1.
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Quiz 6 - Q1
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Unlike supernovae, novae can explode more than once, increasing their luminosity by thousands of times. |
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Student Response | Value | Correct Answer |
True | 100% | True |
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Score: | 5/5 |
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2.
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Quiz 6 - Q2
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A Type I supernova involves the collapsing core of a high mass star. |
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Student Response | Value | Correct Answer |
False | 100% | False |
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Score: | 5/5 |
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3.
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Quiz 6 - Q3
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The Chandrasekhar mass limit is |
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| Student Response | Value | Correct Answer | Feedback |
| .08 solar masses. | | | |
| .4 solar masses. | | | |
| 1.4 solar masses. | 100% | | |
| 3 solar masses. | | | |
| 8 solar masses. | | | |
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Score: | 5/5 |
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4.
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Quiz 6 - Q4
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For a nova to occur, the system must have already been a |
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| Student Response | Value | Correct Answer | Feedback |
| astrometric binary. | | | |
| detached binary. | | | |
| spectroscopic binary. | 0% | | |
| mass-transfer binary. | | | |
| eclipsing binary. | | | |
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Score: | 0/5 |
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5.
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Quiz 6 - Q5
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An iron core cannot support a star because |
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| Student Response | Value | Correct Answer | Feedback |
| iron is the heaviest element, and sinks upon differentiation. | | | |
| iron has poor nuclear binding energy. | | | |
| iron cannot fuse with other nuclei to produce energy. | 100% | | |
| iron supplies too much pressure. | | | |
| iron is in the form of a gas, not a solid, in the center of a star. | | | |
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Score: | 5/5 |
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6.
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Quiz 6 - Q6
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A massive star can fuse only up to the element silicon in its core. |
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Student Response | Value | Correct Answer |
False | 100% | False |
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Score: | 5/5 |
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7.
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Quiz 6 - Q7
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A Type I supernova is more similar to a nova than a Type II supernova. |
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Student Response | Value | Correct Answer |
True | 100% | True |
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Score: | 5/5 |
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8.
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Quiz 6 - Q8
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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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| Student Response | Value | Correct Answer | Feedback |
| hypernova | | | |
| nova | 100% | | |
| gamma ray burster | | | |
| Type I supernova | | | |
| Type II supernova | | | |
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Score: | 5/5 |
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9.
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Quiz 6 - Q9
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Most of the energy of the supernova is carried outward via a flood of |
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| Student Response | Value | Correct Answer | Feedback |
| gamma rays. | | | |
| helium nuclei. | | | |
| protons. | | | |
| neutrinos. | 100% | | |
| positrons. | | | |
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Score: | 5/5 |
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10.
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Quiz 6 - Q10
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Stellar nucleosynthesis is responsible for the existence of all elements except hydrogen. |
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Student Response | Value | Correct Answer |
False | 100% | False |
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Score: | 5/5 |
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11.
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Quiz 6 - Q11
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Match the following: |
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Shows the spectrum with little hydrogen
Red giant losing mass to white dwarf companion
Can be recurrent
an overloaded white dwarf
collapse of a supermassive star
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Type II supernova
Type I supernova
nova
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Statement | Response | Value | Correct Match |
Shows the spectrum with little hydrogen | Type I supernova | 20.0% | Type I supernova |
Red giant losing mass to white dwarf companion | Type II supernova | 0.0% | nova |
Can be recurrent | nova | 20.0% | nova |
an overloaded white dwarf | Type I supernova | 20.0% | Type I supernova |
collapse of a supermassive star | Type II supernova | 20.0% | Type II supernova |
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Score: | 16/20 |
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12.
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Quiz 6 - Q12
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In neutronization of the core, a proton and an electron make a neutron and a |
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| Student Response | Value | Correct Answer | Feedback |
| positron. | | | |
| muon. | | | |
| neutrino. | 100% | | |
| pion. | | | |
| antineutrino. | | | |
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Score: | 5/5 |
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13.
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Quiz 6 - Q13
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As a star's evolution approaches the Type II supernova, we find |
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| Student Response | Value | Correct Answer | Feedback |
| the heavier the element, the less time it takes to make it. | | | |
| the heavier the element, the higher the temperature to fuse it. | | | |
| helium to carbon fusion takes at least 100 million K to start | | | |
| photodisintegration of iron nuclei begins at 10 billion K to ignite the supernova. | | | |
| all of the above. | 100% | | |
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Score: | 5/5 |
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14.
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Quiz 6 - Q14
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Where was supernova 1987a located? |
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| Student Response | Value | Correct Answer | Feedback |
| in the Orion nebula, M42 | | | |
| in the Large Magallanic cloud | 100% | | |
| in Sagittarius | | | |
| in the cluster M13 | | | |
| In M31, the Andromeda galaxy. | | | |
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Score: | 5/5 |
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15.
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Quiz 6 - Q15
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Which of these is the likely progenitor of a type I supernova? |
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| Student Response | Value | Correct Answer | Feedback |
| a mass-transfer binary, with the white dwarf already at 1.3 solar masses | 100% | | |
| a contact binary, with the neutron star at 2.3 solar masses | | | |
| an evolved red giant which is just starting to make silicon in its core | | | |
| an evolved blue supergiant that is about to experience the helium flash | | | |
| a helium-neon white dwarf | | | |
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Score: | 5/5 |
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16.
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Quiz 6 - Q16
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Which of these events is not possible? |
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| Student Response | Value | Correct Answer | Feedback |
| low-mass stars swelling up to produce planetary nebulae | | | |
| red giants exploding as Type II supernovae | | | |
| close binary stars producing recurrent novae explosions | | | |
| white dwarfs and companion stars producing recurrent Type I supernova events | 100% | | |
| a white dwarf being found in the center of a planetary nebula | | | |
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Score: | 5/5 |
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17.
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Quiz 6 - Q17
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Nearly all the elements found in nature were formed inside stars, except for |
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| Student Response | Value | Correct Answer | Feedback |
| carbon and silicon. | | | |
| hydrogen and helium. | 100% | | |
| iron and molybdenum. | | | |
| silver and gold. | | | |
| uranium and radium. | | | |
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Score: | 5/5 |
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