Lecture 2 - Week 1 - Origin of the Earth Flashcards

1
Q

Describe Hubble’s Law in 6 words?

A

Objects in space are moving apart.

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2
Q

What is the evidence of objects moving apart?

A

Redshift

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3
Q

Hubble’s Law supports the Big Bang because…

A

If objects are moving apart, they
must have started together at a
single point.

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4
Q

Big Bang Nucleosynthesis is considered responsible for…

A

The creating of some forms of hydrogen, helium and some lithium.

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5
Q

Stellar Nucleosynthesis creates elements by…

A

The super heating of elements that makes up the star.

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6
Q

In Stellar Nucleosynthesis, combining nucleons of this gas [ __________ ] with other elements (carbon, oxygen, neon, etc.) = magnesium, silicon, sulphur, calcium, iron, etc.

A

Helium

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7
Q

_________ are stellar nurseries. Stars form by collapse of parts of an individual __________.

A

Nebulae. Nebula.

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8
Q

Basic nucleosynthesis is…

A

The creation of nuclei from existing nucleons

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9
Q

Galactic Nucleosynthesis is when…

A

Cosmic rays collide with heavier atoms and create new forms of matter (this occurred in the moments after the BB)

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10
Q

When did the big bang occur?
How long after did the first stars form?
When did our solar system form?

A
  • Big bang: 13.8 billion years ago
  • First stars formed 200-400 million years after the BB
  • Our solar system forms 9 billion years after BB
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11
Q

How do stars form from nebulae?

A
  • Clouds are very large, very cold, very dense
  • Combination means that clumps tend to collapse under own weight (gravity)
  • Clumps = cores where new stars are forming
  • Collapse (shrink)> higher density> higher gravity> collapse> higher density….and so on
  • Eventually core ignites
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12
Q

What is an a accretionary disk?

A

A rotating disk of matter formed by accretion around a massive body due to gravity.

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13
Q

What are two formations in intermediary stage between the accretionary disk and the formation of a solar system?

A

The core of the disk becomes a protostar. Around the protostar is a disk of dust, gas, and other elemental matter known as a protoplanetary disk.

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14
Q

The matter in the ____________ sticks to each other to form clumps known as ____________.

A

Protoplanetary disk. Planetismals.

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15
Q

Eventually, after planetismals keep accreting material due to gravity, they become ____________.

A

Protoplanets.

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16
Q

Once they become large enough, the protoplanets become full-fledged ________.

A

Planets.

17
Q

When the Earth became a planet, the heat from meteor bombardment caused it to melt. The liquified elements allowed…

A

Heavier elements to shift towards the center. And lighter elements to shift towards the surface.

18
Q

The characteristics of the Earth’s physical layers are determined by heat and pressure… Therefore, the core is _______ and made of ______, even though it is very hot.

A

Solid. Metal: Iron.

19
Q

What is the outer core made of?

A

Molten. Metal: Liquid iron and nickel.

20
Q

What is the mesosphere?

A

Hot, solid, rock. Too much pressure for liquid rock to form.

21
Q

What are the two characteristics of asthenosphere (upper mantle)?

A

Weak and plastic.

22
Q

What is lithosphere (uppermost mantle and crust)?

A

Strong and rigid.

23
Q

How old is Earth believed to be?

A

4.6 Billion

24
Q

How old are the oldest rocks on Earth?

A

4.031 Billion years old

25
Q

How old are the oldest minerals on Earth?

A

4.4 billion years old: zircons from a sandstone found in the Jack Hills of Australia

26
Q

How do we know the Earth is 4.6 billion years old
when no rocks and minerals on our planet are older
than 4.4 billion years old?

A

Radiometric dates derived from meteorites during the Late Heavy Bombardment

27
Q

When did the Late Heavy Bombardment end?

A

Aprox. 3.9 BYA