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The change in the right ascension of the Sun between June 21 and December 21 is approximately


A) 18 hours 0 minutes.
B) 0 hours 0 minutes.
C) 6 hours 0 minutes.
D) 12 hours 0 minutes.

E) None of the above
F) All of the above

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The daily and annual rhythms of the sky and Earth arise from all of these celestial motions EXCEPT


A) Earth's spin around its axis.
B) Earth's orbit around the Sun.
C) Moon's spin around its axis.
D) Moon's orbit around Earth.

E) B) and D)
F) C) and D)

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1 arcminute is equal to


A) 1/60 of a full circle.
B) 1/60 arcsecond.
C) 1/3600°.
D) 1/60°.

E) A) and D)
F) A) and C)

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The summer triangle, a group of three bright stars in the summer sky, consists of Deneb, Altair, and


A) Betelgeuse.
B) Vega.
C) Pollux.
D) Polaris.

E) C) and D)
F) A) and D)

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In general, a sundial is NOT a good timekeeper because the


A) Earth's orbital speed around the ecliptic is variable.
B) Earth's rotation rate changes throughout the year.
C) Sun's large angular diameter produces a fuzzy shadow.
D) sky is often cloudy.

E) None of the above
F) B) and C)

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Precession makes the spin axis of Earth move in a slow coning pattern. The end of the axis covers a complete circle in a period of


A) 2600 years.
B) 26 million years.
C) 26,000 years.
D) 1 year.

E) None of the above
F) All of the above

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By what approximate factor, in scientific notation, is a human being (height about 2 m) larger than the nucleus of a hydrogen atom, or proton (diameter about 10-15 m) ?


A) 2 × 1013
B) 2 × 1030
C) 2 × 10-15
D) 2 × 1015

E) All of the above
F) None of the above

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Why do the precise astronomical coordinates of right ascension and declination of a star change systematically night by night?


A) precession of Earth's spin axis
B) bending of light by Earth's atmosphere
C) They do not change because they are fixed positions on a star chart.
D) motion of Earth in its orbit around the Sun

E) B) and C)
F) A) and D)

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In the southern hemisphere, summertime occurs when


A) sunlight falls more directly on this hemisphere, heating it more than at other times of the year.
B) Earth's equator is parallel to the plane of its orbit.
C) sunlight falls less directly on this hemisphere, spreading the heat out over a greater area and thereby heating it more.
D) Earth is farthest from the Sun in its elliptical orbit.

E) A) and B)
F) A) and C)

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A full Moon will always be at its highest in the sky at about


A) sunrise.
B) midnight.
C) midday.
D) sunset.

E) B) and C)
F) B) and D)

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If an observer starts at Earth's South Pole and moves northward, at what latitude would Polaris first become visible?


A) It would always be visible.
B) 66.5S
C) 23.5S
D) at the equator

E) All of the above
F) A) and B)

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In the system of celestial coordinates that matches latitude and longitude upon Earth, which is the coordinate that is equivalent to latitude?


A) precession
B) elongation angle
C) declination
D) right ascension

E) A) and D)
F) A) and C)

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In which direction does the Sun appear to move along the ecliptic over the course of a year, relative to the background stars?


A) west
B) northwest
C) southwest
D) east

E) A) and B)
F) C) and D)

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During which type of lunar eclipse does the Moon remain longest in Earth's shadow?


A) penumbral
B) partial
C) total
D) For all three types of eclipse, the Moon remains in Earth's shadow the same length of time.

E) B) and C)
F) A) and B)

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Where would an observer have to be to see the south celestial pole on the horizon?


A) about 1° away from the South Pole, to allow for Earth's precession
B) at the South Pole of Earth
C) at the North Pole of Earth
D) on the equator

E) B) and C)
F) A) and B)

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In a penumbral lunar eclipse,


A) no points on the Moon are shaded from the Sun, either totally or partially.
B) all parts of the Moon are partially (not totally) shaded from the Sun.
C) the entire Moon is shaded from the Sun.
D) some points on the Moon are totally shaded from the Sun while others are only partially shaded.

E) A) and D)
F) B) and C)

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Which way do observers move with respect to the background stars because of the revolution of Earth in its orbit around the Sun?


A) westward
B) northeastward
C) northwestward
D) eastward

E) A) and B)
F) All of the above

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What was the approximate value of the right ascension of the Sun this year on March 21?


A) no particular value because it can vary between 0 hours and 24 hours
B) 0 hours 0 minutes
C) 12 hours 0 minutes
D) 1 hour 0 minutes

E) A) and B)
F) A) and C)

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From Earth's North Pole,


A) the whole of the celestial sphere is visible at some time during the year.
B) only stars that are within 66.5° of the north celestial pole can be seen.
C) only half the celestial sphere can be seen on any clear night.
D) only stars that are 23.5° above the celestial equator can be seen.

E) A) and B)
F) All of the above

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Because of precession, how long will it be before the spin axis of Earth points toward the present pole star again?


A) at least 1 million years
B) 13,000 years
C) 26,000 years
D) 9 years

E) A) and C)
F) None of the above

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