Midterm 1: 1-5 Flashcards

(74 cards)

1
Q

According to the Giant Impact Hypothesis, how did the moon form?

A

The Moon formed approximately 4.5 billion years ago when a Mars-sized impactor struck the young Earth. The impact blasted mantle material from both bodies into orbit and formed a ring around the Earth, which eventually condensed to create the Moon.

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2
Q

What evidence in the rock record supports the link between the K-T impact and the Chicxulub Crater?

A

Elevated levels of iridium (rare on Earth but common in meteorites) & shocked quartz (formed only under extreme pressure of an impact)

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3
Q

What geological evidence identifies the K-T impact as a significant event in Earth’s history?

A

The K-T impact is marked in the rock record by iridium levels 10 to 100 times higher than typical Earth levels, as well as the presence of impact-derived materials like shocked quartz and tektite spherules.

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4
Q

Why is the Hadean Eon described as the “hellish” era of Earth’s history?

A

Named after the Greek word for “hell,” the Hadean Eon (4.56–4 Gya) was characterized by frequent volcanic eruptions and heavy impacts. It represents the earliest stage of Earth’s history, and conditions were so extreme that no rocks from this period have survived to the present day.

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5
Q

Which time period is characterized by the highest frequency of impacts in Earth’s history?

A

Early Bombardment

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6
Q

Why is it unlikely that Earth acquired its water during its initial accretion phase?

A

Earth formed inside the “water ice snow line” where temperatures were high enough that water existed only as a gas. Because Earth was not massive enough to accrete large amounts of gas, it is more likely that water was delivered later by ice-rich small bodies from the outer solar system. Also, at Earth’s orbital location, rock & metal would have been in solid form while water would have been in gaseous form.

Earth acquired water after formation.
There were lots of impacts in the early solar system. Isotopic analyses show that most of Earth’s water was delivered by small bodies that originated in the outer regions of the asteroid belt, but comets likely contributed as well.

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7
Q

What was the “Great Oxidation Event,” and which eon did it occur in?

A

The Great Oxidation Event occurred during the Proterozoic Eon, approximately 2.4 to 2 billion years ago. During this time, atmospheric oxygen levels rose dramatically due to the emergence and activity of oxygenic photosynthesis.

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8
Q

Why does the presence of Zircons dating back to 4.4 Gya suggest the Hadean Earth might have been ‘calm’ at times?

A

They provide evidence for the existence of early oceans & continents

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9
Q

In the context of geological time, the ‘Precambrian’ refers to what percentage of Earth’s total history?

A

88% (Hadean, Archean, Proterozoic)

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10
Q

What is the primary chemical difference between Earth’s secondary atmosphere and its current atmosphere?

A

The secondary atmosphere was dominated by carbon dioxide and lacked free oxygen. It formed via volcanic outgassing of gases trapped in the Earth’s interior.

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11
Q

Why does the ‘Gow Crater’ in Saskatchewan appear much less defined than the ‘Meteor Crater’ in Arizona, despite being larger?

A

It is significantly older & has been subject to more erosion

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12
Q

Based on Kepler’s Second Law, how does a planet’s orbital speed change relative to its distance from the Sun?

A

Kepler’s Second Law establishes that a line connecting a planet to the Sun sweeps out equal areas in equal time intervals. This implies that a planet must move faster when it is closer to the Sun (covering more orbital distance to sweep the area) and slower when it is further away.

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13
Q

Explain the fundamental difference between Kepler’s work and Newton’s work regarding planetary motion.

A

Kepler’s Laws are descriptive, determining “how” planets move based on observational data. Newton’s Laws provided the physical explanation or the “why” behind that motion by introducing the concepts of inertia, force, and gravity.

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14
Q

What is Newton’s First Law (law of Inertia)?

A

An object at rest will remain at rest and an object in motion will remain in motion in a straight line at a constant speed unless acted upon by an external force

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15
Q

What is Newton’s Second Law?

A

The net force acting on an object is proportional to an object’s mass & its resultant acceleration

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16
Q

What is Newton’s Third Law?

A

For every action there is an equal and opposite reaction

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17
Q

What is Newton’s Law of Universal Gravitation?

A

Objects attract each other with a force that is directionally proportional to the product of their masses & inversely proportional to the square of the distance between them

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18
Q

What is Kepler’s First Law?

A

A planet orbits the Sun in an ellipse, with the Sun at one focus of the ellipse

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19
Q

What specific detail of lunar composition supports the Giant Impact Hypothesis?
What are other observations?

A

It resembles Earth’s mantle.

others:
- moon is receding from Earth
- moon is in a “regular” orbit
- moon is massive compared to Earth
- moon was completely molten roughly 4.5 Ga ago

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20
Q

What were the two primary components of Earth’s atmosphere during the Archean Eon?

A

Nitrogen & CO2

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21
Q

Mercury has an extremely tenuous atmosphere known as what?

A

An exosphere

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22
Q

During the formation of a solar system, why does a collapsing molecular cloud flatten into a spinning disk?

A

Due to the conservation of angular momentum. As the cloud collapses and its radius decreases, it must spin faster to conserve angular momentum, naturally flattening into a disk shape.

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23
Q

Define “periastron” and “apoastron” in the context of orbital velocity.

A

Planets move most quickly when they are near the periastron (the point closest to the star). Conversely, they move most slowly when they are near the apoastron (the point farthest from the star).

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24
Q

What is the semimajor axis of an ellipse?

A

Half of the long side of the ellipse

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25
According to the planetary formation theory provided, what is the role of gravity in the initial stage?
Gravity provides the inward force that overcomes internal pressure, leading to the contraction of the molecular cloud.
26
What is the distance light travels in a single year, and how far away is Proxima Centauri in light-years?
A light-year is the distance light travels in one year, which is 9×10^15 meters. The nearest star other than the Sun, Proxima Centauri, is located 4.2 light-years away from Earth.
27
How does the "snow line" determine the composition of planets forming in a spinning disk?
The snow line is the boundary where the disk is cold enough for water and other volatiles to become solid. Rocky planets form inside this line where only rocks and metals are solid, while giant planets form beyond it.
28
How has the North American continent changed in size over geological time?
North America has grown outward over time as various "terranes" were added along its edges. The interior rocks are the oldest (often >2.5 billion years), while coastal areas like California are geologically young (<0.6 billion years).
29
Where is the oldest oceanic crust located, and how does oceanic crust generally compare in age to continental interiors?
The oldest oceanic crust is found in the Mediterranean and the eastern/western edges of the North Atlantic. Generally, oceanic crust is much younger than the interiors of continents, which contain the oldest crustal material.
30
Identify the differences between the three isotopes of Hydrogen: Hydrogen, Deuterium, and Tritium.
All three have one proton, but different neutron counts: Hydrogen has zero neutrons, Deuterium has one neutron, and Tritium has two neutrons. Tritium is the heaviest of the three isotopes.
31
How do geologists study the first 500 million years of Earth's history given the lack of intact rocks from that period?
Using radiometric dating on tiny remnants (like zircons) and older rocks from elsewhere in the solar system.
32
Define 'radioactivity' based on nuclear physics.
The emission of ionizing radiation resulting from the decay of an unstable atomic nucleus.
33
What type of radioactive decay involves the emission of a helium-4 nucleus?
Alpha decay
34
What type of radioactive decay involves the emission of an electron?
Beta decay
35
Which radioactive decay process involves the emission of high-energy photons without changing the number of protons or neutrons?
Gamma decay
36
What determines whether a planet will be primarily rocky or gas-rich during its formation relative to the snow line?
The local temperature of the disk, which determines which materials can solidify into 'seeds' for planet growth.
37
How does the Rock Cycle tell us how zircons ended up in younger rocks?
- Ancient igneous rocks formed - those rocks were weathered - the rocks eventually broke apart into tiny grains - those tiny grains were transported, buried, and compacted - after a long time, the material in which the grains were buried was so compacted it became sedimentary rock
38
How do you use radiometric dating to determine the age of the solar system?
1. Radiometric dating of Zircons 2. Radiometric dating of Moon rocks (they're over 4.4 billion years old & the moon formed after the Earth so it has to be at least that old). 3. Radiometric dating of Meteorites (~4.57 billion years old)
39
What is a meteor? What is a meteorite?
Tiny solid particle that enters Earth's atmosphere from interplanetary space; "shooting stars" Meteor that survives trip through Earth's atmosphere
40
What is the primary nuclear fusion process occurring in the cores of stars while they are on the main sequence?
Hydrogen into Helium
41
Which event is responsible for the production of the universe's original hydrogen and helium?
The Big Bang
42
A solar mass star eventually ends its life by producing which type of stellar remnant?
white dwarf
43
What is the heaviest element produced by fusion in the core of the most massive stars just before they collapse?
Iron
44
Describe the "onion-shell" structure found in evolved massive stars. In the 'onion-shell' structure of an evolved massive star, where is the hydrogen-burning shell located?
As massive stars exhaust their hydrogen, they begin fusing heavier products into successively denser elements in layers. This creates an onion-shell structure where the core can produce elements as heavy as iron, while lighter elements remain in the outer layers. The outermost shell
45
What is the primary reason that most artistic graphics of the solar system are considered 'misleading' according to the source material?
They do not show objects & distances to scale
46
Which zone of the solar system contains more than 99% of its total mass?
The Sun
47
How do the 'Ice Giants' compare to the 'Gas Giants' in terms of mass and radius relative to Earth?
Ice Giants (Uranus & Neptune) have smaller radii and smaller masses
48
What is an observed clue that supports the Nebular Theory of planet formation? Which two planets are noted as 'exceptions' because their spin direction differs from the others?
Planets orbit in the same flat plane. Exceptions: Venus (spins backwards) & Uranus (spins on its side)
49
What physical principle explains why a collapsing interstellar cloud begins to spin faster as its size decreases?
Conservation of Angular Momentum
50
The 'snow line' in our solar system, which separates rocky planets from those containing ice and gas, is located at approximately what distance from the Sun?
3 AU
51
Explain Planetary Embryo Formation & Runaway Growth
During the formation of planetary embryos, planetesimals—ranging from centimeter to kilometer sizes—collide and fragment and grow. Runaway growth occurs when larger embryos begin to accumulate mass and grow much faster than smaller embryos, eventually dominating their region of the disk. The largest embryos grow to become protoplanets
52
What describes the 'Infall Stage' of planetary disk formation?
Molecular cloud collapses due to gravity. Protostar & disk start to form. Conservation of angular momentum causes them to spin.
53
How does a star's initial mass determine its evolutionary path and lifespan?
Initial mass is the strongest influence on stellar evolution, determining both a star’s main-sequence lifetime and its final form. Less massive stars have longer lifetimes and end as white dwarfs, while more massive stars have shorter lives and end as supernovae, leaving behind neutron stars or black holes.
54
What happens to a solar-mass star once it exhausts the hydrogen in its core?
After the main sequence, a solar-mass star begins fusing helium to produce carbon and oxygen. Because these stars do not become hot enough to fuse these heavier products further, they eventually transition into white dwarfs after passing through stages such as the red giant and planetary nebula phases.
55
What are the primary zones of the solar system, moving outward from the center?
The solar system is organized into distinct zones starting with the Sun, followed by the inner terrestrial planets and the asteroid belt. Moving further out, there are the outer gas and ice giants, the Kuiper Belt, and finally the Oort Cloud at the farthest reaches.
56
How does the "snow line" influence the composition of planets during formation?
Inside the snow line (hotter than 0°C), only rocks and metals can condense because it is too hot for gases like hydrogen and helium to stick to solid surfaces. This explains why only rocky terrestrial planets are found within 3 AU of the Sun, while gas and ice-dominated worlds form further out.
57
According to Nebular Theory, what was the origin of the Sun and the planets? What are key observations explained by this theory?
Nebular Theory posits that the Sun formed at the center of a flattened protoplanetary disk composed of gas and dust. The planets subsequently formed from the material within this disk, with their mass and composition determined by the specific materials available in their region of the disk. observations: 1. Sun spins in the same direction as the planets orbit 2. Planets have (nearly) circular orbits 3. Planets orbit in the same flat plane 4. Planets mostly orbit & spin in the same direction (mostly counterclockwise as viewed from 'above')
58
What is main-sequence?
Main phase of a star's life in which it fuses. While on the main-sequence, stars fuse hydrogen into helium in their cores. When they run out of hydrogen in their cores, post-main-sequence evolution begins.
59
How was hydrogen & helium produced?
Big bang nucleosynthesis
60
How was carbon & nitrogen produced?
Dying low-mass stars
61
How was oxygen, phosphorus & sulfur produced?
Dying high-mass stars
62
What determines a stars main-sequence lifetime & its evolutionary path?
the initial mass of a star. less massive stars have longer main-sequence lifetimes.
63
What will be the evolution of our Sun?
protostar -> main-sequence star -> red giant -> planetary nebula -> white dwarf
64
What are the final two elements produced by fusion in solar mass stars before they cease fusion?
carbon & oxygen
65
Why are solar mass stars unable to fuse elements heavier than carbon and oxygen?
They do not achieve high enough internal temperatures.
66
What is the heaviest element that the most massive stars can produce through core fusion?
iron
67
What are the clues about planet formation from the solar system?
1. Planets are much less massive than the sun 2. Planets have (nearly) circular orbits 3. Planets orbit in the same flat plane 4. Planets mostly orbit & spin in the same direction (mostly counterclockwise as viewed from 'above')
68
Explain Planetesimal Formation.
The protoplanetary disk is established & becomes flat. The disk is significantly less massive than the star. Planetesimals form, collide, fragment, grow to com-km sizes & settle to the midplane of the disk. Planetesimals drift radially based on size.
69
Stars are powered by nuclear fusion. What does that mean? What is fission?
Fusion: Lighter particles are "fused" together to form heavier particles. Fission: heavier particles are split apart into lighter particles
70
What is binding energy?
The amount of energy that would be released if the nucleus were broken apart into protons & neutrons.
71
How do cosmic ray collisions create elements?
Cosmic rays are fast moving-particles. B/c they move so fast, cosmic rays have lots of energy. When a cosmic ray collides with an atom, it can split it into light atoms like lithium, boron, & beryllium
72
What is astrobiology?
The study of the origins, evolution, distribution & future of life in the universe. AKA: exobiology, xenobiology, bioastronomy
73
Whats the scientific method?
Make observations -> ask a question -> suggest a hypothesis -> make a prediction -> test the hypothesis
74
What are the key questions in Astrobiology?
1. How does life begin? 2. What conditions are needed for life to survive? 3. Do habitable environments exist elsewhere in the universe? 4. What is the diversity of life in the universe?