Honors Astronomy Sem 2 Final: Bodecker – Flashcards
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The light we see from the Sun comes from which layer?
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photosphere
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What natural barrier tries to prevent two protons from combining?
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electromagnetic repulsion
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Which is the weakest of the fundamental forces?
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the gravitational force
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When the chromosphere can be seen during a solar eclipse, what is its color?
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red
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How many planet Earths could fit inside the Sun?
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A million
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From where does most of the solar wind flow?
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coronal holes
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What is the net result of the proton-proton chain?
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4 hydrogens are fused into 1 helium, 2 neutrinos + energy
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In the proton-proton cycle, what fraction of the hydrogen's mass doesn't end up as helium?
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.007
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The density of the Sun is similar to which object?
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Jupiter
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What is the size of a typical granule or convection cell seen in the photosphere?
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1,000 km
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Why couldn't you stand on the Sun's surface?
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The Sun doesn't have a solid surface.
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By what mechanism does radiation reach the Sun's surface from its interior?
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Convection
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What is the meaning of the "solar constant"?
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the solar energy reaching Earth per unit area per unit time
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Which of the following is NOT a property of neutrinos?
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never interact with matter
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Why are scientists bothered by the small number of neutrinos they detect coming from the Sun?
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They are not detecting the number of neutrinos predicted by current theories.
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Which is the strongest of the fundamental forces?
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the force that binds atomic nuclei
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What is it about the Sun's corona that astronomers don't understand?
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The corona is much hotter than layers of the Sun that are closer to the solar interior.
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How would sunspots appear if you could magically remove them from the Sun?
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They would shine bright orange in color.
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The numbers of sunspots and their activity peak about every:
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eleven years
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The critical temperature to initiate the proton-proton cycle in the cores of stars is:
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10 million K
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Loops of glowing hydrogen seen hanging out over the solar limb during totality are:
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prominences
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The _______ Minimum was a period of solar inactivity between 1645 and 1715.
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Maunder
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The pattern of rising hot gas cells all over the photosphere is called:
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Granulation
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The ESA satellite which gave us our most accurate distances to stars is called:
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Hipparcos
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If two stars differ in brightness by 5 magnitudes, the light ratio received by us is ______ to 1.
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100✕
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In comparing first magnitude Deneb with second magnitude Polaris, we find that:
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Deneb appears 2.5✕ brighter to us than does Polaris
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What are the two most important intrinsic properties used to classify stars?
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Luminosity and surface temperature.
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If a star has a parallax of 0.05", then its distance in light years is about:
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66 light years
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If a star is found by spectroscopic observations to be about 500 parsecs distant, its parallax is:
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.002"
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Hipparcos observations have given us good data on stars out to about:
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200 parsecs
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About how many stars has Hipparcos given us accurate distance data on?
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a million, those with parallaxes of .005" or larger
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Which of the following spectral types is the hottest?
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G2
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While Sirius, the Dog Star, is type AO, a star just a step hotter than M0 is a related:
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K9
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The Hertzsprung-Russell Diagram plots ______ against the spectral type or temperature.
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luminosity or absolute magnitude
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Two stars which differ by 5 magnitudes in apparent brightness have the same parallax; thus, one star must be intrinsically ______ times as luminous as the other.
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a hundred
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Stellar masses are determined directly by observation of the orbits and periods of ______ stars.
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all types of bianary
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In what range of masses are most stars found?
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.1 to 20 solar masses
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Why are star clusters almost ideal "laboratories" for stellar studies?
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Stars in clusters have the same age, similar composition, and are at the same distance away.
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Perhaps the greatest of the Greek astronomers, _______ compiled the first catalog of stars, accurately measured their positions, and defined the basic system of stellar brightnesses.
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Hipparcos
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Which of the following spectral types is the hottest?
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O9
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Which of these pairs of spectral types is most similar in temperature?
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K9 and M0
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What physical property of a star does the spectral type measure?
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temperature
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The star's color index is a quick way of determining its:
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temperature
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Which of the following is the most common type of star?
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main sequence
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Which of the following apparent magnitudes is the brightest?
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-1.1
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What is the absolute magnitude of our Sun?
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+4.8
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What is the single most important characteristic in determining the course of a star's evolution?
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mass
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The absolute magnitude of a star is its brightness as seen from a distance of:
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1o parsecs
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Which statement about stellar motion is incorrect?
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proper motion is measured over intervals of exactly six months
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If the radial velocity were -3 km/sec, and the transverse velocity were +4 km/sec, then:
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the space velocity would be 5 km/sec.
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What characteristic of the stars in a binary system can be determined by knowing the period of the stars' common orbit and the distance between them?
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mass
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Which type of binary can have their sizes measured directly by photometry?
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eclipsing
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Upon what data do measurements of sizes of eclipsing binaries depend?
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their Doppler shifts and the duration of stages of the eclipse
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The HR diagram can be a plot of _________.
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absolute magnitude versus color index
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What is the typical main sequence lifetime of a B-type star?
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20 million years
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What is the typical main sequence lifetime of a G-type star?
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10 billion years
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What is the typical main sequence lifetime of a M-type star?
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a trillion years
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A nearby star has a parallax of 0.2 arc seconds. What is its distance?
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5 pc
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Procyon lies about 13 light years distant, thus its parallax is about:
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0.25"
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In the H-R diagram, the bright blue-white stars that dominate the naked eye sky lie to the:
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upper left quadrant
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On the H-R diagram, the Sun lies:
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about the middle of the main sequence
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On the H-R diagram, white dwarfs lie Sirius B and Procyon B lie:
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to the lower left
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On the H-R diagram, red supergiants like Betelguese lie:
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the top right
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______ have masses like that of the Sun, and radii like that of the Earth.
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white dwarfs
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What is proper motion?
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It is the annual apparent motion of a star across the sky.
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In order to turn a star's proper motion into its space velocity, we must also know:
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its distance and radial velocity
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Which of the following best describes the size and distance relationship of our Sun and the nearest star?
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Two golfballs separated by 100 kilometers.
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Compared to the size of the Sun, in what range of sizes are most stars found?
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0.01 to 100 solar radii
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How might the most common occurring stars be described, based on our stellar neighborhood?
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M-type main sequence stars
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What are the characteristics of an open cluster of stars?
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a few hundred, mainly main sequence stars
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What are the characteristics of globular cluster stars?
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old age and hundreds of thousands of stars
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What makes the subject of star formation so difficult and complex?
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Stars live too long to be observed from birth to death.
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A typical protostar may be several thousand times more luminous than the Sun. What is the source of this energy?
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From the release of gravitational energy as the protostar continues to shrink.
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Which of these is not typical of a condensing protostar?
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fusion of helium into carbon in their cores
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What is the critical temperature at which hydrogen can fuse into helium in the star's core?
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10 million K.
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What happens when an interstellar cloud fragment shrinks?
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all
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What is characteristic of a main sequence star?
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The rate of nuclear energy generated in the core equals the rate radiated from the surface.
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Most stars probably formed:
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in clusters
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How long does it take for a star like our Sun to form?
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50 million years
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Which relationship concerning the mass of protostars is false?
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The more massive ones glow red, accounting for the color of H II regions.
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What is the key factor that determines the temperature, density, radius, luminosity, and pace of evolution of a protostellar object?
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Mass
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When an H II region is observed, it signals what stage in stellar formation?
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Depending on their masses, the stars inside may be at different stages of formation.
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What is the size of a typical interstellar cloud that is dense enough to form stars?
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10 pc
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As a star forms, the photosphere first appears:
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When the protostar forms
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For gravity to contract a spinning interstellar cloud, there needs to be sufficient:
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Mass
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If the initial interstellar cloud in star formation has a mass sufficient to form hundreds of stars, how does a single star form from it?
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The cloud fragments into smaller clouds and forms many stars at one time.
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A cloud fragment too small to form a star becomes:
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A brown dwarf
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Which event marks the birth of a star?
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Fusion of hydrogen atoms into helium atoms.
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At what stage of evolution do T Tauri stars occur?
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When a protostar is on the verge of becoming a main sequence star.
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How many hydrogen atoms does it take to make a typical star?
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10^57
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How are T Tauri stars characterized observationally?
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By sudden changes in their brightness.
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Evidence for star formation theory comes from:
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Studying different objects at different stages and piecing together an evolutionary picture.
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How long does it take an M-type star to form, compared to the time for a solar-type star to form? `
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20 times as long.
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When a typical open cluster forms, which type of stars are formed most often?
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low mass M type dwarfs
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A star will evolve "off the main sequence" when it uses up which of the following?
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most of the hydrogen in the core
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On the main sequence, massive stars do which of the following?
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burn their hydrogen fuel more rapidly than the Sun
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When the Sun is on the red-giant branch, it will be found where on the H-R diagram?
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upper right
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After the core of a Sun-like star starts to fuse helium on the horizontal branch, the core becomes which of the following?
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hotter
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When the Sun leaves the main sequence, it will become which of the following?
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brighter
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A star like the Sun will end up as what?
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a white dwarf
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The order of evolutionary stages of a star like the Sun would be Main Sequence, giant, planetary nebula, and finally ______.
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none of these
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The helium flash converts helium to the heavier element _____.
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carbon
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How many helium atoms must be fused at 100 million K in the helium flash?
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three
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Which of the following best describes the evolutionary track followed in the HR diagram for the most massive stars?
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horizontally right
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What is used, observationally, to determine the age of a star cluster?
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the luminosity at the main-sequence turnoff
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What is the source of pressure in the core of a red giant that resists the force of gravity?
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electrons which have become incompressible
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In a white dwarf, we have packed the mass of the Sun into the volume of Earth, so the density is:
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a million times that of the Sun.
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What, in addition to its HR diagram, is needed to age-date a star cluster?
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theoretical models of stellar evolution
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What characteristic of a star cluster is used to determine its age?
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The main sequence turnoff.
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The brightest stars of a young open cluster will be:
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massive blue main sequence stars
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In globular clusters, the brightest stars will be:
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red supergiants
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A high-mass star dies more violently than a low-mass star because:
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It generates more heat and its core eventually collapses.
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A ______ is a relatively gentle mass-loss event which allows a star to peacefully readjust its structure into a white dwarf configuration.
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planetary nebula
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Which of these will the Sun probably become in the very distant future?
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planetary nebula
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The evolution of stars appears inevitable. But what likely circumstance can radically alter this evolutionary sequence?
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The stars can be in a short period binary system.
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Which statement is true, in terms of stellar evolution?
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Sooner or later, gravity wins.
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Can a star become a red giant more than once?
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Yes
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Which statement about blue stragglers is false?
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They are much more massive than any other stars known.
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If one star of a binary fills its Roche lobe and is spilling matter onto the other, then the system is a:
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mass-transfer binary
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If two stellar cores share a single envelope, we have a:
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contact bianary
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What results from the mass loss from K and M red giants?
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The wind is rich in dust particles and molecules, including diamonds.
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In a star cluster, just as the most massive stars are evolving into giants and supergiants, what is happening for the lowest mass stars?
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They are just starting to approach the zero-age main sequence.
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Luminous hot stars and luminous cool stars:
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have stellar winds, but each are driven by a different source.
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What is a typical age for a globular cluster?
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12 billion years
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What temperature is needed to fuse helium?
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100 million K
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What are black dwarfs?
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cooled off white dwarfs
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Which of the following is true regarding planetary nebulae?
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They are the ejected envelopes of highly evolved low-mass stars.
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The Roche lobe of a star in a binary star system:
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is, in terms of the star's gravity, its "zone of influence."
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What is a planetary nebula?
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The ejected envelope of a red giant surrounding a stellar core remnant.
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Astronomers talk about "low-mass" and "high-mass" stars with regard to their evolution. In units of solar masses, what is the dividing line, that is, the lowest mass for a high-mass star?
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8 solar masses
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What inevitably forces a star like the Sun to evolve away from being a main sequence star?
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It builds up a core of hellium
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In the evolution of massive stars, what is the significance of the temperature 600 million K?
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The ejected envelope of a red giant surrounding a stellar core remnant.
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A star spends most of its life:
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as a main sequence star.
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What is the significance of 100 million K to the core of a star?
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Temperature need to start triple alpha process and turn helium into carbon.
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The "helium flash" occurs at what stage in stellar evolution?
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red giant
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Just as a low-mass main sequence star runs out of fuel in its core, it actually becomes brighter. How is this possible?
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The core contracts, raising the temperature of the region of hydrogen shell-burning.
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A white dwarf can dramatically increase in brightness only when which of the following applies?
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It has another star nearby.
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Which of the following stars will become hot enough to form elements heavier than oxygen?
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A Star that is eight times more massive than the Sun.
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When does a massive star become a supernova?
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When it forms iron in its core.
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An observable supernova should occur in our Galaxy how often?
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about once every century
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Which one of the following does not provide evidence that supernovae have occurred in our Galaxy?
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The existence of binary stars in our Galaxy.
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Most of the carbon in our bodies originated where?
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the core of a red-giant star
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The silver atoms found in jewelry originated where?
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a supernova
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A surface explosion on a white dwarf, caused by falling matter from the atmosphere of its binary companion, creates what kind of object?
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Nova
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For a nova to occur, the system must have already been a:
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mass-transfer bianary
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Which type of heavy atomic nuclei are most common, and why?
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Even numbered elements, for helium is "giant food" for everything beyond itself.
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Nearly all the elements found in our environment were formed inside stars, except for:
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Hydrogen and Hellium
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The production of which element in the core of a highly evolved giant leads to type II supernovae?
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iron
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Why does neutron capture work?
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Neutrons have no repulsive barrier to overcome in combining with positively charged nuclei.
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What is the only way that a white dwarf can suddenly explode in a type I supernova?
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if it is a member of a mass-transfer binary
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What is stellar nucleosynthesis?
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The formation of heavier elements inside stars.
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Of the elements in your body, the only one not formed in stellar nucleosynthesis is:
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hydrogen
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How long does it take a stellar iron core to collapse?
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one second
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The heaviest nuclei of all are formed:
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By neutron capture during a supernova explosion
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An iron core cannot support a star because:
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Iron cannot fuse with other nuclei to produce energy.
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What direct evidence do astronomers have that supports the heavy element formation in stars?
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all of these
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What was most surprising about SN1987A?
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The parent star was a B supergiant, not a red supergiant.
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The upper mass limit of 1.4 solar masses for white dwarfs won a Nobel prize for:
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Chandrasekhar
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The Chandrasekhar mass limit is ______.
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1.4 solar masses
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A 20 solar mass star has a main sequence lifetime of 10 million years, yet its iron core exists for only about how long?
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less than a day
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As a star evolves, heavier elements tend to form by various processes. Which of the following is not one of these processes?
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Neutronization
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The iron we commonly find in our surroundings came from this source.
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decay of nickel-56 and cobalt-56 in a supernova remnant
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What is the reason a type-II supernova slows its dimming after about 2 months?
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Energy is released from the decay of radioactive cobalt-56 to iron-56.
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The transformation of cobalt 56 into iron 56 is an example of:
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the weak force and nuclear fission
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The making of abundant iron nuclei is typical of:
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type II supernova
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What made supernova 1987a so useful to study?
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all of these
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Where was supernova 1987a located?
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In our companion galaxy, the Large Magellanic Cloud
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Which of these is least likely to happen?
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recurrent supernova of type I
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Which of these is the likely progenitor of a type I supernova?
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a mass-transfer binary, with the white dwarf already at 1.3 solar masses
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Which of these is the likely progenitor of a type II supernova?
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an evolved red giant which is just starting to make silicon in its core
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Which of the following does not fit a type I supernova?
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Implosion-explosion of the core of a massive star.
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A star can be a supernova:
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once
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The supernova that formed M-1, the Crab Nebula, was observed in what year?
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1054 AD by the Chinese
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What is the total energy radiated by a supernova equal to?
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1 billion suns
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The total energy emitted by the brightest nova explosions is about:
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1 million suns
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What produces a type-I supernova?
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Mass transfer to a white dwarf in a binary where the Chandrasekhar mass is exceeded.
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When helium capture occurs with a carbon-12 nucleus, what results?
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oxygen-16
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When two silicon-28 nuclei fuse, the initial result is:
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nickel-56
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What evidence is there that supernovae really have occurred?
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All of these
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When a stellar iron core collapses, large numbers of neutrinos are formed, then:
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They immediately pass through the core and escape to space.
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A recurrent nova can eventually build up to a:
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type I supernova
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In order of visual luminosity at the start, which is most luminous?
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type I supernova
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Which of these do not depend on a mass-transfer binary to occur?
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a type II supernova
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The alpha process tends to produce chiefly:
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even numbered elements
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Which of the following is not an argument for Cygnus X-1's being a true black hole?
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The mass of the visible B star is even greater than Cygnus X-1, at around 30 solar masses.
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What explanation does general relativity provide for gravity?
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Gravity is a result of curved spacetime.
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What makes the Crab pulsar somewhat unusual among pulsars in general?
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It is rather bright at visible wavelengths.
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Three terrestrial planetary-sized masses have been discovered orbiting what type of object?
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a millisecond pulsar
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What compelling evidence links pulsars to neutron stars?
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Only a small rotating source of radiation is thought to be able to emit precisely timed pulses such as those from pulsars.
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The key to identifying a black hole candidate in a binary system is the following:
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the unseen companion in the system must have a sufficiently high mass
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Which of these is least likely to exist?
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a 1.8 solar mass white dwarf
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Almost half of all known millisecond pulsars are found in what type of object?
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globular clusters
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Who discovered the first object that eventually became known as a pulsar?
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Jocelyn Bell
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Who received the Nobel Prize in Physics for relating pulsars to neutron star formation?
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Anthony Hewish.
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The supernova of 1054 AD produced:
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a pulsar with a period of 33 milliseconds, visible optically.
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Which of the following is not a property of the first discovered pulsar (nor any other pulsar)?
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emissions only in the visible part of the spectrum
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In the Lighthouse model,
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if the beams sweeps across us, we can observe the pulse.
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What are X-ray bursters?
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They are neutron stars on which accreted matter builds up, then explodes in a violent nuclear explosion.
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What is Cygnus X-1?
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a leading candidate for being a black hole
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X-ray bursters occur in binary star systems. What are the two types of stars that must be present to make up such an object?
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a main sequence or giant star and a neutron star
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Which of the following are attracted by gravity?
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all of these
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Which of the following can actually escape a black hole?
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nothing
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What would happen if mass is continually added to a 1.4 solar mass neutron star?
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The star would eventually become a black hole.
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What would happen if mass is added to a 1.4 solar mass white dwarf?
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The star would erupt as a type I supernova.
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Which statement about gamma ray bursts is not correct?
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They are a scaled up version of the X-ray bursts, with more massive stars involved.
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In a "hypernova", the very energetic supernova creates a:
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black hole
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While perhaps affected by rotation and magnetism, we think the lower limit for black holes is:
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Schwartzchild's limit of 3 solar masses.
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When we use Hubble's law to estimate the age of the universe, which of the following is true of the answer?
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the answer is the same for all galaxies
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Olber's paradox is resolved by which of the following?
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the finite age of the universe
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On the basis of our current best estimate of the present mass density of the universe, astronomers think which of the following?
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the universe is infinite in extent and will expand forever
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Because almost all of the galaxies are redshifted, we know that:
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the universe is expanding
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The redshift of galaxies in the universe is correctly interpreted as:
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Space itself is expanding with time; the wavelengths of photon are stretched while they travel through space.
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From the 1970's through the 1990's, the accepted value of H was almost doubled. This meant:
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the Hubble Time was halved.
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What does the Hubble law imply about the history of the universe?
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The universe started expanding at some time in the past; the universe has an age.
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The cosmic microwave background is important mostly because:
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It confirmed a major prediction made by the Big Bang theory.
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Who was involved in the discovery of the cosmic microwave background radiation?
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Bell Labs and Princeton
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The universe has three possible futures. Which one is correct depends only on the average density of matter in the universe. Why is this?
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The density of matter determines the strength of gravity, which decelerates the expansion over time.
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The presently accepted values for Hubble constant gives which range of ages for the universe?
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10 to 20 billion years
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What is the meaning of a "closed" universe?
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The universe will someday stop expanding and start to collapse.
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Homogeneity and isotropy, taken as assumptions regarding the structure and evolution of the universe, are known as:
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The cosmological principle.
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In which of the following models will the universe stop expanding?
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Closed universe.
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The geometry of a closed universe, in two dimensions, resembles which one of the following?
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The surface of a sphere.
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What is the meaning of isotropic?
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The same in all directions.
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The darkness of the night sky in a seemingly infinite universe is addressed in:
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Olbers' Paradox.
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The explanation for the darkness of the night sky is that (select all that apply):
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-the Big Bang means the universe is not infinitely old or large. -the energy of the distant galaxies has been weakened in their red shifting.
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If the density of the universe is less than critical, then:
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the universe will "survive" to expand forever.
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For a Hubble constant of 65 km/s/Mpc, the critical density is about:
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8 ✕ 10-27 kg/m3
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Recent work with supernovae at great distances suggests the universe may in fact be accelerating its expansion, a startling discovery attributed to a new:
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dark energy
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In the critical universe now proposed, the ratio of matter/energy is about:
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35/65
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According to their H-R diagram turn-off points, the oldest globular clusters are about:
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12 billion years old
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The satellite most responsible for studying the microwave universe is:
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COBE
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For a spatially flat (Euclidean) universe, o is:
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1.0
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If the presently accepted value of o = 0.3 is indeed correct, then the universe will:
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expand forever