Exam 3: Cycles of the Sun and Moon

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What two pieces of information are needed to determine the diameter of a faraway object? Explain how that information is used to determine the diameter.

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A(n) ____________________ Moon rises in the eastern sky approximately as Sun sets.

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The Moon has an angular diameter of 0.5°. What is the Moon's angular diameter in minutes of arc?

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A portion or all of the same zodiac constellations can be seen by those in either hemisphere year round.

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The ecliptic can be defined as

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The equator receives the same amount of sunlight from season to season.

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A total lunar eclipse is

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An eclipse season is the interval during which the Sun crosses a node of the Moon's orbit.

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A total lunar eclipse is visible only from the path of totality.

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Why can neither Venus nor Mercury remain visible throughout the night as the full Moon does?

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Relative to the stars in the sky, the Sun moves

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Describe the evidence that best supports the Milankovitch hypothesis.

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  ​ The solar corona is shown as white lines streaming from the Sun and you are viewing it from Earth. Which eclipse are you observing? ​ The solar corona is shown as white lines streaming from the Sun and you are viewing it from Earth. Which eclipse are you observing?

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  ​ In the picture shown, in which hemisphere is the person located and the location of the Sun is above what geographic point on Earth? ​ In the picture shown, in which hemisphere is the person located and the location of the Sun is above what geographic point on Earth?

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Why don't eclipses occur at every new Moon and full Moon?

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Describe the difference between an umbral and a penumbral lunar eclipse as seen by an observer on Earth.

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The seasons are caused by the precession of Earth's axis.

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A dime is 1.8 cm in diameter. Earth's Moon is 3.844 × 1010 cm from Earth and has a diameter of 3.76 × 108 cm. At what distance from your eye would you have to hold a dime so that it has the same angular diameter as the full Moon?

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A waxing crescent Moon is visible

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Assume all else is unchanged, and the Earth's rotational axis is perpendicular to the ecliptic. As a result, seasonal variations on the Earth would

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