ASTR103 - Solar system formation

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Created by:

bbarocho Plus on September 16, 2011

Subjects:

astronomy

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Week 4 topics

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ASTR103 - Solar system formation

Evolutionary hypothesis
Descartes proposed that the solar system formed from a contracting vortex of matter.
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Evolutionary hypothesis Descartes proposed that the solar system formed from a contracting vortex of matter.
Catastrophic hypothesis 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
Nebular 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
Terrestrial planets Inner four planets, small, rocky, dense
4 terrestrial planet Mercury
Venus
Earth
Mars
Jovian planets Outer planets, large, low density
4 jovian planets Jupiter
Saturn
Uranus
Neptune
Asteroids Small, irregular, rocky bodies, are located between the orbits of Mars and Jupiter
Kuiper belt Small, icy bodies that orbit the sun beyond the orbit of neptune
Comets 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
Meteoroids Rock in space in space before it plunges into the Earth's atmosphere
Meteors 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".
Meteorites Specks of dust, grains of sand, or tiny pebbles that survive the passage to Earth's surface.
Half-life the age of a rocky body found by radioactive dating based on decay
Condensation During the solar nebula converted some of the gas into solid bits of matter
Accretion Bits of matter from condensation grow by this process
Planetesimals Accretion bits of matter form billions of these
Protoplanets Planets begin growing by accretion of solid material into this
Gravitational collapse Once a protoplanet approaches about 15 Earth masses, it can begin growing by this process by pulling gas from the solar nebula

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