Lecture 2: The Planet Earth Flashcards
Differentiate heliocentrism from geocentrism
Heliocentrism - Copernican Model
Geocentrism - Ptolemaic Model
Explain the Big Bang
“singularity” – explosion of space-time; extremely hot and dense state which expanded rapidly and then slowly (dark matter) while cooling
What were the pieces of evidence for the Big Bang?
- Hubble’s Law (red shift) – 1929; star moves away
- Cosmic Microwave Background Radiation – remnant/heat
- Abundance of H, He
What were the limitations of the big bang?
- Only explains the universe
- What was present before Big Bang?
- How will it end? Will it ever end?
Explain how the solar system forms
spins (contraction)
- conversion of Gravitational Energy to Thermal Energy
- cooling
- Temperature coalesce forming extraterrestrial bodies
Differentiate terrestrial planets and jovian planets in terms of:
*composition
Rocky composition
Gaseous liquid form composition
(denser materials go through the center of mass)
Differentiate terrestrial planets and jovian planets in terms of:
*elements
Si, Fe, O (Silicate rocks and metals) Light elements (H, He, Ar, C, O, Ni)
shape of earth
Oblate Spheroid
Describe Oblate Spheroid
*flattened at poles; bulging at the equator
Earth’s Axial Tilt
21.5 to 24.5 degrees
Obliquity
23.4 degrees
Orbital Speed
30 km/s
Nebula planetesimals protoplanets
accretion, differentiation
- accretion * differentiaion *
Nebula, planetesimals, protoplanets
*: the process of growth or increase, typically by the gradual accumulation of additional layers of material
Accretion
Accretion: the process of * or increase, typically by the gradual * of additional * of material
growth, accumulation, layers
*: random chunks of primordial matter were transformed into a body whose interior is divided into concentric layers that differ from one another both physically and chemically.
Differentiation
Differentiation: random * were transformed into a * whose interior is divided into * that * from one another both physically and chemically.
chunks of primordial matter, body, concentric layers, differ
In Stage 1 of the formation of earth:
Fe, O, Si, Mg
*no continents, oceans, atmospheres
*Temperature of the planet reached and surpassed the melting point of iron; denser elements sink to center and lighter elements float to top.
Iron Catastrophe
Chemically distinct layers
- Core:
- Mantle:
- Crust:
Fe, Ni
O, Si, Fe, Mg
O, Si
exposures on the surface of the Earth; large scale sequence of rocks
Ophiolites
foreign rock (rock from mantle)
Xenoliths
CO Age
4 Ga
160 Ma