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1. Features of the ocean floor – Mid-ocean ridges and rises: underwater mountain ranges *Ridges tend to be steeper and the width narrower *Rises are opposite with no central valley. - trenches: deep gashes in the ocean crust - convection currents in the mantle causes seafloor to spread at ridges and rises *new crust made at ridges/rises - oceanic crust sinks into trenches *subduction zones have oldest ocean crust |
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the earth is divided into lithospheric plates that separate, collide, or move parallel to one another *creates certain ocean and land features |
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locations of earth quakes |
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convection currents in the mantle |
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– Paleomagnetism: Rock evidence showing the past movement of earth’s magnetic poles, found mainly in oceanic rock. – Earth’s magnetic poles flip and change locations. – Normal and Reverse Polarity • Occurs every few million years • probably due to turnover of liquid in the outer core – Fe and other magnetic elements in lava solidify w/ the magnetic poles – Fe sediments align w/ poles when setting out of water – Magnetic reversals are recorded on ocean floor at ridges and rises – Magnetic signatures match each other on opposite sides of ridges |
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Types of convergent boundries • 3 types of convergent boundaries: Cont-Ocean, Ocean-Ocean, Cont-Cont. • Cont-Ocean: volcanic arcs, trenches, subduction zones, shallow to deep-focus earthquakes • subduction zone: overriding plate scrapes off seafloor sediments and island arcs • subducting plate is heavier and denser • Ocean-Ocean: island arcs, trenches, subduction zones, deep-focus earthquakes • Cont-Cont: mountain ranges, slide underneath but can not sink, not many volcanoes |
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Types of divergent boundries • Divergent or Rift Zones: separating plates, new crust • 2 types: Cont-Cont, Ocean-Ocean – Cont-Cont: rift valleys, geysers, hot springs, long lakes, volcanos, shallow earthquakes, lava flows, pillow lava in lakes, hydrothermal vents, convection cell underneath – Ocean-Ocean: ridge or rise, same as above with pillow lava and hydrothermal vents |
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Transform boundries • Transform: plates slide past or next to each other, on land or water. – shallow earthquakes, escarpments (continuous line of slopes or cliffs), crust not destroyed or created. |
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Active margin • Active Margins: edge of a continental that is tectonically active – usually a trench is offshore and volcanic range near coast |
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Hot spots • Found in center of plates and along ridges/rises, • Magmatic plume from mantle, not a convection current • Plates move over the stationary hot spot • Creates island chain where islands move off hot spot • Chain of extinct volcanic islands off hot spot • Only active island is on hot spot • Lifespan of hot spot is 100 million years. • On land: geysers, hot springs, volcanoes, small concentrated area compared to rift zone. |
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• Since 1900: – Edwin Hubble’s (1889-1953) 2 big discoveries: • Discovered the Andromeda galaxy approximately 2.5 million light years away • Galaxies are moving rapidly away from each other – not in random directions |
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Evidence for Big Bang • Oldest object is a gamma-ray burst 13 billion light-years away. – Brightest, most intense radiation event in the universe. – Occurs when massive star collapses into a black hole. • Calculations show that expanding universe derived at a single point • Immense amount of space in an atom. – conceivable atom reduced to an extremely small amount of space • The Big Bang should produce an immense amount of heat. – Cosmic background radiation of 2.75 degrees above absolute zero (lowest temperature possible). • The abundance of H and He (98% of universe) shows the formation from an explosive event – more complex elements formed through atomic fusion in stars from H and He. |
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Distances and definitions • Light-year: distance of light traveled in one year - 186,000 miles/sec |
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Distances and definitions • Universe - the totality of space, time, matter, and energy. |
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Distances and definitions • Superclusters/localclusters - clusters of galaxies that are usually gravitationally bound |
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Distances and definitions • Galaxy - A collection of stars that bound together by gravity. |
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Distances and definitions • Solar system - planets that orbit a sun or group of suns. |
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Distances and definitions • Star - a glowing ball of gas held together by its own gravity and powered by nuclear fusion. |
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Distances and definitions • Planet - a space body within the solar system: • is in orbit around the Sun • has sufficient mass to produce a round shape • cleared the neighborhood around its orbit • not a satellite (a moon) |
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Distances and definitions • Moon - a small body that is in orbit about a planet. |
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• Spiral galaxy - flattened disc of stars rotating around the center of a black hole. • Galactic bulge - the center of a spiral galaxy, spherical in shape, stars closer together • Galactic disk - the sheet of young stars, dust, and gas revolving around the galactic bulge. • Galactic halo - ancient stars and dust outside of the galactic disk. |
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• Nebular Theory • A previous star was present and exploded (supernova) producing vast amounts of gas and dust. • Dust and gases collect together forming larger bodies. • Passing of a nearby star creates rotation in solar system. • Most dust/gas begin to contract by gravity into protosun. • Smaller eddies of gas/dust begin to contract into protoplanets • Protosun has 99.9% of material, great heat from fusion produces light. • Explosion of solar winds (ions from the sun) blow lighter gases far forming outer planets • Heavier gases and dust remain closer forming inner planets. |
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• Inner Planets • Rocky crust, mantle, iron/nickel core • No or few moons • Small or no atmosphere • Small diameters • Have or had some degree of plate tectonics |
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• Outer Planets – Small core of rock or liquid – Liquid hydrogen mantles – Thick atmosphere of H and He – Large diameters – Many moons/all have rings |
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• Asteroid Belt between Mars and Jupiter – Asteroids - made of carbon, or rocky material, or iron. – Sizes: 10 meters to 1000 kilometers in diameter – 400,000 orbit Sun |
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• Kuiper Belt – a flat disc of comets and dwarf planets beyond Neptune, rotates around the sun. – Comet: a space body made of ice, dust, and rocky material that orbits the Sun. |
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• Oort Cloud – a sphere of comets extending 1 light year away from the Sun. – Contains billions of long-period comets – Comets in the Oort Cloud revolve in random directions around the Sun. |
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Devonian period • Devonian, 408-360 Ma, Nov 28-Dec 3 • Acadian and Ural Orogenies • Age of Fishes • Transition of vertebrates to land • First trees and seed-bearing plants |
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Devonian period • Climate is really controlled on a local level, especially on Laurasia. • Most of continent lay in the rain shadow behind the mountain ranges • Erg • Rain was falling on the eastern side of mountains around Laurasia. • Forests growing on eastern side |
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Devonian period • Ostracoderms ("shell-skinned") - jawless fishes completely covered in armor of bony plates. • The Placodermi (bony-head fish) – fish with armored head and thorax, rest of body was scaled or skin. • Dunkleosteus: • 30 ft long, placiderm, top predator in ocean |
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Devonian period • Crossopterygians: group of lobe-fin fish with muscular fins for moving occasionally on land • Ichthyostega: one of the first true amphibians to exist on land |
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Devonian period • Development of woody plants; the ability to grow taller to reach open sunlight and to carry a greater weight of branches and leaves. • 4 Plant Guilds: • Trees • Shrubs • Weeds • Survivalists • Archaeopteris: earliest modern tree, grew 30 meters tall |
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• For North America, Carboniferous divided into 2 periods: • Mississipian (360-320 Ma) known for its limestone deposits across Laurasia • Pennsylavanian (320-286 Ma) known for swamplands and coal deposits when regression occurred later. |
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• Late Carboniferous, Gondwanaland collides with Laurasia to form Pangea. • Collision of Gondwanaland begins the last phase of Appalachian Mountains – Appalachian orogeny. |
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• Vigorous growth of trees may have sucked much of the CO2 out of the atmosphere, producing a surplus of oxygen. • Oxygen levels were higher during this time than at any other time in the history of the Earth (30% of atmosphere). • Gondwanaland has its own very distinct flora, dominated by glossopteris |
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Stocky-bodied and armoured millipede-like Arthropleura was 1.8 meters long |
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Carboniferous period – The first reptiles appear |
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Carboniferous period – The key feature in the origin of reptiles is the amniotic egg. – Durable outer shell protects embryo from drying – Egg can be laid on land – Yolky part of egg provides nutrition; sac contains embryo and another sac collects waste products. – Young adult hatches; no need for larval stage – Eliminated need to lay eggs in water, allowing vertebrates to live and reproduce on dry land for the first time. |
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Carboniferous period – General trends how E’s food chain is built. – Plants first on land: – Reproduced by spores but tied to water – Seed allows plants to grow on dry land – Seeds are opportunistic waiting for water to germinate. – Animals follow plants: – Insects eat plants and are in turn food for other animals – Lobe-finned fishes and amphibians still tied to water for reproduction. – Vertebrates eat plants, insects, and other vertebrates – Amniotic egg allows reptiles to colonize dry land. |
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– Early in Permian, Pelycosaurs (fin backed reptile) became the top carnivores and herbivores. – Dimetrodon and Edaphosaurus – attained lengths ~ 3 meters – The large dorsal "sails" may have helped control body heat – advantage over more sluggish sail-less relatives – Limited to the equatorial tropics. |
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– Therapsids (Mammal-like reptiles) – Skulls resembles mammals – Legs positioned more vertically under body – Teeth were dog-like – May have been endothermic (warm-blooded) and hair – Cold-adapted. |
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– Permian flora changes from swamp conditions to dry – Biggest change is the growth of gymnosperms (flowerless seed plants); conifers dominate |
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– Evidence for extinction: – 1st: Fossilized pollen shows biological complexity up until the Permian; then worldwide fungal material at Triassic – Whatever died on land, fungi being decomposers took over most of plant life on land – 2nd: Several C-12 spikes in rocks at this time – all life is made of C-12 and maintains a steady rate unless an extinction occurs; more C-12 seen in rocks at Permian extinction. – 3rd: Huge amounts of lava flowed out of Siberia for a million years – Huge emissions of Cl2, SO2, and CO2. – 4th: Layer of black shale deposited in ocean – Represents anoxic conditions where organic material is not decomposed – not enough O2. – 5th: Ocean regression at end of Permian – Triassic rocks are stained red color; means a lot of oxygen taken out of atmosphere to form rusted minerals. – Many of these rocks exposed from regression – 6th: Huge rise in worldwide temperatures (up to 6°C) – 7th: Meandering rivers – Lots of sediment from continental eroding – Little plant life |
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– Crinoids (echinoderm): animals that have stalk, long arms, head with mouth. – Most crinoids lived attached to the sea-floor by a flexible stem – Crinoids have a cup-shaped head with long, branching arms. – Remains can form thick LS. |
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– Blastoids (echinoderm), a long stalk with a head at the top. Fragile and slender arms attach near the mouth of the individual |
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