Astronomy Final Test 3 assesses knowledge on stellar processes, including solar energy generation, star luminosity, surface phenomena, and lifecycle stages of stars like the Sun. It is designed to evaluate understanding of fundamental astronomical concepts and their practical implications.
Temperature and radius
Mass and temperature
Brightness and distance
Age and temperature
None of the above
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Fusion rate in the core
Convection process near the surface
Temperature distribution at the surface
Magnetic field near the surface
None of the above
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The ignition of carbon in the star's core
The helium flash
The expulsion of the star's outer layers in a planetary nebula
The formation of a white dwarf
None of the above
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Mass
Luminoisity
Temperature
Radius
All of the above
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White dwarf
Brown dwarf
Planetary nebula
Red giant
None of the above
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Helium
Iron
Carbon
Neutrons
None of the above
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A star spends the majority of its lifetime in the red giant stage
Red giants are cool stars yet still are quite luminous
Red giants fuse hydrogen into helium in their cores
Red giants are the largest stars that exist in the Universe
None of the above
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Fusion and fission
Mass and energy
Temperature and luminosity
Fusion and electric repulsion
Pressure and gravity
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Fifteen thousand K
Fifteen million K
Sixty K
Six thousand K
None of the above
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Cooler
Smaller
More Massive
Older
All of the above
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Protostar, main sequence, red giant, yellow giant, red supergiant, planetary nebula, white dwarf
Main sequence, protostar, yellow giant, red giant, red supergiant, planetary nebula, white dwarf
Protostar, red giant, main sequence, yellow giant, red supergiant, white dwarf, planetary nebula
Main sequence, red giant, protostar, yellow giant, red supergiant, white dwarf, planetary nebula
None of the above
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The star must be far away
The star must be young
The star must be on the main sequence
The star must be at the end of its lifetime
None of the above
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Expand and cool
Contract and heat
Expand and heat
Turn into iron
Turn into uranium
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The core would subsequently rise in temperature even more and shrink in size
The outer layers of the Sun would shrink and heat up
The core would expand in size and cool
The outer layers of the Sun would expand and heat up
None of the above
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B3 III
A4 V
M7 I
B7 V
All of the above have the same surface temperature
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Helium created during nuclear fusion
Convection dredging that brings cores material to the surface of the Sun
Magnetic fluctuations in the Sun's corona
Solar neutrinos that escape from the Sun's core
None of the above
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Yellow giant
White dwarf
Red giant
Blue supergiant
Red supergiant
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They are cooler than the surrounding material
They do not emit any light
The Sun's magnetic field suppresses visible light
They are holes in the surface of the Sun
None of the above
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Age
Luminoisity
Mass
Temperature
None of the above
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Alternative convection motion
Coronal revolution
Magnetic resonance differentiation
Atypical spiral motion
None of the above
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4 hydrogen atoms: 1 carbon atom
1 helium atom: 4 hydrogen atoms
1 hydrogen atom: 4 helium atoms
4 hydrogen atoms: 1 helium atom
None of the above
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A yellow star
A blue star
An orange star
A red star
None of the above
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Corona
Chromosphere
Radiative zone
Core
None of the above
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Lumionisty
Radius
Brightness
Mass
All of the above
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Convection
Magnetic fields
Winds
Conduction
Radiation
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Sun, white dwarf, red giant
Red giant, white dwarf, Sun
Red giant, Sun, white dwarf
White dwarf, Sun, red giant
None of the above sequences is correct
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Protostar
Main sequence
Red giant
Double shell burning phase
White dwarf
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The core shrinks up and heats
The core shrinks and cools down
The core expands and heats up
The core expands and cools down
The core expands without changing temperature
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They would be too massive for hydrogen fusion to occur
They would shine exclusively at X-ray wavelengths and would be difficult to detect
Molecular could do not have enough material to form such massive stars
They would fragment into binary stars because of their rapid rotation
They would generate so much power that they would blow themselves apart
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