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What factors can complicate the collapse of an interstellar cloud into a star?

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The initial spin of the cloud and the co...

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Type M stars evolve to the main sequence faster than our G type Sun.

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Which relationship concerning the mass of protostars is FALSE?


A) The more massive ones will reach the main sequence first.
B) The more massive ones will be the hottest and most luminous.
C) The more massive ones one will be made of the heaviest elements.
D) The more massive ones are so luminous they ionize the gas, hence red H II regions.
E) The more massive ones create a lot of ultraviolet as well as visible light.

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Brown dwarfs are most easily detected which portion of the electromagnetic spectrum?


A) X-ray
B) ultraviolet
C) visible light
D) infrared
E) radio

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Why does a star's luminosity drop so much during the Hayashi track?

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The surface of the star maintains a fair...

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Our Sun,along with most of the stars in our neighborhood,probably formed:


A) a few million years ago.
B) about 10 million years ago.
C) hundreds of millions of years ago.
D) billions of years ago.
E) at the beginning of the universe.

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Protostars can be observed in:


A) the Crab Nebula.
B) the Andromeda Galaxy.
C) the Orion Nebula.
D) our Solar System.
E) the Helix Nebula.

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Discuss the relationship between young stars and the interstellar medium.

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Young stars give off ultraviolet radiati...

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Why are brown dwarfs difficult to detect? Why have we had recent successes?

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They are too cool to ignite nuclear fusi...

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Higher mass protostars enter the main sequence:


A) faster and at a higher luminosity and temperature.
B) faster and at a lower luminosity and temperature.
C) slower and at a higher luminosity and temperature.
D) slower and at a lower luminosity and temperature.
E) at the same rate, but at a higher luminosity and temperature.

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What makes the subject of star formation so difficult and complex?


A) It is so slow that no visible proof of it exists.
B) Star formation is too expensive to study in detail.
C) Stars live too long to be observed from birth to death.
D) Clouds, fragments, protostars, stars, and nebulae all interact and influence each other.
E) Shock waves disrupt the orderly evolution of stars.

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A protostar of 20 solar masses will probably turn into a type O main sequence star.

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Most stars are usually formed singularly or as binaries,not in clusters.

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In the collapsing cloud fragment stage (stage 2) of star formation,the size of the cloud fragment is about:


A) the size of the solar system.
B) 10 times the size of the solar system.
C) 100 times the size of the solar system.
D) 1,000 times the size of the solar system.
E) 10,000 times the size of the solar system.

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How long does it take for a star like our Sun to form?


A) 100 thousand years
B) two million years
C) fifty million years
D) one billion years
E) 4.6 billion years

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At the end of the Kelvin-Helmholtz contraction a star is hundreds of times brighter than it will be as a main sequence star.

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What is the key factor that determines the temperature,density,radius,luminosity,and pace of evolution of a protostellar object?


A) composition of the nebula
B) rotation of the nebula
C) mass of the nebula
D) temperature of the nebula
E) magnetism of the nebula

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How long does it take an O-type star to form,compared to the time for a solar-type star to form?


A) 1/300 as long
B) 1/30 as long
C) about the same time
D) 30 times longer
E) 300 times longer

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During a protostar's T Tauri phase,it:


A) begins a period of reduced activity.
B) expands dramatically.
C) lies on the main sequence.
D) may develop very strong winds.
E) changes its spin direction.

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Brown dwarfs are failed stars,never igniting their hydrogen fusion.

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