Chapter 7 Flashcards

(16 cards)

1
Q

The fact that Earth is geologically active means…

A

It’s surface is constantly being reshaped be volcanic eruptions, earthquakes, erosion, etc

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2
Q

Interior structure

A

1) core - the highest density - in the center
2) mantle - rocky materials of moderate density - around the core
3) crust - the lowest density - visual part - forms the outer skin

+ lithosphere - Earth outer layer of cool and rigid rock (crust + upper layers of mantle)

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3
Q

Differentiation

A
  • a process by which gravity separates materials according to their density, with high density material sinking and low density materials rising—> multiple interior layers
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4
Q

Why terrestrial planets were once hot enough to melt materials to form layers?

A

1) after accretion Ep transformed into E(thermal)
2) radioactive decay released heat directly into a planetary interior, converting mass-energy (E=m*c) into E(thermal)

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5
Q

Convection

A

The energy transport process in which warm materials expands and rises while cooler materials contracts and falls (happens very slow)

How it happens: core releases heat that melts lower mantle, makes the material less dense -> it rises —> cycle

—> Magnetic field —> magnetosphere (— the region surrounding a planetary interior in which charged particles are trapped by the planet’s magnetic field (exists due to convection)) —> protects Earth shielding it from solar wind

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6
Q
A
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7
Q

What processes shape Earth’s surface?

A

1)impact cratering
2) volcanism - the eruption of molten rock (lava) from its interior to the surface — volcanic outgassing formed atmosphere and ocean
HOW: during Earth’s formation -> accretion -> rock, water and gas trapped beneath the surface -> later some were released by volcanic eruption
3) tectonics (esp planet tectonics) — disruption of a planet’s surface by interior stresses

2-3 require internal heating and therefore depend on a planet’s size

4) erosion — the wearing down and building up of geological features by water, wind, rain, snow and other phenomena of planetary weather

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8
Q

How does Earth’s atmosphere affect the planet?

A

1) greenhouse effect —> warm temperatures + water stays liquid
2) surface protection from solar radiation by absorbing X-rays in high atmosphere and ultraviolet light in the middle of atmosphere by ozone. Only visible light reaches the ground (blue light is scattered => blue color of the sky), and than remitted as infrared light

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9
Q

The Moon’s geographic features

A

— the moon’s dark, smooth Maria - lava flooded craters later after they were formed when the Moon’s interior were heat by the radioactive decay
— has water ice (from impacts from comets) (very little)
— NOW geologically dead

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10
Q

Mercury geological features

A

— NOW geologically dead (small size)
— some crater floors appear to release easily vaporized materials from the rock, causing the rock to crumble and make “hollows”
— the release of easily vaporized gases leaves behind a light-colored coating whose composition remains unknown
— water ice in permanently shadowed craters near Mercury’s poles (from impacts from comets)
— has a set of tremendous cliffs all over its surface (probably formed when tectonic forces compressed crust, causing the surface to crumble ==>==> Mercury appears to have shrunk long ago, leaving behind long, steep cliffs)

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11
Q

Mars

A

— has frozen
— more elliptical => more extreme seasons
— thin atmosphere => weakened greenhouse effect => cold
— geological evidence of past water flows: river bends/ lake bends, indistinct rims of many large craters and lack of small craters (erosed)
—the dramatic difference in Mars’s terrain around different parts of the planet
— past volcanism -> dotted with many volcanoes

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12
Q

Why did Mars froze?

A

Apparently Mars must have somehow lost its carbon dioxide (hypothesis: due to change in its magnetic field) -> weakened greenhouse effect -> lower t until the planet frozen over

+ small proportion of carbon dioxide condensed forming ice caps of Mars’s poles (polar caps) (the majority was lost in space)

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13
Q

Venus

A

— similar in size and composition to Earth but different in other ways
— geologically active
— very strong greenhouse effect — b/c of thick carbon-dioxide atmosphere — somehow lost its outgassing water (from volcanism activity) leaving carbon dioxide (hypothesis: its evaporated b/c Venus is closer to the Sun) **— gases are trapped within atmosphere—> very-very hot
— shows features of volcanism and tectonics
— no erosion b/c too hot for water and snow/ rain AND too slow (rotation) for wind and weather
— absence of planet tectonic. Instead surface is all the same age on Venus (hypothesis: b/s Venus has a thicker and stronger lithosphere)

**Earth has as much carbon dioxide but because it is mostly locked in rocks rather than in our atmosphere, we don’t have that bizarre greenhouse effect)

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14
Q

What unique features of Earth make it habitable?

A

1– surface liquid water
2– atmospheric oxygen — from photosynthesis
3– plate tectonics — act like a giant conveyor belt for Earth’s lithosphere, recycling the sea floor and building the continents (-> subduction (zones))
4– stable climate — the process of Earth self-regulating its t — carbon dioxide (CO2) cycle - the process that cycles carbon dioxide between Earth’s atmosphere and surface rock
The higher⬆️ the t = the higher⬆️ rate at which carbon dioxide is removed

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15
Q

Carbon dioxide cycle (=CO2 cycle)

A
  • the process that cycles carbon dioxide between Earth’s atmosphere and surface rock
    That’s how Earth self-regulates its t ensuring stable climate
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16
Q

The consequences of climate change

A

1- ⬆️t -> ⬆️E(total) available-> ⬆️more frequent extreme weather events
2- ⬆️⬆️the level of ocean
3- ocean more acidic