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.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
2
Q

Nebula

A

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

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
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.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
4
Q

Planetestimals

A

Constant collisions caused Boulder
Astreoid size particles coalesce because of Gravity

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
5
Q

Accretion

A

Collision growth of planets by constant bombardment

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
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

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
7
Q

Meteorites

A

Chunks of rock metal that fall to earth from space

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
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

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
9
Q

Core

A

Dense interior, in planets

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
10
Q

Mantle

A

Surrounds core, less dense

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
11
Q

Crust

A

Thin, least dense

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
12
Q

Hydrosphere

A

Surface water on earth, along with ground water

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
13
Q

Atmosphere

A

Develops from for volcanic gas

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
14
Q

Heat of formation

A

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

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
15
Q

radioactive heat

A

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

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
16
Q

Magma ocean

A

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

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
17
Q

Hadean Era

A

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

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
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
Composition and characteristics of core
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
Composition and characteristics of mantle
(s), Dense, 'Silicate rock and metal oxides that are a thick(l), Behaves, like plastic, greatest volume of earth
27
Composition and characteristics of crust
(s), thin, silicate rock that is brutal
28
seismology
study of earthquake waves that can be analyze to discern the interior dimensions and compositions of the earth
29
body waves
pass through interior of Earth (P and S waves)
30
P waves (primary)
travels fastest, compresses and pull rock, can travel through (s) and (l)
31
S waves (secondary)
slower, shears rock sideways or up/ down, only (s)
32
wave paths & rays
seismic energy moves as series as waves and rays show direction of wave movement
33
reflection and refraction
Seismic waves may reflect or refract (bend)
34
seismic velocities
depends on densite and elastic properties
35
crust/mantle boundary (Moho)
P-wave velocities that increase rapidly because of abrupt increase in densite of mantle rock realtive to crustal rock
36
core/mantle boundary
P-wave decreases at the abrupt change from mantle to liquid outer core
37
inner core/outer core boundary
P-velocity changes at outer-to-inner core
38
shadow zone
Where no s-waves penetrate the liquid outer core of Earth
39
seismic tomography
computer-aided technique that details variations in seismic velocity of materials within Earth
40
Wegener
German meterologist/geologist; 1915 book suggested all continents combined into Pangea but then drifted into configurations of today
41
Pangea
Super-continent that contained ALL continents that was proposed by Wegner
42
continental drift
criticized idea b/c no one could find a way where continents could move
43
exploration of oceans
happened in WWIl and Cold War; helped understand continent configurations
44
echo sounding
recording of a sound wave bounced off the ocean floor