Exam 15: Origin of the Solar System and Extrasolar Planets

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The oldest objects found so far in our solar system are Earth rocks that are 1 billion years old.

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Describe four effects that helped to clear the solar nebula.

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We observe a planet crossing in front of its host star and the planet is smaller than the star. We call this crossing motion a ____________.

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Outgassing is

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The solar system contains no extrasolar planets.

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The iron in our solar system was created from smaller-mass atomic nuclei in

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The ___________ hypothesis of the formation of the solar system uses sudden events that drastically alter the form of the early solar system.

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Terrestrials are small, rocky, and dense.

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Once a terrestrial planet had formed from a large number of planetesimals, heat could have melted it and allowed it to differentiate into a metallic core of ____________density and a rocky mantle or crust of ____________ density.

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A meteoroid, meteor, and meteorite could come from the same celestial body.

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All planets in the solar system orbit counterclockwise as seen from the north.

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All old surfaces in the solar system were heavily cratered during the ________________ period by leftover debris from when the planets formed.

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Describe some characteristics that all the planets seem to share and use the solar nebula theory to explain them.

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The speed of the solar wind is approximately 400 km/s and the distance from the Sun to Saturn is 9.5 AU (1 AU = 1.5 × 108 km). How long does it take a particle in the solar wind to reach Saturn?

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How do the motions of the Sun and planets reflect the disk shape of the solar nebula?

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Massive planets create ____________ Doppler shifts of their stars than lower-mass planets.

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51 Pegasi is important because

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In one sentence, write a scenario involving a meteor, meteorite, and meteoroid.

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How does the solar nebula theory account for the presence of comets?

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  Using the graph shown above, find out how many half-lives does it take for all radioactive atoms to decay into daughter products, Using the graph shown above, find out how many half-lives does it take for all radioactive atoms to decay into daughter products,

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