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Low mass stars should produce white dwarfs,while high mass stars will produce more compact end products.

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What is peculiar about Sirius based on historical records?

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Records from 100 B.C.to 200 A....

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How is the age of a star cluster determined?

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The stars are plotted on an H-R diagram....

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What is the typical age for a globular cluster associated with our Milky Way?


A) a few million years
B) 200 million years
C) a billion years
D) 10-12 billion years
E) 45 billion years

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How has the chemical composition of the core of the Sun changed in the past 4.5 billion years? Are earthlings (if any)likely to freeze in another 4-5 billion years? Explain.

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The core of the Sun had an initial compo...

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A star is on the horizontal branch of the H-R diagram.Which statement is true?


A) It is burning both hydrogen and helium.
B) It is about to experience the helium flash.
C) It is burning only helium.
D) The star is contracting.
E) The star is about to return to the main sequence.

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A high-mass star dies more violently than a low-mass star because:


A) it must always end up as a black hole.
B) it generates more heat and its core eventually collapses very suddenly.
C) it cannot fuse elements heavier than carbon.
D) gravity is weakened by its high luminosity.
E) it is most often found as part of a binary system.

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The order of evolutionary stages of a star like the Sun would be Main Sequence,giant,planetary nebula,and finally:


A) hypernova.
B) neutron star.
C) white dwarf.
D) nova.
E) black hole.

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For our Sun,the production of carbon will be the end of its nucleosynthesis.

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What is the significance of 8 solar masses in stellar evolution?

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Above 8 solar masses,a high mass star mu...

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A solar mass star will evolve off the main sequence when:


A) it completely runs out of hydrogen.
B) it expels a planetary nebula to cool off and release radiation.
C) it explodes as a violent nova.
D) it builds up a core of inert helium.
E) it loses all its neutrinos, so fusion must cease.

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Isolated main-sequence stars as massive as 10 to 12 times the mass of the Sun may still manage to avoid going supernova.Why?


A) because they can also have strong stellar winds
B) because about half that mass will be contained in the carbon core
C) because they would be classified as brown dwarfs
D) because these stars will eject at least 4 solar masses in the planetary nebula stage
E) because their masses will decrease as they fuse heavy elements into lighter elements in their cores

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The age of a star cluster may be estimated by determining the ________ of the Main Sequence at which stars are just in the process of evolving away to become giant stars.

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A star (no matter what its mass) spends most of its life:


A) as a protostar.
B) as a main sequence star.
C) as a planetary nebula.
D) as a red giant or supergiant.
E) as a T Tauri variable star.

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Mass transfer will almost always occur for spectroscopic and eclipsing binaries.

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The longest stage in the life cycle of a star is as a(n)________ star.

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Eventually,all low mass stars will become white,then black,dwarfs.

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Modern astronomers have observed the complete life cycle for many stars,making stellar evolution one of the best-tested astronomical theories.

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Noting the turnoff mass in a star cluster allows you to determine its:


A) distance.
B) radial velocity.
C) age.
D) total mass.
E) number of stars.

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As a 4-10 solar mass star leaves the main sequence on its way to becoming a red supergiant,its luminosity:


A) decreases.
B) first decreases, then increases.
C) increases.
D) remains roughly constant.
E) first increases, then decreases.

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