Exam 14: A Run-Of-The-Mill G-Type Starour Sun

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At the center of the Sun,the temperature is roughly 15 million K.

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Detection of solar neutrinos confirms that

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In our Sun,hydrostatic equilibrium exists only in the core,where energy production via fusion can balance gravity.

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Magnetic field is continuously produced and deformed in the Sun by

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In a sunspot,the umbra is cooler than the penumbra.

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The surface of the Sun appears sharp because

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The solar magnetic field switches polarity every 11 years.

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The solar neutrino problem was solved by postulating that neutrinos have a small mass and oscillate between five different types of neutrino.

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The temperature of the corona is much hotter than any other layer in the solar atmosphere.

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If a sunspot is half as bright as the surrounding photosphere of the Sun,what is the approximate temperature of the gas in the sunspot if the photosphere's average temperature is 5,800 K?

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If the Sun converts If the Sun converts   of H to He per second and 10 percent of the Sun's total mass is available for nuclear burning,how long might we expect the Sun to live? of H to He per second and 10 percent of the Sun's total mass is available for nuclear burning,how long might we expect the Sun to live?

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If a coronal mass ejection occurred on the Sun and ejected particles toward the Earth that traveled at the speed of 1,000 km/s,how long would it take them to reach Earth?

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Explain why magnetic fields trap coronal gas over much of the solar surface but allow it to escape in coronal holes.

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In the text we considered the case of a "too-large" Sun.Show that a star with the same mass,composition,radius,and luminosity as the Sun,but with a higher temperature (that is,a "too-hot" Sun),also leads to a contradiction.

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Approximately how long does it take the photons released in nuclear reactions in the core of the Sun to exit the photosphere?

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Our Sun is unique compared to the other stars in our galaxy because of its

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Sunspots appear dark because

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Hydrostatic equilibrium is a balance between

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Why is hydrogen burning the main energy source for main-sequence stars? Give at least two reasons.

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If the Sun converts If the Sun converts   of H to He per second and the mass of a single hydrogen nucleus is   ,how many net proton-proton reactions go on per second in the Sun? What is the luminosity produced if the mass difference between a single helium nucleus and four hydrogen nuclei is   ? Note that   . of H to He per second and the mass of a single hydrogen nucleus is If the Sun converts   of H to He per second and the mass of a single hydrogen nucleus is   ,how many net proton-proton reactions go on per second in the Sun? What is the luminosity produced if the mass difference between a single helium nucleus and four hydrogen nuclei is   ? Note that   . ,how many net proton-proton reactions go on per second in the Sun? What is the luminosity produced if the mass difference between a single helium nucleus and four hydrogen nuclei is If the Sun converts   of H to He per second and the mass of a single hydrogen nucleus is   ,how many net proton-proton reactions go on per second in the Sun? What is the luminosity produced if the mass difference between a single helium nucleus and four hydrogen nuclei is   ? Note that   . ? Note that If the Sun converts   of H to He per second and the mass of a single hydrogen nucleus is   ,how many net proton-proton reactions go on per second in the Sun? What is the luminosity produced if the mass difference between a single helium nucleus and four hydrogen nuclei is   ? Note that   . .

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