midterm 1 Flashcards
do earthquakes occur at predicted/pattern frequencies?
no
lots of randomness
where smaller ones happen often and major/great earthquakes happen less frequently
Great (8 or higher)
freq per year = ~1
return period = ~1 year
Major (7–7.9)
freq per year = ~10
return period = ~1 month
Strong 6–6.9
freq per year = ~100
return period = ~½ week
Moderate 5–5.9
freq per year = ~1,000
return period = ~8 hours
Light 4–4.9
freq per year = ~10,000
return period = ~1 hour
Minor 3–3.9
freq per year = ~100,000
return period = ~5 minutes
Very minor 2–2.9
freq per year = ~1,000,000 return period = ~½ minute
equation for hazard, vulnerability, and risk
risk = hazard x vulnerability
what is a “natural hazard”?
natural event that is potentially dangerous
what is a “natural disaster” ?
when a hazardous event causes loss of life, injury, damage to property or infrastructure, or economic losses
how did earth form, how long did it take (roughly), and how long ago ?
accretion and differentiation
around 30 million years
∼4.55 billion years ago
moon around same time
what compound formed mantle ?
SiO2
metal sinks and silicate rises
how did differentiation occur ?
formed into distinct layers – SiO2 formed mantle
metal sinks and silicate rises
meteorites
fragments of protoplanets
look similar to rocks found on earth
easy to spot in deserts or frozen deserts
DIFFERENT TYPES:
*CHONDRITES
- 75-90% silica (SiO2) + 10-25% nickel-iron alloy
- bubbles prove its never been molten
- oldest rock in entire solar system
- chondrules
–> representation of how earth
and other planets formed
–> represent primitive material
and protoplanetary disk
*ACHONDRITES
- 75-90% silica (SiO2) + 10-25% nickel-iron alloy
- NO chondrules
- outer silica mantle
–> represent molten differentiation of protoplanets
*STONY-IRONS
- 50% silica + 50% nickel-iron alloy
- boundary between outer silica mantle and core
- molten iron and molten silica are unmissable (dont mix)
–> represent differentiated cores
of these bodies
*IRON meteorites
- 100% nickel-iron alloy
- earliest sources of iron
- origin in cores of protoplanets
–> represent differentiated cores
of these bodies
radiometric dating
Chondrites
~4.56 billion yrs ago
Achondrites,
Stony-irons, and
Irons
- Processes took up to 30 million years
80% of geological
time: no animals
- humans: 0.004%
earths mantle much hotter when formed than it is today
Impact events
- energy, return periods
amount of energy released is enormous
avg return is proportional to size of impacter
inversely proportional to size
earths surface is constantly changing by erosion and tectonics - therefore less traceable with events than the moon
have caused mass extinctions in past
asteroids
rocky bodies up to several hundred kilometers in diameter which orbit the Sun in the Asteroid Belt between Mars and Jupiter, or in the Kuiper Belt beyond Neptune
too small to be considered planets
- mostly in asteroid belt and kuiper belt
Comets
bodies composed of rock, dust and ice up to ∼60 km in diameter
normally orbit the sun
vaporize causing tail
different than asteroids
bc also contain ice
water, methane, and ammonia
tails can be really long
“mostly originate from the Kuiper Belt or the distant Oort Cloud and which orbit the Sun in highly elliptical orbits”
impact craters on earth
just under two hundred confirmed impact craters on Earth,
amongst the largest of which are the
∼214 million year-old Manicouagan, Quebec
and ∼1.85 billion year-old Sudbury, Ontario
Earth’s structure
density increases inwards
Sedimentary rocks:
~2 g/cm3
Granite:
~2.8 g/cm3
Basalt:
~3.0 g/cm3
Earth’s structure – the mantle (components)
Olivine
Spinel
Perovskite
earthquake waves
- can be used to infer depths of the boundaries
- know outer core is still molten since s waves dont pass thru liquids
P-waves: faster,
can travel through liquid
S-waves:
slower, cannot travel through liquid
Earth’s physical and chemical structure
Crust: (light colour, low
density rock)
~0.5% of Earth mass
Temp: ~0–1000 ºC
Silicate rocks (Al, Na)
Mantle: (solid, rocky)
~67% of Earth mass
Temp: ~1000–3000 ºC
Silicate rocks (Fe, Mg)
Core: outer core = liq iron
inner core = solid iron
~32% of Earth mass
Temp: ~4000–6000 ºC
Fe-Ni alloy (metal)
Earth’s rheological structure
atmosphere (gas)
hydrosphere (liquid)
lithosphere (solid)
asthenosphere (“soft plastic”)
mesosphere (“stiff plastic”)
outer core (liquid)
inner core (solid)
Rheology – stress and strain
stress = force per unit area
strain = deformation of material occurs under stress
(unitless)
shear = one side goes one way, one goes another
elastic, plastic, ductile, brittle
Rheology is dependent on time, temperature, and pressure (and composition)
mechanisms of heat transfer
conduction
- particles themselves dont move, just transfer of heat thru electrons
convection
- heat transfer thru particles in a fluid –> v little gradient in temp from top to bottom
radiation
The geothermal gradient
3 different melt states
3 distinct layers on outer part of earth
solid, partially molten, liquid
mesosphere
= no melting
- stiff, plastic, solid
asthenosphere
= partial melting
- soft, ductile
lithosphere
- no melting
- brittle
Oceanic and continental crust
Oceanic crust:
= basalt
~3.0 g/cm3
- iron and magnesium rich rock
Mantle:
= peridotite
~3.2 g/cm3
Continental crust:
= granite
~2.8 g/cm3
- sodium and aluminum
- lighter than basalt
Earth’s magnetic field
north magnetic pole and south magnetic pole are not same as geographic north and south poles