Monday, December 30, 2013

PHYS 107 ASTRONOMY MIDTERM 2

  • Question 1

    3 out of 3 points
     On a Hertzsprung-Russell diagram, where on the main sequence would you find stars that have the greatest mass?
    Selected Answer:
    Correct 
     upper left
    Correct Answer:
    Correct 
    Response Feedback:
     Correct, O stars have the largest mass
  • Question 2

    3 out of 3 points
     When we see a region of a planet that is not as heavily cratered as other regions, we conclude that
    Selected Answer:
    Correct 
     the surface in the region is younger than the surface in more heavily cratered regions.
    Correct Answer:
    Correct 
    Response Feedback:
     Correct, the regions that have been reformed via vulcanism, erosion, etc most recently have fewer craters
  • Question 3

    3 out of 3 points
    Hydrostatic equilibrium means that:
    Selected Answer:
    Correct 
    stars have a higher temperature and pressure in their centers to support the mass of their outer layers
    Correct Answer:
    Correct stars have a higher temperature and pressure in their centers to support the mass of their outer layers
    Response 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

    0 out of 3 points
    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:
    Incorrect 
    3,000 K
    Correct Answer:
    Correct 10,000K
    Response 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

    3 out of 3 points
     The core of the Sun is
    Selected Answer:
    Correct 
     much hotter and much denser than its surface.
    Correct Answer:
    Correct 
    Response Feedback:
     Correct, remember our discussion based upon the average density and the luminosity relationship with temperature and radius
  • Question 6

    0 out of 3 points
    Type II supernovae occur in evolved O and B stars because they:
    Selected Answer:
    Incorrect 
    form white dwarf stars in binary systems
    Correct Answer:
    Correct can fuse elements heavier than helium and thus have large iron cores
    Response 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

    3 out of 3 points
    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:
    Correct 
    10 billion years.
    Correct Answer:
    Correct 
    Response Feedback:
    Correct, stars like the Sun live 10 billion years
  • Question 8

    3 out of 3 points
    Compared to stars like the Sun, B stars like RigeL have:
    Selected Answer:
    Correct 
    lifetimes much shorter than the Sun
    Correct Answer:
    Correct lifetimes much shorter than the Sun
    Response 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

    3 out of 3 points
     What happens to the core of a star after it ejects a planetary nebula?
    Selected Answer:
    Correct 
     It becomes a white dwarf.
    Correct Answer:
    Correct 
    Response Feedback:
     Correct, this is the path stars like the Sun take in becoming white dwarfs
  • Question 10

    3 out of 3 points
    If we see a high mass Ostar in the Andromeda galaxy tonight, we know that:
    Selected Answer:
    Correct 
    it will have already gone (Type II) supernova
    Correct Answer:
    Correct it will have already gone (Type II) supernova
    Response 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

    0 out of 3 points
    About how old is the Solar System?
    Selected Answer:
    Incorrect 
    5 trillion years
    Correct Answer:
    Correct 5 billion years
  • Question 12

    3 out of 3 points
    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:
    Correct 
    star Y is 4 times further away
    Correct Answer:
    Correct star Y is 4 times further away
    Response 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

    0 out of 3 points
     How thick are Saturn's rings from top to bottom?
    Selected Answer:
    Incorrect 
     a few hundred kilometers
    Correct Answer:
    Correct 
    Response Feedback:
     Incorrect, the rings are incredibly thin
  • Question 14

    3 out of 3 points
    We currently know of approximately how many exo-planets?
    Selected Answer:
    Correct 
    900 
    Correct Answer:
    Correct 900 
    Response Feedback:
    Correct, and increasing steadily.
  • Question 15

    3 out of 3 points
     What do asteroids and comets have in common?
    Selected Answer:
    Correct 
     Most are unchanged since their formation in the solar nebula.
    Correct Answer:
    Correct 
    Response Feedback:
     Correct, both are left over from the formation of the Solar System
  • Question 16

    3 out of 3 points
    Why does the fusion of hydrogen release energy to power the Sun and stars?
    Selected Answer:
    Correctb. 
    fusion combines 4 hydrogen atoms into one helium which has less mass than 4 protons
    Correct Answer:
    Correctb. fusion combines 4 hydrogen atoms into one helium which has less mass than 4 protons
    Response 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

    3 out of 3 points
    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:
    Correctb. 
    A appears brighter, but B is actually brighter
    Correct Answer:
    Correctc. A appears brighter, but B is actually brighter
    Response 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

    3 out of 3 points
    Pluto is now classified as a dwarf planet because:
    Selected Answer:
    Correct 
    it is in the Kuiper belt
    Correct Answer:
    Correct it is in the Kuiper belt
    Response Feedback:
    Correct, Pluto has not "cleared" its orbit as it is surrounded by similar sized bodies.
  • Question 19

    3 out of 3 points
    A main sequence star's luminosity comes from:
    Selected Answer:
    Correcta. 
    fusion of hydrogen into helium in the core
    Correct Answer:
    Correctc. fusion of hydrogen into helium in the core
    Response 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

    3 out of 3 points
    The MK-spectral types OBAFGKM must represent a sequence of:
    Selected Answer:
    Correct 
    decreasing temperatures
    Correct Answer:
    Correct decreasing temperatures
    Response 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

    3 out of 3 points
     Why do asteroids and comets differ in composition?
    Selected Answer:
    Correct 
     Asteroids formed inside the frost line, while comets formed outside.
    Correct Answer:
    Correct 
    Response Feedback:
     Correct, asteroids formed where the pre-Solar nebula was too hot for ices to form
  • Question 22

    3 out of 3 points
    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:
    Correct 
    stay in the same orbit
    Correct Answer:
    Correct stay in the same orbit
    Response 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

    3 out of 3 points
    How do the planets near the Sun differ from those farther out?
    Selected Answer:
    Correct 
    The ones nearest the Sun are generally smallest.
    Correct Answer:
    Correct The ones nearest the Sun are generally smallest.
  • Question 24

    3 out of 3 points
    Incandescent light bulbs have a temperature of ~2700 K, this means that their light is emitted mostly:
    Selected Answer:
    Correct 
    at infrared wavelengths
    Correct Answer:
    Correct at infrared wavelengths
    Response 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

    3 out of 3 points
    A G2V star and a K2V star have the same:
    Selected Answer:
    Correct 
    none of the above
    Correct Answer:
    Correct none of the above
    Response 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

    3 out of 3 points
    The Sun will most likely never become a nova or type Ia supernova because such events only happen to stars that
    Selected Answer:
    Correct 
    are in close binary systems
    Correct Answer:
    Correct are in close binary systems
    Response Feedback:
    Correct, novae and type Ia supernovae occur in binary systems where one member is a white dwarf.
  • Question 27

    3 out of 3 points
     Which of the following is not a characteristic of the inner planets?
    Selected Answer:
    Correct 
     They all have substantial atmospheres.
    Correct Answer:
    Correct 
    Response Feedback:
     Correct, only Venus and Earth have significant atmospheres
  • Question 28

    3 out of 3 points
    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:
    Correct 
    be approximately the same temperature as the Earth
    Correct Answer:
    Correct be approximately the same temperature as the Earth
  • Question 29

    3 out of 3 points
     On a Hertzsprung-Russell diagram, where would you find red giant stars?
    Selected Answer:
    Correct 
     upper right
    Correct Answer:
    Correct 
    Response Feedback:
     Correct, red giants are cool (to the right) and bright (toward the top)
  • Question 30

    3 out of 3 points
    Remembering that the surface temperature of the Sun is ~6000K, a red giant would have a temperature of:
    Selected Answer:
    Correct 
    3000 K
    Correct Answer:
    Correct 3000 K
    Response Feedback:
    Correct, a red giant like Arcturus is ~1/2 the (surface) temperature of the Sun
  • Question 31

    3 out of 3 points
    Type-II supernovae occur when:
    Selected Answer:
    Correctd. 
    a massive star collapses after running out of fuel
    Correct Answer:
    Correctc. a massive star collapses after running out of fuel
    Response Feedback:
    Correct, a Type II supernova is when the core of a massive star collapses, releasing energy that explodes the rest of the star
  • Question 32

    3 out of 3 points
    After the collapse began were all parts of the Solar Nebula the same temperature, and if not which part was hottest?
    Selected Answer:
    Correct 
    Not all the same temperature, and the inner parts were the hottest.
    Correct Answer:
    Correct Not all the same temperature, and the inner parts were the hottest.
  • Question 33

    3 out of 3 points
    A constellation is
    Selected Answer:
    Correcta. 
    stars at varying distances in the same part of the sky
    Correct Answer:
    Correcta. stars at varying distances in the same part of the sky
    Response 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

    3 out of 3 points
    A star like the Sun will:
    Selected Answer:
    Correcta. 
    become a white dwarf
    Correct Answer:
    Correcta. become a white dwarf
    Response 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 dwarf
  • Question 35

    3 out of 3 points
    Approximately how many Earth's fit inside the Sun:
    Selected Answer:
    Correctb. 
    1,000,000
    Correct Answer:
    Correcta. 1,000,000
    Response Feedback:
    Correct, the volume of the Sun is ~1,000,000 times that of the Earth.
  • Question 36

    3 out of 3 points
    An M-star which is 1/1000th the luminosity of the Sun an 1/10th its mass should live approximately
    Selected Answer:
    Correctc. 
    1 trillion years
    Correct Answer:
    Correctb. 1 trillion years
    Response 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

    3 out of 3 points
    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:
    Correct 
    the same
    Correct Answer:
    Correct the same
    Response Feedback:
    Correct, your mass is always the same.  Note that the weight increases as the gravitational force increases.
  • Question 38

    3 out of 3 points
    We can determine the age of a globular cluster by:
    Selected Answer:
    Correct 
    finding the spectral types of the most luminous main sequence stars.
    Correct Answer:
    Correct 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

    3 out of 3 points
    What was the material out of which the Solar System formed primarily made of?
    Selected Answer:
    Correct 
    Mostly hydrogen and helium with a small amount of dust grains
    Correct Answer:
    Correct Mostly hydrogen and helium with a small amount of dust grains
    Response Feedback:
    Correct, the Universe is still mostly hydrogen and helium (from the Big Bang)
  • Question 40

    3 out of 3 points
    Open clusters contain approximately ( ) stars:
    Selected Answer:
    Correct 
    1,000
    Correct Answer:
    Correct 1,000
    Response 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.

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