1/10th the fuel, it should last 100 times longer- since the Sun lives 10 billion years an M star should live 1 trillion years.Question 37
Your mass would be approximately ( ) times larger than it is here on Earth if you were on a 1 Solar mass white dwarf:Selected Answer: 
 
the sameCorrect Answer: 
 the sameResponse Feedback: Correct, your mass is always the same. Note that the weight increases as the gravitational force increases.Question 38
We can determine the age of a globular cluster by:Selected Answer: 
 
finding the spectral types of the most luminous main sequence stars.Correct Answer: 
 finding the spectral types of the most luminous main sequence stars.Response Feedback: Correct, the most massive/luminous main sequence stars left are the ones whose lifetime is less than the age of the cluster, so the cluster must be just older than that age.
All of the stars with lifetimes less than the age of the cluster will have evolved off the main sequence already.Question 39
What was the material out of which the Solar System formed primarily made of?Selected Answer: 
 
Mostly hydrogen and helium with a small amount of dust grainsCorrect Answer: 
 Mostly hydrogen and helium with a small amount of dust grainsResponse Feedback: Correct, the Universe is still mostly hydrogen and helium (from the Big Bang)Question 40
Open clusters contain approximately ( ) stars:Selected Answer: 
 
1,000Correct Answer: 
 1,000Response Feedback: Correct, open clusters typically contain fewer stars (1,000) than the globular clusters (~100,000-1,000,000) which formed early in the galaxies history.
Monday, December 30, 2013
PHYS 107 ASTRONOMY MIDTERM 2
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