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ASTR103 - Solar system formation
Week 4 topics
Descartes proposed that the solar system formed from a contracting vortex of matter.
Buffon later suggested that a passing comet pulled matter out of the sun to form the planet
Passing star hypothesis
Astronomers replaced the comet with a star from catastrophic (comet) hypothesis
Laplace's hypothesis required a contracting nebula to leave behind rings that formed each planet
Angular momentum problem
Puzzle of the sun's low angular momentum
Solar nebula theory
Theory proposes that the planets formed in a disk of gas and dust around the protostar that became the sun
Inner four planets, small, rocky, dense
4 terrestrial planet
Outer planets, large, low density
4 jovian planets
Small, irregular, rocky bodies, are located between the orbits of Mars and Jupiter
Small, icy bodies that orbit the sun beyond the orbit of neptune
Icy bodies that pass through the inner solar system along long elliptical orbits. As the ices vaporize and release dust, the comet develops a tail that points approximately away from the sun
Rock in space in space before it plunges into the Earth's atmosphere
Small bits of rock and metal colliding with Earth's atmosphere and bursting into incandescent vapor because of friction with the air about 80 km above the ground. Commonly called "shooting stars".
Specks of dust, grains of sand, or tiny pebbles that survive the passage to Earth's surface.
the age of a rocky body found by radioactive dating based on decay
During the solar nebula converted some of the gas into solid bits of matter
Bits of matter from condensation grow by this process
Accretion bits of matter form billions of these
Planets begin growing by accretion of solid material into this
Once a protoplanet approaches about 15 Earth masses, it can begin growing by this process by pulling gas from the solar nebula