Exam 15: Star Formation and the Interstellar Medium

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The entire process of star formation is really just an evolving balance between:

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C

Because angular momentum must be conserved,as a gas cloud contracts due to gravity it will also:

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The lowest-density gas in the interstellar medium is also the coldest.

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How long does it typically take for a protostar to form a 1 M star?

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A _________ is a failed star that shines primarily because of energy derived from its gravitational collapse rather than nuclear burning.

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Dust that is heated to 30 K will emit a blackbody spectrum that peaks at:

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We observe neutral hydrogen gas using 21-cm emission.

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Why does a protostar continue to collapse as it is forming?

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Some molecular clouds have so much internal pressure that it exceeds their self-gravity.What keeps them from expanding and dissipating?

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The source of energy for a contracting protostar comes from:

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What primarily makes it difficult to observe protostars?

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The average density of the interstellar medium is:

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Compare the volume of the Sun with the volume of interstellar space it occupies.Is the occupied percentage large or small? Consider the volume around the Sun to be a sphere whose radius is equal to the distance to the nearest star,which is equal to 5 light-years.(Note: the radius of the Sun is 7 × 105 km,and 1 light-year = 9.5 × 1012 km. )

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What is the interstellar medium made of? Give rough percentages of each.

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Given the low efficiency of the star formation process,the initial mass of a molecular cloud fragment that formed a 2 M star was probably close to:

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Molecular cloud cores are places where you might find:

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What critical event transforms a protostar into a normal main-sequence star?

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The average density of the interstellar medium is many times less dense than the best vacuum on Earth.

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Why can we see dust in the interstellar medium better at far-infrared wavelengths than we can at optical wavelengths?

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As a protostar evolves,its temperature:

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