Birth Of Earth Flashcards

1
Q

Explain nebular theory

A
  1. Solar nebula formed
  2. Gravity contracted solar nebula
  3. Material collected in center
  4. condensation sparked nuclear fusion to create photosun
  5. Remains formed rotating disk
    - matter cooled and condensed into icy, rocky stuff that collided to form planetismals
  6. Collisions and accretion formed protoplanets
  7. Protoplanets accumulated most of the debris in their orbit to be planets
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2
Q

Solar nebula definition

A

Rotating cloud of interstellar gases (helium and hydrogen mainly) and dust

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3
Q

How did the moon form?

where did most of its mantle and core come from?

A

collision w/ a Mars-sized body
Ejected material was caught in Earth’s orbit and eventually formed the moon
* with most of its mantle coming from the impactor and its core from the Earth

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4
Q

Why do scientists use meteorites to determine the age of the Earth?

composition of meteorites
what do they represent
indication of surface

A

irons, stony materials, iron-stony represent composition of terrestrial planets
Earth has more iron and nickel than what surface rocks indicate

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5
Q

What protects Earth from solar wind? How? what phenomenon is this?

A

Magnetosphere - solar winds goes through the poles—> northern and southern lights

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6
Q

What led to the four seasons?

A

Tilt of earth from mars-sized body

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7
Q

What special type of rock formation did reactions between oxygen and the iron rich ocean produce?

A

Banded iron formations

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8
Q

Relative mass of Terrestrial planets vs Jovian planets

A

Terrestrial: less than 1 (earth=1)
Jovian: more than 1

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9
Q

Number of satellites of terrestrial planets vs number of satellites of Jovian planets

A

Terrestrial: few
Jovian: many

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10
Q

Inclination of orbit of terrestrial planets vs Jovian planets

A

Terrestrial: larger (earth=0)
Jovian: smaller

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11
Q

Polar flattening definition and terrestrial vs Jovian

A

Measure of how squished a planet is from north to South Pole

Terrestrial: smaller
Jovian: larger

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12
Q

Planetismals composition (inner planetismals)

temp

A

Metals and rocky substances, stuff with high melting temperatures

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13
Q

Planetismals composition (outer planetismals) accumulation of this led to

what did it have small amounts of

A

High percentages of ices - water, co2, ammonia, and methane, small amounts of rocky and metallic debris

Large size and low density

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14
Q

Period of revolution definition aka
Terrestrial vs Jovian

A

How long it takes for a planet to go around the sun

Orbital period

terrestrial: shorter
Jovian: longer

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15
Q

Orbital velocity definition
Terrestrial vs Jovian

A

Speed a planet moves on it revolution
terrestrial: faster
Jovian: slower

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16
Q

AVG density terrestrial vs Jovian
How is density measured?

defintion of density

A

Terrestrial: much larger than 1
Jovian: cluster around 1

Weight per unit volume (g/cm^3)

17
Q

Diameter of Terrestrial vs Jovian

A

Terrestrial: thousands of miles
Jovian: tens of thousands of miles

18
Q

Period of rotation meaning
Terrestrial vs Jovian

A

How long it takes to rotate around axis (how long a day is for that planet)

Terrestrial: longer (days)
Jovian: shorter (hours)

19
Q

Interiors of terrestrial planets

core
mantle
crust

A

large cores of iron and nickel
Rocky mantle and crust

20
Q

Why does Earth have a strong magnetic field?

A

core is hot enough to undergo convection and rapid rotation

21
Q

Interior of the Jovian planets

core
layers above core for jupiter and saturn, & uranus and neptune

A

small, rocky/iron core

Jupiter and Saturn: liq. metallic hydrogen (electric currents), liq. molecular hydrogen, gaseous hydrogen/helium, visible clouds

Uranus and Neptune: ices (water/methane), gaseous hydrogen/helium, visible clouds

21
Q

Atmosphere of terrestrial planets vs jovian

A

terrestrial: co2 and nitrogen, thinner
jovian: thicker, hydrogen and helium

22
Q

Where do airless bodies develop?

A

warm surface temperatures and weak gravities bc gas particles move faster and don’t stay around bc it can escape gravity

23
Q

where did the outer planets form? and how was this related to solar heating?

A

temps are low and minimal solar heating allowed gases to condense into ices

24
Q

what are asteroids? size of debris

A

piles of rubble where fine debris concentrates in in low areas and is surrounded by large boulders

25
Q

what are comets?

A

collections of rocky material, dust, water ice, and frozen gases

26
Q

where do meteors originate from

A

debris missed by the sweep of planets during formation, asteroid belt, or comets

27
Q

where did earth’s water come from

A

asteroids that jupiter sent to earth