ORIGINS: Creation and Composition of the Earth Flashcards

1
Q

creation of the new solar system

A
  • derived from the death of the previous one

- star becomes supernova, destroying itself, simultaneously creating new solar system (w elements)

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2
Q

nebula to solar system

A
  • gravitational energy is converted to heat (the cold cloud warms up)
  • vapourizes all of the elements
  • heat at the center lights up the sun
  • gas/vapour blown away cools and recondenses as dust
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3
Q

Condensation of planetesimals from dust and gas

A
  • first by electrostatic forces, then by gravity

- elements interact, sharing and donating electrons

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4
Q

rocky vs gas vs ice rich planets

A
  • planets forming close to the sun are rocky
  • planets condensing far from the sun are gas & ice rich
  • the planets comprised of heavier elements (rocks) are (terrestrial planets) did not travel as far
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5
Q

half-finished Earth (10-100MYA)

A
  1. Earth bombarded by millions of smaller bodies (meteors and comets)
  2. bombardment heated the Earth (collisions)
  3. heating increased by gravitational contraction
  4. melting of Earth creating magma ocean. Iron-rich fraction of this liquid was heavier and it settled to Earth’s centre
    * this melting drove off H, He- rich primordial atmosphere
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6
Q

Earth 4.4 Ga (billion years)

A
  • solid core (iron-rich)
  • ‘outer core’ of liquid iron
  • partly molten ‘mantle’
  • thin skin of solid rock at its surface
  • too hot for liquid water
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7
Q

Jupiter and Saturn atmosphere

A

-close to the frost line

  • gas giants as a result of no hot melting event
  • retain a “primordial” atmosphere
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8
Q

uranus and neptune

A
  • light gases turned to ice
  • made of mostly ice
  • same composition as Jupiter and Saturn but at much lower temperature
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9
Q

ontology of Earth’s Moon

A
  • collision between large body and Earth
  • moon grew from ejected material of this collision
  • initially closer to the Earth
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10
Q

on a moonless Earth:

A
  • tides would be solar and less powerful
  • days would be shorter
  • faster winds
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11
Q

Igneous Rocks

A
  • “fire formed:” cooled from liquid
  • the most accurate to date
  • basalt, granite
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12
Q

sedimentary rocks

A
  • tell us about relative order in which events occurred

- formed from chemical precipitates or fragments of earlier formed rocks

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13
Q

metamorphic rocks

A

-formed by application of heat and pressure to either igneous or sedimentary rocks

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14
Q

radioactive decay

A
  • useful until about 6 half lives

- measures proportions of parent and daughter isotopes of an element in SEVERAL samples

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15
Q

age of the moon

A
  • Earth’s major structures were established prior to the birth of the Moon
  • BC an impact on Earth that did not have a separate Fe-rich core would have contributed more Fe to the moon
  • by 4.4 Ga Earth and Moon were already a pair
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16
Q

Bombardment of Earth and the Moon today

A

-prevented by LARGE Jupiter

17
Q

differences between the Earth and the Moon

A
  • both heavily bombarded, yet the Moon has many more craters
  • this is bc the moon is too small to hold a dense atmosphere
  • also cooled much more rapidly, now has no volcanic activity and is lifeless
18
Q

Earth’s early atmosphere came from

A
  • impact degassing (comets, bolides vapourizing)
  • volcanic activity (gases released from magma)
  • comets brought H2O, CO2, NH3 and many more building blocks of life, but could NOT bring O2 gas to the atmosphere