CP 16 Star-Forming Clouds Flashcards

1
Q

Most interstellar clouds remain stable in size because the force of gravity is opposed by __________ within the cloud.

A

thermal pressure

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2
Q

What conditions of gas cloud is most likely to give birth to stars?

A

a cold, dense gas cloud

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3
Q

Which molecule is the most abundant in an interstellar molecular cloud?

A

H2

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4
Q

How do we learn the chemical composition of the interstellar medium?

A

By studying spectra of interstellar gas clouds

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5
Q

Which part of the electromagnetic spectrum generally gives us our best views of stars forming in dusty clouds?

A

infrared

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6
Q

What is the cloud required to do to allow a gravitationally-collapsing gas cloud to continue to collapse?

A

The cloud must radiate away much of its thermal energy.

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7
Q

Which two processes can generate energy to help a star or gas cloud maintain its internal thermal pressure?

A

nuclear fusion and gravitational contraction

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8
Q

TF The first stars born in the universe were made only of Hydrogen and Helium

A

T

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9
Q

During the time before fusion begins, a protostar’s core gradually ________.

A

shrinks and heats

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10
Q

When does a protostar become a main-sequence star?

A

when rate of H fusion = rate which the star radiates energy into space

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11
Q

Approximately what core temperature is required before hydrogen fusion can begin in a star?

A

10 million K

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12
Q

Why are the very first stars thought to have been much more massive than the Sun?

A

The temperatures of the clouds that made them were higher because they consisted entirely of hydrogen and helium.

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13
Q

What is the approximate range of masses that newborn main-sequence stars can have?

A

0.1 to 150 solar masses

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14
Q

If a star is extremely massive (more than 100-solar masses), why isn’t it likely to survive

A

It may blow itself apart because of radiation pressure.

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