Exam 14: Our Starthe Sun
Exam 1: Why Learn Astronomy92 Questions
Exam 2: Patterns in the Skymotions of Earth96 Questions
Exam 3: Motion of Astronomical Bodies91 Questions
Exam 4: Gravity and Orbits88 Questions
Exam 5: Light87 Questions
Exam 6: The Tools of the Astronomer94 Questions
Exam 7: The Birth and Evolution of Planetary Systems87 Questions
Exam 8: The Terrestrial Planets and Earths Moon99 Questions
Exam 9: Atmospheres of the Terrestrial Planets92 Questions
Exam 10: Worlds of Gas and Liquid the Giant Planets92 Questions
Exam 11: Planetary Adornmentsmoons and Rings93 Questions
Exam 12: Dwarf Planets and Small Solar System Bodies89 Questions
Exam 13: Taking the Measure of Stars88 Questions
Exam 14: Our Starthe Sun88 Questions
Exam 15: Star Formation and the Interstellar Medium89 Questions
Exam 16: Evolution of Low-Mass Stars90 Questions
Exam 17: Evolution of High-Mass Stars90 Questions
Exam 18: Relativity and Black Holes90 Questions
Exam 19: The Expanding Universe90 Questions
Exam 20: Galaxies95 Questions
Exam 21: The Milky Waya Normal Spiral Galaxy96 Questions
Exam 22: Modern Cosmology92 Questions
Exam 23: Large-Scale Structure in the Universe65 Questions
Exam 24: Life61 Questions
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Astronauts in space could be harmed by the high-energy particles given off during a solar flare. So, when a solar flare is observed, a warning can be given to astronauts to tell them to get inside the space station for protection. Explain why there is enough time between the first observation of a flare and the arrival of the harmful particles for this system to work.
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Calculate the amount of energy released by converting four hydrogen atoms into one helium atom. The mass of a hydrogen atom is 1.67 * 10-24g; the mass of a helium atom is 6.65 *10-24
g. The speed of light is 3 * 108 m/s.
(Essay)
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How do periods of strong solar activity affect near-Earth orbiting spacecraft?
(Essay)
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The Sun's corona has a temperature of approximately 1 million degrees. At what wavelength and in what part of the electromagnetic spectrum does its radiation peak?
(Multiple Choice)
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If the Sun went through a period where there were many sunspots for a number of decades straight, what would happen to the climate of the Earth?
(Essay)
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Density, temperature, and pressure increase as you move inward in the interior of the Sun. This means that the force of gravity, (Fg = GMm/r2), _________ as you move inward toward the core.
(Multiple Choice)
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Why is hydrogen burning the main energy source for main-sequence stars?
(Multiple Choice)
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Why is hydrogen burning the main energy source for main-sequence stars? Give at least two reasons.
(Essay)
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Which of the following are created by solar magnetic activity?
(Multiple Choice)
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The fact that the surface of the Sun rings like a bell lets us understand its interior better.
(True/False)
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Through hydrogen fusion, the Sun loses approximately 4 million tons of mass each second. If it burns hydrogen at this rate for 10 billion years, what percentage of its original mass will it lose in all? (Note: The mass of the Sun is 1.99*1030 kg, and 1 ton = 1,000 kg.)
(Essay)
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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.
(Essay)
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Which force is responsible for holding the protons and neutrons in the nucleus of an atom together?
(Multiple Choice)
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If you observe a maximum number of sunspots right now, how long would you have to wait to see the next solar maximum?
(Multiple Choice)
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If neutrinos oscillated between five different types of neutrino during their transit from the Sun to Earth, then how many neutrinos would we have detected compared to what was emitted by the Sun?
(Multiple Choice)
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Sunspots appear dark because they have _________ than the surrounding gas.
(Multiple Choice)
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