Geology + Astronomy Flashcards

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1
Q

The Big Bang Theory is the origin of time and space according to science. According to this theory the universe started out of _______ and will continue to ______

A

Nothing;expand

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2
Q

What is the Red shift of Galaxies

A

There is a Red and Blue shift. When objects are moving towards or away from something they emit a light. Depending on the light’s wavelength and frequency. Red light = longer wavelength + lower frequency while blue light = higher frequency + shorter wavelengths. Objects in the universe display a red shift as they are moving away from us, or the universe is expanding. This was discovered by Edwin Hubble.

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3
Q

What are the Abundance of Light Weight Elements

A

Hydrogen, Helium, and Lithium are the most abundant elements in the universe.

If the universe started with nothing, then the most prevalent elements would be the building blocks of other elements.

Hydrogen and helium led to the larger elements such carbon and iron

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4
Q

What is the Cosmic Background Radiation (cmb)

A

The leftover heat from the Big Bang

Satellite imaging of the CMB is getting better through the year

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5
Q

What are the 3 main concerns of the big bang theory

A

The monopole, flatness, and horizon problems

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6
Q

What is the monopole problem

A

The theory states that there should be an abundance of single sided (only north or south) magnets within the universe. The amount observed around our galaxy does not confirm this.

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7
Q

What is the flatness problem

A

WMAP has determined the geometry of the universe to be nearly flat. However, under Big Bang cosmology, curvature grows with time. A universe as flat as we see it today would require an extreme fine-tuning of conditions in the past, which would be an unbelievable coincidence.

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8
Q

What is the horizon problem

A

Distant regions of space in opposite directions of the sky are so far apart that, assuming standard Big Bang expansion, they could never have been in causal contact with each other. This is because the light travel time between them exceeds the age of the universe. Yet the uniformity of the cosmic microwave background temperature tells us that these regions must have been in contact with each other in the past.

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9
Q

Life cycle of a small star

A

Nebula, main sequence star, red giant, planetary nebula, white dwarf, white dwarf cools, black dwarf.

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10
Q

Life cycle of a giant star

A

Nebula, main sequence star, red supergiant, supernova, then a supernova turns into either a black hole or a neutron star.
black hole - the core collapses completely and vanishes
neutron star - the core collapses and gets extremely dense.

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11
Q

How does a star change form (what is happening to the core)

A

When a star goes from one stage to the next it is caused by what is happening in the core. Inside the core there should be equal parts of gravity pushing down and nuclear fusion of lighter elements (hydrogen and helium). Once the gravity and fusion are not equal such as when fuel or the main element is used up the core will collapse upon itself starting to heat up which causes more fusion of the newly made element and the star will start to expand. The next stages depend on the mass of the star though. Both start out as a main sequence star using hydrogen as the main source of fuel that fuses together to make helium. When hydrogen runs out the core collapses and will either grow into a red giant or red supergiant depending on the mass of the star.

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12
Q

What color star is cooler and what is hotter: a red star and a blue star

A

a red star is cooler than a blue star

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13
Q

What does mass determine in a star

A

Luminosity of a star, the bigger the star, the brighter it is.

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14
Q

What are Kepler’s laws

A

1 - Planets don’t have a circular, but an elliptical path around the sun
2 - The closer a planets orbit is to the sun, the more distance it will cover fast.
3 - the farther a planet is from the sun it will take longer to completely orbit the sun.

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15
Q

What does p^2 d^3 mean

A

You square the AU’s/years then cube the total
P= AU’s/years
D= Distance

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16
Q

What is a terrestrial planet

A

Very dense
First 4 planets - Mercury, Venus, Earth and Mars
If could go to the planets could stand on them

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17
Q

What is a jovian planet

A

Gas planets
Last 4 planets - Jupiter, Saturn, Neptune, Uranus
Can’t stand on them if could visit them
Lighter in density

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18
Q

Planets vs. Dwarf Planets

A

To be a planet have to follow the three criteria:
Orbit the sun
Hydrostatic equilibrium that makes it spherical in shape
Clears one’s neighborhood

An astral body is considered a dwarf planet when it doesn’t follow the last criteria of clearing the neighborhood.
For example Pluto is a dwarf planet due to not clearing the neighborhood of Neptune. Pluto goes into Neptune’s orbit as it goes around the sun.

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19
Q

Asteroids

A

Found in the asteroid belt between Mars and Jupiter
Huge piece of space rock
Very eccentric (oval) orbits

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20
Q

Comets

A

Known as a “dirty snowball”
Made up of dirt and frozen gases
Develop a tail that points away from the sun.
Eccentric (oval) orbits

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21
Q

Meteors, Meteorites, and Meteoroids

A

Made up of iron and nickel
The names depends on location
Meteors - space rock that is burning in Earth’s atmosphere known as shooting star
Meteorites - space rock that that has travelled through Earth’s atmosphere and has hit the ground
Meteoroid - space rock that is in space orbiting around

22
Q

Crust

A

Solid, surface temp, 5-25 km thick

23
Q

Lithosphere

A

Solid, surface temp to upper mantle temperature, 100km

LITHOSPHERE IS THE PLATES

24
Q

Asthenosphere

A

Molten rock, 2300 F, 180 km thick

ASTHENOSPHERE IS THE MOLTEN TOP PART OF THE MANTLE UNDER THE LITHOSPHERE

25
Q

Mantle

A

thickest layer, 2900 km, molten and liquid

26
Q

Outer Core

A

Liquid, 4500 - 5500 C, 2200 km

27
Q

Inner Core

A

Solid, 1200 km thick, 5200 C

28
Q

Divergent Boundaries

A
Seafloor spreading (O-O)
Rift valley, Volcanoes, and Ridges
29
Q

Convergent Boundaries

A

Collision Boundaries
two continental crust push upward against each other
Subduction zones (O-C)
older and dense plate goes under the less dense plate
Mountains, Volcanoes, and Earthquakes

30
Q

Transform Boundaries

A

Two plates move horizontally past each other

Earthquakes and faults

31
Q

Normal fault

A

tension stress

32
Q

Reverse/Thrust fault

A

Compression

33
Q

Strike-slip fault

A

Shear Stress

34
Q

What side is the footwall

A

Left side is footwall because it is below the fault in normal and reverse fault images

35
Q

The three types of waves are below. Describe what type of wave they are, how they move through the medium and what mediums it can move through
primary-
secondary-
surface-

A

Primary (P) Waves: These are compression waves, so they compress and stretch the medium in the same direction as it travels. It moves through solids, liquids and gases
Secondary (S) Waves These are shear waves, so they move the medium in a perpendicular direction as it travels. It moves through solids only
Surface (L) Waves These are waves that both compress and slide material. They can only travel along the surface of the medium

36
Q

Rock types

A

Sedimentary, Metamorphic and Igneous

37
Q

Rock Characteristics

A

Sedi- Layers, Brittle, contains fossils or other small pebbles

Meta- Ribbon like bands, Crystals

Igne- Extrusive: Hard, smooth, and Glassy
Intrusive: Rough, Air bubbles, and brittle

38
Q

How the rocks are formed

A

Sedi- Extrusive: Hard, smooth, and Glassy
Intrusive: Rough, Air bubbles, and brittle

Meta- Heat and Pressure

Igne- Melting and cooling

39
Q

Examples

A

Sedi- Conglomerate, sandstone, opals

Meta- Marble

Igne- Extrusive: Pumice
Intrusive: Obsidian

40
Q

Weather is

A

Day to day changes in atmospheric conditions

41
Q

Atmospheric Pressure

A

High or low systems.
High pressure - Causes winds to leave area, generally nicer weather
Low Pressure - Causes winds to enter area, generally more stormy weather

42
Q

Greenhouse Effect

A

The absorption of longwave radiation by chemical compounds such as methane, carbon dioxide, and water. Creates an increase in temperature.

43
Q

Latitude

A

near equator is warmer, closer to poles is colder

44
Q

Elevation/Altitude

A

Higher elevation results in colder climate

45
Q

Bodies of Water/Currents

A

bodies of water lead to more mild temperatures and an increase in precipitation

46
Q

Landscape

A

In the northern hemisphere more rain if on the western side of mountains, drier on the eastern side. The opposite is true in the southern hemisphere.

47
Q

Greenhouse effect

A

Increased temperature

48
Q

What is the defining characteristic that makes up the layers of the atmosphere

A

Chemical composition, Temperature, density and Pressures

49
Q

What phenomena occur at each layer of the atmosphere

A
Troposphere - Weather
Stratosphere - Ozone Layer
Mesosphere - Meteors/shooting stars
Thermosphere - Ionosphere/Northern and Southern lights
Exosphere - Satellites
50
Q

How does pressure and temperature changes in each layer of the atmosphere

A

temp. air pressure
Troposphere - Decreases Decreases

Stratosphere - Increases Decreases

Mesosphere - Decreases Decreases

Thermosphere - Increases Decreases

Exosphere - Decreases Decreases