Lesson 2 Flashcards

1
Q

Explain the Rare Earth Hypothesis

A

Rare Earth Hypothesis: complex life needs a “Goldilocks” planet like Earth (stable star, right size, liquid water, etc.). These conditions are likely rare, making Earth and complex life uncommon

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

Explain Climate change, and what causes it.

A

Climate change describes long-term shifts in temperature and weather patterns across the globe. These changes are largely caused by human activities, primarily greenhouse gas emissions and other human activities such as deforestation and land use.

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

Explain the Montreal Protocol

A

The Montreal Protocol, signed in 1987, is a global agreement that successfully tackled the thinning ozone layer. It phased out harmful chemicals like chlorofluorocarbons (CFCs) used in refrigerants, aerosols, and more. By uniting nations, this treaty has allowed the ozone layer to gradually recover, protecting us from harmful ultraviolet radiation.

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

Describe a dwarf planet and give an example

A

“A dwarf planet is a celestial body that orbits the sun, is spherical in shape, but has not cleared its orbital path of other debris like a planet. They are smaller than planets but larger than typical asteroids or comets. An example of a dwarf planet is Pluto, located in the Kuiper Belt beyond Neptune.”

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

Explain the nebular hypothesis

A

dust. As gravity caused the cloud to condense, it flattened into a disk shape, leading to the formation of planets, moons, and other celestial bodies within this disk around a central mass, which became the Sun.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
6
Q

Will the Universe continue to expand forever?

A

The future of the universe can totally be predicted if only we know the total of matter it contains.

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

Discuss the difference between blue giants and red giants.

A

Blue giants are massive, hot stars in the late stages of their evolution, characterized by their high surface temperatures and blue-white color. They burn through their nuclear fuel quickly, leading to shorter lifespans compared to red giants. In contrast, red giants are cooler, larger stars that have exhausted their core hydrogen, causing them to expand and cool down, leading to their characteristic red hue.

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
8
Q

Explain the abundances of the elements

A

H and He are the most abundant. Abundances of the first 50 elements decreases exponentially. Atomic numbers greater than 50 are very low. Elements having even atomic numbers are more abundant than of odd (Oddo-Harkins Rule)

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

How has the abundance of hydrogen (H) in the universe changed since the Big Bang?

A

“Since the Big Bang, the abundance of hydrogen in the universe has remained very high, constituting about 75% of all baryonic matter. While there have been changes in the distribution and concentration of hydrogen due to processes like stellar fusion and nucleosynthesis, the overall abundance of hydrogen has remained relatively constant on cosmic timescales.”

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

What is the Big Bang Theory?

A


The Big Bang Theory is the prevailing cosmological model that describes the early development and expansion of the universe. It posits that the universe originated from a singular, extremely hot and dense state about 13.8 billion years ago and has been expanding and cooling ever since. This theory explains the observed cosmic microwave background radiation, the abundance of light elements, and the large-scale structure of the universe.”

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

Explain the Oddo-Harkins rule

A

Elements having even atomic numbers are more abundant than their immediate neighbors with odd atomic numbers

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

Write or recite the critical reaction for helium burning in the fusion of 3 alpha particles (triple alpha process) to form the nucleus of Carbon 12.

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

Explain why Fe is the heaviest element that a star can produce

A

Elements heavier than iron have fusion reaction with temperature and pressure requirements greater input than those that can occur within the core of a giant star

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

“What is a planet? According to the International Astronomical Union
(IAU)”

A

“a) is in orbit around the Sun
b) has sufficient mass for its self-
gravity to overcome rigid body forces
so that it assumes a hydrostatic
equilibrium (nearly round) shape
c) has cleared the neighborhood
around its orbit.”

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

Explain the key differences of Asteroid belt and the Kuiper belt in terms of their composition and formation

A


The Asteroid Belt, situated between Mars and Jupiter, primarily consists of rocky and metallic objects that failed to coalesce into a planet due to gravitational perturbations from Jupiter. In contrast, the Kuiper Belt, located beyond Neptune, is predominantly composed of icy bodies such as dwarf planets, comets, and icy debris, believed to be remnants from the outer solar system’s formation.”

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

What is a branch of science which deals with celestial objects, space, and the physical universe as a whole

A

Astronomy

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

It is the science of the origin and development of the universe

A

Cosmology

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
18
Q

It is the pattern that appears when the actual brightness and color of many stars are plotted against each other

A

Hertzsprung-Russell Diagram

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
19
Q

Comprises of a system or billions of stars held together by gravity

A

Galaxy

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
20
Q

Our solar system consists of ____ planets

A

8

How well did you know this?
1
Not at all
2
3
4
5
Perfectly
21
Q

According to the mass distribution of our solar system, how many percent is the mass of all planets?

A

0.14%

22
Q

The solar system is composed of _____% Hydrogen and Helium Gas

A

98

23
Q

1 AU = _________

A

149.6 million km

24
Q

These are relatively small bodies (1-10km) in diameter which are composed off small rocky fragment of ice and frozen gases

A

Comet

25
Q

It is a solid piece of debris that originated in outer space and survived its passage through the atmosphere to reach the surface or a planet.

A

Comet

26
Q

It is a solid piece of debris that originated in outer space and survived its passage through the atmosphere to reach the surface or a planet.

A

Meteorite

27
Q

How many years is the cycle change of Eccentricity?

A

100,000

28
Q

Earth’s obliquity changes every ______ years.

A

41,000

29
Q

______ is the light colored portion of the moon which is rich in Ca-rich plagioclase

A

Highlands

30
Q

______ is the largest extinction event where 90% of all the life forms are wiped out

A

K-T extinction

31
Q

Average temperature of the sun.

A

17,000,000 C

32
Q

Enumerate all the terrestrial planets

A

Mercury, Venus, Earth, Mars

33
Q

Enumerate the heirarchy of matter in the universe from planets to clusters of galaxies

A

Planets - stars/pulsars/blackholes - galaxies - clusters of galaxies

34
Q

Life cycle of a star

A

“Giant Gas Cloud
and Dust (Nebula)
2. Protostar
3. T-Tauri Phase
4. Main Sequence
5. Red Giant
6. Fusion of Heavier
Elements
7. Supernovae and
Planetary Nebulae”

35
Q

Draw the position of Perihelion and Aphelion with distances

A

Perihelion 142M km, Aphelion 157M km

36
Q

Enumerate the 4 types of processes that appreciably affect the planetary surfaces

A

Impact cratering, Volcanism, Tectonism, Atmosphere

37
Q

What are the 3 types of meteorites?

A

Stony Meteorites, Stony-Iron Meteorites, Iron Meteorites

38
Q

These elements do not occur in the solar system because all of their isotopes are unstable and decay rapidly

A

technicium and promethium

39
Q

Differentiate prograde vs retrograde rotation

A

“Prograde refers to an object that spins in the same direction as its orbit
Retrograde refers to an object that spins in the opposite direction of its orbit.”

40
Q

Differentiate, protium, deuterium, and tritium

A

These are isotopes of hydrogen. Protium has no neutrons, deuterium has one neutron, and tritium has two neutrons.

41
Q

Enumerate five elements that formed from the stellar nucleosynthesis of small and large stars

A

C, N, O, Ne, S

42
Q

What elements stand out with surprisingly low abundance despite having low atomic numbers?

A

lithium, beryllium, boron

43
Q

Enumerate all the waves and rays in increasing wavelength

A

Gamma, X-rays, UV, Visible, Infrared, Mircowave, Radio Waves

44
Q

Enumerate all the colors of the visible light in increasing wavelength

A

Violet, Blue, Green, Yellow, Orange, Red

45
Q

Enumerate 3 types of chondrites

A

Carbonaceous, Ordinary, Enstatite

46
Q

Enumerate types of achondrites

A

Primitive, Lunar, Martian, HED

47
Q

List the three main components of the solar nebula theory

A

The three main components of the solar nebula theory are: a. Solar Nebula b. Accretion Disk c. Condensation Theory

48
Q

Enumerate the four major steps in the formation of the solar system, in chronological order

A

The four major steps in the formation of the solar system, in chronological order, are: a. Collapse of a Solar Nebula b. Formation of the Protostar and Accretion Disk c. Accretion of Planetesimals d. Formation of Planets and Moons

49
Q

Identify the three primary sources of energy during the early stages of solar system formation.

A

The three primary sources of energy during the early stages of solar system formation are: a. Gravitational Potential Energy b. Heat from Collisions c. Radioactive Decay

50
Q

Name the process by which planetesimals grow larger through collisions and gravitational attraction.

A

The process by which planetesimals grow larger through collisions and gravitational attraction is called accretion.

51
Q

List the three key factors that influenced the differentiation of planets during the formation of the solar system

A

a. Density stratification b. Heat from accretion and radioactive decay c. Gravitational compression

52
Q
A