Exam 11: Formation and Structure of Stars
Exam 1: Here and Now50 Questions
Exam 2: A Users Guide to the Sky68 Questions
Exam 3: Moon Phases and Eclipses68 Questions
Exam 4: Origins of Modern Astronomy64 Questions
Exam 5: Gravity76 Questions
Exam 6: Light and Telescopes69 Questions
Exam 7: Atoms and Spectra73 Questions
Exam 8: The Sun70 Questions
Exam 9: The Family of Stars70 Questions
Exam 10: The Interstellar Medium51 Questions
Exam 11: Formation and Structure of Stars44 Questions
Exam 12: Stellar Evolution51 Questions
Exam 13: Deaths of Stars74 Questions
Exam 14: Neutron Stars and Black Holes69 Questions
Exam 15: The Milky Way Galaxy72 Questions
Exam 16: Galaxies75 Questions
Exam 17: Supermassive Black Holes and Active Galaxies68 Questions
Exam 18: Modern Cosmology71 Questions
Exam 19: Origin of the Solar System and Extrasolar Planets69 Questions
Exam 20: Earth the Active Planet71 Questions
Exam 21: The Moon and Mercury70 Questions
Exam 22: Venus and Mars67 Questions
Exam 23: Jupiter and Saturn68 Questions
Exam 24: Uranus Neptune Pluto and the Kuiper Belt68 Questions
Exam 25: Meteorites Asteroids and Comets65 Questions
Exam 26: Astrobiology68 Questions
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Hydrostatic equilibrium is the balance between _____________ and radiation _____________.
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(Short Answer)
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weight; pressure
When a large gas cloud starts to collapse in a free-fall due to gravity, the rotation rate will ______________.
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(Short Answer)
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increase,go faster
During the main sequence lifetime of a star of any mass, the core of the star will be composed mainly of ____.
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(Multiple Choice)
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Correct Answer:
B
When a large gas cloud starts to collapse in a free-fall due to gravity, the temperature of the gas will _____________.
(Short Answer)
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How do large mass stars in the upper region of the main sequence produce energy?
(Multiple Choice)
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The proton-proton chain needs a high temperature because the protons must overcome the _____________.
(Short Answer)
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Eighty percent of the stars on the H-R Diagram are on the main sequence, and that is because the star is in hydrostatic equilibrium due to the _____.
(Multiple Choice)
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One of the major star forming regions in space is the Orion Nebula.
(True/False)
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Pre-main sequence stars (not protostars) on the H-R Diagram are _____.
(Multiple Choice)
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One of the factors that a large molecular cloud must overcome in order for gravitational contraction to begin is the thermal energy of the gas.
(True/False)
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Hydrostatic equilibrium in a newborn star is regulated by a very unique thermostat called the _____________ thermostat.
(Short Answer)
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There are several triggers that could start the gravitational contraction of a molecular cloud and subsequent star formation. List two of these triggers.
(Essay)
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Energy flows by radiation or convection inside normal stars but almost never by _____________ because radiation or convection is much more efficient.
(Short Answer)
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A protostar will continue to collapse due to gravity until it reaches the main sequence, and then gravitational collapse will stop when _____ begins.
(Multiple Choice)
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Low mass stars like the Sun transport energy near their surface using convection.
(True/False)
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Stellar winds and _____ will eventually blow away the protostellar disk and remnant cocoons of a protostar apart.
(Multiple Choice)
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One of the factors that a large molecular cloud must overcome in order for gravitational contraction to begin is rotation of the gas cloud.
(True/False)
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Before a giant molecular cloud can contract gravitationally, it must overcome four physical factors that resist compression. What are these four factors?
(Essay)
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Describe the concept of a "birth line" and identify where it falls on the H-R Diagram.
(Essay)
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