Test 1 Flashcards

1
Q

what is geology? (4)

A

Geology is the study of Earth’s physical structure, history, substance and processes that have acted on it

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2
Q

what is comparative geology?

A

It is the study of how we compare different planets of the solar system and observe their similarities and differences that they have towards Earth.

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3
Q

Definition of a planet

A

A celestial body that
-orbits the Sun
-Has enough mass to maintain hydrostatic equilibrium
-must be able to clear it’s neighborhood

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4
Q

name the planets of our solar system in order

A

-Mercury
-Venus
-Earth + Moon
-Mars
-Astroid Belt
-Jupiter
-Saturn
-Uranus
-Neptune

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5
Q

what is a dwarf planet?

A

It is a body that doesn’t satisfy the rule that a planet needs to clear it’s neighborhood. Like Pluto, Pluto doesn’t have enough sufficient mass to clear it’s neighborhood.

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6
Q

Name 5 dwarf planets

A

-Pluto
-Eris
-Ceres
-Haumea
-Makemake

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7
Q

Definition of a moon

A

A natural satellite that orbits around a celestial body or a body that is not a star

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8
Q

Where are we in the universe?

A

The Milky Way Galaxy

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9
Q

What happened after the Big Bang?

A

The Dark Ages began. There was no light because there was no stars.

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10
Q

How did our S.S form?

A

The Nebular Hypothesis

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11
Q

What is the 4 main processes of the Nebular Hypothesis?

A

-A cloud of matter (nebula) began to contract at the center giving us our protosun
-at high temps, nebula flattens into disk by nuclear fusion (H fuses with He, light and energy)
-Dust and ice accumulate around it and clump together forming planetesimals. Protoplanetary disk is formed by cloud differentiation and accretion
-Planetesimals grew into planets. They cleared their orbit by gravitationally attracting or ejecting other planetesimals.

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12
Q

What is cloud differentiation?

A

-The heavier elements such as dense rocky elements would condense closer to the Sun
-The gaseous elements would condense in the outer part of the planetary disk.

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13
Q

What is accretion in terms of the nebular hypothesis? (Think of how the solar system is organized)

A

It’s when larger planetesimals would pull and attract smaller ones

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14
Q

Evidence for the Nebular Hypothesis?

A

The chemistry of the Sun and it’s elements

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15
Q

What are the main processes of the planetary evolution?

A

After Accreted, planets and moons evolved to…
-Melting and differentiation of elements
-volcanism
-planetary mass
-distance from the Sun
-Presence of biosphere

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16
Q

What is the formation of Terrestrial Planets? (3)

A

-Accretion: Planets bang into each other or other bodies and heat up
-Differentiation: The internal structure splits into categories. The metallic towards the core and the low-density magma towards the crust
-Stratification: Zones of different elements–> creating minerals—> creating rocks

17
Q

Basic Internal structure of Earth?

A

-Crust (litho & asthenosphere)
-Mantle (solid)
-outer core (liquid)
-inner core (solid because of pressure)

18
Q

Hubble space telescope’s goal

A

to measure the distance of our galaxy

19
Q

OSIRIS-REx mission

A

To collect samples of asteroid Bennu and bring back to Earth (sample return mission)

20
Q

Key observations of densities of planets: (4)

A

-They inform about composition
-Reflect rocks and metals
-Terrestrial = silicate planets
-Density increases as you move from crust –> inner core

21
Q

What are the terrestrial planets made up of?

A

-Minerals, rocks, metals, volatiles

22
Q

Which are denser? Volatiles, sillicates, metals?

A

1-metal
2-sillicate
3-volatile

23
Q

What is the importance of
Si + O?

A

They make up the crust (rocks)

24
Q

Why is there less iron in the crust?

A

Because due to differentiation, denser elements (like Fe) migrate towards the inner core

25
Q

what is planetary differentiation?

A

the split of the planets structure
- the heavier elements will migrate towards the core and the loghter will migrate towards the crust through accretion

26
Q

what are the planetary heat sources?

A

1-Accretion (planets bang into each other)
2-Differentiation and crystalization of metal core
3-Radioactive decay (isotopes supply heat)

27
Q

how do planets cool down?

A

volcanoes

28
Q

what does the cooling rate depend on for planets?

A

the size, smaller planets cool down faster

29
Q

4 main processes affecting planetary surfaces?

A

-Impact cratering
-volcanism
-Tectonics
-Weathering erosion

30
Q

What does impact cratering cause?

A

circular shock waves

31
Q

What does impact cratering mean?

A

comets, asteroids, meteorites hit planets

32
Q

Key features of Mercury

A

-closest to sun
-smallest
-heavily-cratered
-no tectonic plates
-no moons
-no liquid water
-no winds
-no atmosphere

33
Q

Internal structure of Mercury?

A

-crust
-solid mantle
-central core

34
Q

what is the main mission of Mercury?

A

-MESSENGER
They found water ice in shadowed-craters

35
Q

What’s Mercury’s orbit and rotation type?

A

-excentric orbit and 1 rotation takes 59 days

36
Q
A