Exam 19: Origin of the Solar System and Extrasolar Planets

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Explain the steps involved in clearing a nebular of its interstellar material that stopped planetary formation.

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Which is the correct order of planetary object class during their formation?

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What are the small bits of rock and metal that collide with Earth's atmosphere?

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The most important source for determining the age of the Solar System is by sampling a planet's core.

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Kuiper belt objects are small, rocky bodies orbiting beyond Mars.

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According to solar nebula theory, what is the first step in planetesimal formation?

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What astronomical object is the most important source for determining the age of our Solar System?

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Why do Terrestrial planets not have rings?

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Which space observatory uses the transit method to detect extrasolar planets?

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Which hypothesis was out-ruled by the solar nebular theory?

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Descartes' hypothesis of solar system formation was problematic because he did not understand the ____.

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Asteroids are believed to be debris left over from the failure of a planet to form at a distance of about 3 AU from the Sun.

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The passing star hypothesis suggests that planets form in the rotating disks of gas and dust around young stars.

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The _______________ of a radioactive substance is the time it takes for half of the parent isotope atoms to decay into daughter isotope atoms.

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Match the planetary body with its definition.
small, irregular icy bodies found orbiting beyond Neptune
meteor
the inner four rocky planets of our Solar System
Kuiper belt objects
piece of dust or tiny rock burning in a planet's atmosphere
Planetesimals
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small, irregular icy bodies found orbiting beyond Neptune
meteor
the inner four rocky planets of our Solar System
Kuiper belt objects
piece of dust or tiny rock burning in a planet's atmosphere
Planetesimals
extrasolar Jovian worlds that have been found orbiting close to their parent stars
Terrestrial planets
planets orbiting stars outside of our Solar System
extrasolar planets
the outer four gaseous planets of our Solar system
asteroids
icy bodies with "tails" on a extreme elliptical orbit
hot Jupiters
small, irregular rocky bodies mostly found between Mars and Jupiter
comets
coalescing planetesimals that eventually become planets
Jovian planets
solid bits of matter that will eventually be made into protoplanets
protoplanets
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During Solar System formation, solid particles contracted from the gas of the nebula as it cooled.

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The first extrasolar planets discovered are small and have long orbital periods.

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During the growth of planetesimals to protoplanets, could the planetesimals have collided into one another? Why or why not?

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Once a protoplanet reached a large mass, what is the next step for it to formally grow into a planet?

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Which term is described as small, icy bodies that orbit the Sun just beyond Neptune?

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