GEL 001 Midterm 1 Flashcards

1
Q

Solar nebula hypothesis

A

Plants form from discs of gas and dust that surrounded the sun as it formed.
Planets are byproduct of star formation from nebula.

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2
Q

Nebula

A

Clouds of gas and dust in space that Mark birthplace of stars

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3
Q

Solar system

A

Begin with slow, spinning cloud of gas, nebular cloud begins in collapse and toward center, because of gravity
As it collapse It heats up and compresses the center (proto-sun) revolving gas and dust become trapped and stable orbits (rings)
When’s sons internal fusion? Reactor turns on a become real son, and rings matter, clumps as temps drop, planetestimals become planets.

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4
Q

Planetestimals

A

Constant collisions caused Boulder
Astreoid size particles coalesce because of Gravity

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5
Q

Accretion

A

Collision growth of planets by constant bombardment

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6
Q

4.6 b.y age of Earth

A

Formation of sun, 8 planets, over 130 mins, and assorted space debris —> Determined by dating of radioactive elements within meteorites found on earth

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7
Q

Meteorites

A

Chunks of rock metal that fall to earth from space

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8
Q

Differentiation

A

Planets, evolved by progressive differentiation (separation) of materials, according to
density,
under the influence of internal heating,
heavy moved to core

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9
Q

Core

A

Dense interior, in planets

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10
Q

Mantle

A

Surrounds core, less dense

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11
Q

Crust

A

Thin, least dense

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12
Q

Hydrosphere

A

Surface water on earth, along with ground water

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13
Q

Atmosphere

A

Develops from for volcanic gas

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14
Q

Heat of formation

A

Frictional heating through constant collision, (kinetic energy of informing matter converts to heat energy)

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15
Q

radioactive heat

A

Accumulation of U, Th, K, that spontaneously Decay to form heat

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16
Q

Magma ocean

A

Young earth was hot enough for the uppermost several tens of kilometers to covered by magma ocean

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17
Q

Hadean Era

A

Magma rock existing in cooling off,
unlivable period,
First 600–700 million years of earth history

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18
Q

Volcanic outgassing

A

Volcanoes emenate copious quantities of water, paper, CO2, SO2, NO2, and other gases

19
Q

Rules of comets

A

“Dirty snowball”
Contributed huge amounts of water to interior of planet,
outgasesand contributed to early atmosphere and hydrosphere

20
Q

Main elements in the Earth

A

Fe, O, Si, and Mg

21
Q

Silica & Silicates

A

Si and O Create silica (SiO2) Which is the main component of silicates. Silicates doninates the rocky mantle and crust

22
Q

Geothermal gradient

A

Rate of change in temperature with depth
Temperature increases towards the center of the Earth

23
Q

Iron inner core

A

(s), Very hot and dense, made of metallic Fe With small amounts of Ni and S

24
Q

Iron outer core

A

(l), Very hot in tents, made out of metallic Fe with small amounts of Ni and S

25
Q

Composition and characteristics of core

A

Solid inner core- pure crystalline Fe, But “frozen” At center of planet, because intense pressure
Liquid outer core- (l), Molten Fe With traces of other metals, generates Earths magnetic field, (l), Because pressure and temperature increases (the Temp melts it)

26
Q

Composition and characteristics of mantle

A

(s), Dense, ‘Silicate rock and metal oxides that are a thick(l), Behaves, like plastic, greatest volume of earth

27
Q

Composition and characteristics of crust

A

(s), thin, silicate rock that is brutal

28
Q

seismology

A

study of earthquake waves that can be analyze to discern the interior dimensions and compositions of the earth

29
Q

body waves

A

pass through interior of Earth (P and S waves)

30
Q

P waves (primary)

A

travels fastest, compresses and pull rock, can travel through (s) and (l)

31
Q

S waves (secondary)

A

slower, shears rock sideways or up/ down, only (s)

32
Q

wave paths & rays

A

seismic energy moves as series as waves and rays show direction of wave movement

33
Q

reflection and refraction

A

Seismic waves may reflect or refract (bend)

34
Q

seismic velocities

A

depends on densite and elastic properties

35
Q

crust/mantle boundary (Moho)

A

P-wave velocities that increase rapidly because of abrupt increase in densite of mantle rock realtive to crustal rock

36
Q

core/mantle boundary

A

P-wave decreases at the abrupt change from mantle to liquid outer core

37
Q

inner core/outer core boundary

A

P-velocity changes at outer-to-inner core

38
Q

shadow zone

A

Where no s-waves penetrate the liquid outer core of Earth

39
Q

seismic tomography

A

computer-aided technique that details variations in seismic velocity of materials within Earth

40
Q

Wegener

A

German meterologist/geologist; 1915 book suggested all continents combined into Pangea but then drifted into configurations of today

41
Q

Pangea

A

Super-continent that contained ALL continents that was proposed by
Wegner

42
Q

continental drift

A

criticized idea b/c no one could find a way where continents could move

43
Q

exploration of oceans

A

happened in WWIl and Cold War; helped understand continent configurations

44
Q

echo sounding

A

recording of a sound wave bounced off the ocean floor