A) the rotation period of the Moon about its axis
B) the rotation period of Earth about its axis
C) the period of Earth's motion around the Sun
D) the period of the Moon's motion around Earth
Correct Answer
verified
Multiple Choice
A) its own diameter or 1/2°
B) 4°
C) 1/10°
D) 13°
Correct Answer
verified
Multiple Choice
A) new
B) third quarter
C) first quarter
D) full
Correct Answer
verified
Multiple Choice
A) the equator.
B) the Tropic of Cancer.
C) the Tropic of Capricorn.
D) the prime meridian.
Correct Answer
verified
Multiple Choice
A) The star will always remain overhead since the Moon does not rotate on its axis.
B) 29 1/2 days
C) 365 1/4 days
D) 27 1/3 days
Correct Answer
verified
Multiple Choice
A) Archimedes.
B) Eratosthenes.
C) Aristotle.
D) Ptolemy.
Correct Answer
verified
Multiple Choice
A) reversing the direction of the Moon's rotation about its axis
B) changing the period of Earth's motion around the Sun
C) reversing the direction of Earth's motion around the Sun
D) reversing the direction of Earth's rotation about its axis
Correct Answer
verified
Multiple Choice
A) the length of a synodic month
B) the length of a sidereal month
C) the frequency of lunar eclipses
D) None of these would change.
Correct Answer
verified
Multiple Choice
A) not predictable from this information alone.
B) full.
C) new.
D) either first or last quarter.
Correct Answer
verified
Multiple Choice
A) from third quarter to new moon.
B) between the two positions when the Moon and the Sun are at right angles to each other during which new moon occurs.
C) from new moon to first quarter.
D) from first quarter to full moon.
Correct Answer
verified
Multiple Choice
A) measuring the angle between the Sun and Moon when the Moon is at first or third quarter.
B) calculating their orbital radii from their orbital periods around Earth, using Kepler's law.
C) noting the size of Earth's shadow on the Moon during a lunar eclipse.
D) estimating the positions of the Moon and Sun in the sky from different positions on Earth as they passed through the due south direction on the same day.
Correct Answer
verified
Multiple Choice
A) The length of a sidereal month varies slightly from one orbit to the next.
B) The length of a synodic month varies slightly from one orbit to the next.
C) The Moon's orbit changes slightly from one month to the next.
D) The appearance of the Moon seen from Earth varies significantly from one month to the next.
Correct Answer
verified
Multiple Choice
A) 6 A.M.
B) noon
C) 3 A.M.
D) 6 P.M.
Correct Answer
verified
Multiple Choice
A) The shape of the darkening across the Sun's disk during a solar eclipse always appeared circular.
B) The shape of Earth's shadow on the Moon during a lunar eclipse was always circular.
C) The Sun disappears below one horizon each day and reappears above the opposite horizon.
D) The shape of the eclipse shadow on Earth during a solar eclipse was always circular.
Correct Answer
verified
Multiple Choice
A) 19
B) 16.7
C) 18
D) 17.6
Correct Answer
verified
Multiple Choice
A) full.
B) waxing crescent.
C) waning gibbous.
D) dark, as always.
Correct Answer
verified
Multiple Choice
A) length of an eclipse cycle.
B) diameter of Earth.
C) relative distances of the Sun and the Moon.
D) precise distance between Alexandria and Syene in ancient Egypt.
Correct Answer
verified
Multiple Choice
A) waxing gibbous.
B) full.
C) waning gibbous.
D) waning crescent.
Correct Answer
verified
Multiple Choice
A) less than 45°.
B) 45°.
C) 86.5°.
D) 89.5°.
Correct Answer
verified
Multiple Choice
A) measuring the diameter of Earth by comparing the direction to the Sun at noon at two different points on Earth.
B) measuring the diameter of Earth by timing how long it took the Moon to traverse Earth's shadow during a lunar eclipse.
C) measuring the relative distances to the Sun and the Moon by timing the exact moments when the Moon was at first and third quarter.
D) measuring the distance to each of the known planets by timing how long it took the planet to orbit the Sun.
Correct Answer
verified
Showing 41 - 60 of 67
Related Exams