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Stellar Evolution 2021

Science, Physics

11th - 12th Grade

Used 9+ times

Stellar Evolution 2021
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30 questions

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1.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

The most important property that determines the evolution of a star is its ________________.

temperature

composition

mass

location

2.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

For a star like the Sun, the gravitational collapse of the interstellar cloud lasted for about ______________ and stopped with the ignition of the fusion reaction.

50–100 billion years

5–10 billion years

1 billion years

100 million years

1–10 million years

3.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

____ is the most significant force that determines the evolution of stars.

Temperature

Luminosity

Energy

Gravity

4.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

Why does a high-mass star evolve differently from a low-mass star?

It can fuse additional elements because its core can get hotter.

It has more material to burn so it can last longer.

It is so bright that it drives material in space away from it so it can't gather up more fuel.

It has a lower gravity so it can't pull in more fuel from space.

The statement is false. High and low-mass stars evolve the same way.

5.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

The Sun's evolution from youngest to oldest stage is

white dwarf, red giant, main sequence, protostar.

red giant, main sequence, white dwarf, protostar.

protostar, red giant, main sequence, white dwarf.

protostar, main sequence, red giant, white dwarf.

6.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

Brown dwarfs are

large terrestrial planets.

objects massive enough to fuse deuterium but not massive enough to sustain hydrogen fusion.

very low-mass main sequence stars.

what is left over after a massive star ejects most of its material through a supernova.

7.

MULTIPLE CHOICE QUESTION

30 sec • 1 pt

When do we say that a star is born?

when the interstellar cloud collapses

when the interstellar matter achieves the Jeans instability

when fusion of hydrogen atoms into helium atoms starts

when the star leaves the main sequence

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