Exam 10: The Interstellar Medium

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The composition of the interstellar dust suggests that it is formed primarily in the atmospheres of cool stars.

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Elements such as carbon, silicon and oxygen have been produced in stars and expelled as stars age in the interstellar medium. This is most likely due to these elements having cooled and condensed from aging stars to form dust grains, and carried out by a powerful winds.

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Molecules in the interstellar medium emit radiation at what wavelengths?

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The type of radiation that is emitted when the electron in a hydrogen atom experiences a spin flip is a (n) _______________.

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H I clouds can be observed using _____.

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______________ are cool, with temperatures of about 100 K and densities of ten to a few hundreds of atoms per cubic centimeter.

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Interstellar dust scatters _____________light more than _____________light.

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Calculations of the Sun's future evolution indicate that it will blow away almost half of its mass in several relatively short episodes about 4 to 5 billion years from now before it is finally extinguished.

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H II emission nebula regions are found around _____________.

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Large molecular clouds will form into protostars because of ____.

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The _______________ is a high temperature, low density region in the interstellar medium around the Sun.

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Why is the sky blue during the day?

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If hydrogen (H2) gas is the most common molecule found within the interstellar medium, then why do astronomers measure the amount of carbon monoxide (CO) gas to map molecular clouds?

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_______________ is believed to be produced by supernova explosions.

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Stars are born in reflection nebulae.

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The intercloud medium is believed to make up 90 percent of the mass of the interstellar medium.

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The interstellar reddening does not shift the _______________ of spectral lines, as does the Doppler effect.

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Which mission passed the bow shock in the Universe?

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Which telescope imaged the center of the Milky Way Galaxy at a wavelength of 8 microns to reveal the distribution of the dusty interstellar medium?

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The emission lines from O III are called ____ because they are not visible laboratories on Earth due to the much greater pressure of the gas on Earth.

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