EDWARD'S LECTURE NOTES:
More notes at http://tanguay.info/learntracker
C O U R S E 
Formation of the Universe, Solar System, Earth and Life
Henning Haack, University of Copenhagen
https://www.coursera.org/course/origins
C O U R S E   L E C T U R E 
The Origin of Solar Systems
Notes taken on May 30, 2016 by Edward Tanguay
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while solar systems are based on hydrogen and helium, they also also likely to include all the elements of the period table
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many generations of dying stars have injected freshly synthesized matter into interstellar space
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how can this widely scattered matter be used to form dense solar systems for planets
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if the matter was evenly distributed throughout the universe, this would be a hopeless task
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fortunately, due to the force of gravity, matter is concentrated in galaxies such as our own Milky Way galaxy
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within the galaxies, most of the matter is concentrated in molecular clouds
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these are enormous clouds, even when we observe them from as far away as the Earth
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yet because they are also very faint, they also remain almost invisible to the naked eye
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the Orion constellation which lies close to the terrestrial equator
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the three bright stars are known as Orion's belt
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if we zoom in and increase the brightness, the underlying cloud becomes visible
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Horsehead Nebula
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Orion Nebula
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this is a star-forming region
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we cannot observe how our own solar system formed, but observing places like this, we can deduce how solar systems form in general
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the size of molecular clouds can be measured in units of light years
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molecular clouds look passive but they are highly dynamic
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stellar winds push the gas around at speeds up to several hundred km/s
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even at these speeds, it would take a millions years to traverse the width of these clouds
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we use computer simulations to fast-forward this process
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can run the simulation for two million years
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newborn stars light up within the cloud as the simulation runs
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but we need to compress it by many orders of magnitude to form a solar system
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sometimes gas gets compressed to a point that gravity is stronger than the gas pressure
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the result is a runaway collapse resulting in star formation
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a famous example of star formation is seen in the Hubble image of the Eagle Nebula
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intense stellar winds have created a bubble in the cloud
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the stellar winds not only push the gas further and further away from the star through a process known as photoevaporation
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it also compresses the gas to point where a gravitational collapse is triggered
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this is exactly what we need to form a new star
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once a dense core is formed, it's gravity field will start to grow as attracts more and more gas and thus further increases a gravity field, which is called accretion
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each of these tentacle-like structures contains a new star at the tip
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eventually the gas will clear around the new star, accretion will cease, and the star will begin its life as an independent object
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as the gas collapses toward the growing star, it will rotate faster and faster, much like water running out of a bathtub
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the accretion prevents all of the gas from accreting directly to the star
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instead, a rotating disc of gas and dust is formed around the young star
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it is from these discs that planets are formed
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this explains why all of the planets in our solar system orbit in the same plane around the sun
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early solar systems
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matter from the cloud is falling in toward the disc
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most of the mass is drifting inwards toward the star
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concentrated toward the mid-plane, we find solids of different sizes
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near the start, milimeter-size particles known as CAI's condense out of the gas
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Calcium/Aluminum-rich inclusions
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calcium and aluminum condense at very high temperatures
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meteorites have CAIs, e.g. white, irregular inclusions in a rock
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further away from the star we find silicate spheres known as chondrules
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the disc is composed of dust and gas
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near the center there are no ice crystals, further out there are ice crystals
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as a result, outer planets grow faster and bigger
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the gas in the disc was only present for a few million years
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the outer planets beyond the frost line grew big enough to capture gas from the disc while it was still there
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became gas giants
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inside the frost line, smaller rocky or terrestrial planets formed, e.g. Mercury, Venus, Earth and Mars
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accretion of the planets
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a protoplanetary core
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accretes dust, condrules and CAIs
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in the last stages of accretion there were only a few large planetary formations
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one of the last of these later formations which accreted to the Earth was probably Mars-sized
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resulted in a collision of cataclysmic proportions
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the presence of our Moon was likely a consequence of this event