Exam 10: Structure and Formation of Stars

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What observations reveal star formation in the Orion nebula?

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Opacity is

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Stars with masses less than ____ produce most of their energy via the proton-proton chain.

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The lowest mass object that can initiate thermonuclear fusion of hydrogen has a mass of about

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Why are interstellar absorption lines so narrow compared to the width of lines which originate in the photopsheres of stars?

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What causes the outward gas pressure that balances the inward pull of gravity in a main sequence star?

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____ are small dark nebulae about 1 light-year in diameter that contain 10 to 1,000 solar masses.

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The lower edge of the Main Sequence band is known as ____ and represents the location in the HR-diagram at which stars begin their lives as main sequence stars.

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The dust in the interstellar medium can make distant stars look redder than they really are.

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The capture of too few solar neutrinos by Davis in the solar neutrino experiment

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How do measurements of neutrinos from the sun pose a problem for modern astronomy?

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If energy is carried by the bulk motion of matter, that is called ____________________.

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In the proton-proton chain

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The nuclear reactions in a star s core remain under control so long as

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Protostars are difficult to observe because

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The thermal motions of the atoms in a gas cloud can make it collapse to form a protostar.

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Some young star clusters contain large numbers of T Tauri stars.

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What is the difference between the proton-proton chain and the CNO cycle?

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What observations demonstrate the existence of an interstellar medium?

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The condition of ____________________ means that the force due to gravity pushing down on a layer is exactly equal to the pressure pushing outward on that layer.

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