Astronomy Final Review

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Flashcards about the Interstellar Medium, Nebulae, Star Birth, and Planet Formation

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23 Terms

1
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What is the Interstellar Medium (IM)

The name for all material between the stars, made of gas and dust.

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What is the composition of the Interstellar Medium (IM)

75% Hydrogen, 24% Helium, 1% Dark Dust

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What is the temperature and Density of the Interstellar Medium

Very cold (10-100* K) and extremely low density

4
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What does the composition of the Interstellar Medium (IM) prove?

That the sun was made from the IM.

5
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What is a Nebula?

Any blob of gas and dust in space.

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Where atoms stay together to become molecules

In dark nebulae (colder clouds of gas and dust)

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Who first proposed the idea of the birth of stars?

Immanuel Kant

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Which stars are born most quickly?

Heavier stars

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What are the early steps in the growth of a star

  • As the original cloud collapses, the cloud’s temperature gets hotter;

  • 99% of the cloud material gets to the center and begins to resemble a protostar (center is about 1,000,000* K)

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What happens to the spin of a cloud after it collapses?

The cloud spins faster.

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What happens as a result of increased cloud spin during the birth of a star?

The cloud flattens into a disk shape, called a proplanetary disk.

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What are the later steps in the growth of a star

  • Nuclear fusion begins in its core once it reaches the appropriate, hot, temperature;

  • Fusion causes energy to flow out, providing outward pressure as it flows;

  • The star is no longer being shrunk by gravity, making it a “real star”

13
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Why are Brown Dwarfs considered “failed stars”?

Their masses are too light, making the temperature inside too cold to perform nuclear reactions.

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How do protoplanets start to form?

  • Grains/clumps of dust cling to each other by the electromagnetic force, creating clumps of dust called planetesimals;

  • Once the planetesimals gain mass, their gravity increases, causing mass to be added on at a faster rate (accretion);

  • Gravity makes the planetesimals rounder, forming protoplanets

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Why did planets nearest to the sun not grow large?

  • There was less material for them to scoop up in their shorter paths;

  • The temperature was too hot meaning that material was not solid, preventing growth (planets need solid materials to grow large)

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How did outer planets, like Jupiter & Saturn, grow to be so huge?

  • There was more material in their longer paths;

  • Many gases out there froze, creating solids which then fuel growth.

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What caused the era of bombardment?

Outer layers of young planets turned solid, as well as planetesimals. These bodies collided a lot, leading to shattering and meteors flying everywhere, constantly striking planets and moons.

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How was Mercury affected during the era of bombardment?

Some of its thin, outer layers were removed.

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How was Mars affected during the era of bombardment?

Its northern parts were knocked off, and some of that debris made Mars’s 2 moons.

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How was the Moon affected during the era of bombardment?

Material was ripped off of Earth, loose material clung back together to create the Moon.

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What affected planets’s orbits, causing planetary migration after being born?

Planets pulled on each other;

Jupiter invaded the Asteroid Belt;

Uranus & Neptune invaded the Kuiper Belt

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How did liquid water end up being on Earth?

Melted ice that came from comets and asteroids which were tossed around due to the gravity of invading planets.

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What will happen when the Sun dies?

A Planetary Nebula will appear; A White Dwarf (remaining dead core of a star) will be seen