Chapter 6- Earth evolution and Earth structure Flashcards
(67 cards)
solar system
consists of the sun, planets, moons, comets, and asteroids
sun
a star composed of hydrogen and helium, largest object in the solar system, making up 99.8% of the total mass of the solar system
Planet
a sizeable objects orbiting a star, massive enough to have it’s own gravity
moon
/natural satellite, body that orbits a planet
asteroids
rocky objects which failed to form a planet
meteorites
rock fragments which fall to earth from space
comet
composed of ice and dust. outer layer melts into water vapour as it gets closer to the sun
Density/Composition/Comparison of metallic meteorites
7.0-8.0 gcm-3. Iron and nickle with some sulfur and silicon. Similar to Earth’s core
Density/Composition/Comparison of stony meteorites
3.0-3.7 gcm-3, silicate minerals similar to peridotite, similar to Earth’s mantle. high porosity
Protoplanetary disc
rotating disc of dense gas and dust surrounding a newly formed stars
Planetisimals
solid objects in protoplanetary discs
protoplanet
moon-sized planetary body that formed within a protoplanetary disc
Impact crater
-circular with a rim of broken rock built up of ejected material
-quartz grains may be shocked or even melted
-rock strata are tilted
-material at depth is broken up
-ejected material is in an inverted sequence
Elastic rebound theory
-two parts of a solid/brittle/competent rock are under stress from opposing forces
-the body of the rock is deformed and put under strain
-energy applied is stored as elastic strain energy
-deformation continues until the stress is more than the strength of the rock and it snaps
-the two parts of the rock suddenly move relative to each other and there is displacement along the fault
-elastic strain energy that was stored is transmitted through the earth by seismic waves
stress
the force per unit area acting on/within a body
strain
the change in shape of a body in response to stress
seismometer
a device which receives seismic vibrations and converts them into a signal which can be transmitted and recorded
seismogram
paper or electronic record made by a seismograph
seismograph
a device which receives and records seismic vibrations
P wave properties
-primary, travel fastest and arrive first
-push, longitudinal/compressional waves, can travel through any type of material
-pressure, particles move together and apart (compression and rarefaction) longitudinal
S waves
-secondary, travel at 60% the speed of P waves
-Shear, the particle movement is sideways in a shearing motion, making it transverse (cannot travel through liquid)
-several, times larger in amplitude than P waves
L waves
-particles oscillate in a circular movement so the wave looses energy quickly with long distance
-travel on the surface
-low frequency, long duration, and large amplitude make them the most destructive
-long, longest wavelength of all the waves
-last, travels slower than P and S waves and arrives last
Formula for velocity of a P wave
Velocity = square root of ( (incompressibility + 3/4 rigidity) / (density) )
formula for velocity of an S wave
Velocity = Square root of ( rigidity/density )