2.1 Solar nebular model Flashcards

1
Q

When was the Big Bang?

A

14 billion years ago (14 Ga)

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2
Q

When was the solar system formed?

A

4.6 billion years ago (4.6 Ga)

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3
Q

What is a nebula?

A

A giant cloud of molecular hydrogen and dust.

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4
Q

What happened to the nebula to begin the creation of the solar system?

A

It collapsed, possibly due to the shockwave from a nearby exploding star) and became denser.

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5
Q

What is a protoplanetary disc?

A

A rotating flat gaseous cloud that was created due to the collapse of the solar nebula.

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6
Q

What occurred as a result of the heat and high density occurring at the centre of the protoplanetary disc?

A

It triggered nuclear fusion, increasing the temperature of the surface of the star at the centre of the protoplanetary disc.

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7
Q

What is meant by the term accretion?

A

An increase in mass by the addition of material e.g. by rocky particles colliding.

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8
Q

What is a planetesimal?

A

A small body of rocky material that has been created by gravitational and electrostatic forces. They are around 1 km in diameter.

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9
Q

What is a protoplanet?

A

It forms when planetesimals accrete (join together). They are approximately the size of the moon.

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10
Q

Approximately how long did it take for protoplanets to collide and form the terrestrial planets?

A

Up to 1 billion years.

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11
Q

Why did giant gas planets form in the outer reaches of the solar system?

A

They formed from the less dense elements that was sent further away from the sun when it collapsed and produced a shockwave.

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12
Q

What are asteroids?

A

The left over planetesimals that did not form planets.

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13
Q

What are meteorites?

A

Fragments of asteroids.

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14
Q

How did the moon form?

A

A protoplanet impacted the young Earth between 30 and 50 million years after the formation of the Solar System.

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15
Q

What assumption do we have to make in order to use meteorites as evidence for the Earth’s composition and structure?

A

All the material in the Solar System originated from the same source.

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16
Q

What feature do meteorites have that means that can be used as a record of planet formation?

A

The have remained unaltered since they were formed.

17
Q

What is the evidence for the solar nebular hypothesis?

A
  1. The rocky planets are closest to the Sun and the gas giants further away
  2. Most solar system objects orbit and rotate in an organised fashion
18
Q

Which type of meteorites represent the Earth’s core?

A

iron meteorites

19
Q

What are iron meteorites composed of?

A

an alloy of iron and nickel

20
Q

Which type of meteorites represent the Earth’s mantle?

A

stony meteorites

21
Q

What are stony meteorites composed of?

A

silicate mineral including olivine, pyroxene and plagioclase feldspar

22
Q

Which type of meteorite are thought to represent the overall composition of the Earth?

A

chondrites

23
Q

What are chondrites composed of?

A

silicate minerals plus water, organic compounds, and chondrules

24
Q

What are chrondules?

A

originally molten droplets, for example of olivine, which formed at high temperatures in the early solar cloud (found in chondrite meteorites)

25
Q

Which type of meteorite is chemically similar to the Sun, except for the absence of hydrogen and helium?

A

chondrites

26
Q

State three pieces of evidence for asteroid impact.

A
  • the impact sites are circular and have a rim of broken rock built up of ejected material
  • quartz grains may be violently shocked and even melted
  • rock strata are tilted
  • material at depth is brecciated (broken up)
  • the ejected material falls back to the surface in an inverted sequence because material closer to the surface is ejected first and falls back to the surface earlier
27
Q

What is the relationship between the size of an asteroid or meteorite impact and their frequency?

A

The larger the size of the impact, the less frequent the impacts are (negative correlation).