In astronomy and navigation, the celestial sphere is an abstract sphere with an arbitrarily large radius concentric to Earth. All objects in the sky can be conceived as being projected upon the inner surface of the celestial sphere, which may be centered on Earth or the observer. Test your knowledge of the sphere with the test below.
Celestial equator
Ecliptic
Celestial horizon
Horizon
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Zenith
The equinoxes
Right ascension
The celestial poles
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Equator
Celestial meridian
horizon
Altitude
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Right ascension
Declination
Azimuth
Altitude
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North celestial pole
Polaris
North pole
North Star
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Rise straight up in the east and set straight down in the west
Rise straight up in the west and set straight down in the east
circle around the sky parallel to the horizon
Set at 5:36 a.m. in the Summer months only
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Rise straight up in the east and set straight down in the west
Rise straight up in the west and set straight down in the east
Have equal amounts of darkness in the Summer months only
circle around the sky parallel to the horizon
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Ecliptic
Ecliptic plane
Celestial equator
equinox
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Mar. 21
Dec. 21
June 21
Depends on which hemisphere one is in
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Mar. 21
Dec. 21
June 21
Depends on which hemisphere one is in
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Back and forth along an arc
In a large ellipse pattern every 100 thousand years
Along the ecliptic
In a large circular pattern that takes 26 thousand years to complete
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Mar. 21
Dec. 21
June 21
Depends on which hemisphere one is in
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Constellation belt
Oort Cloud
Celestial sphere
Heliosphere
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Polaris
Pole Star
North Pole
All answers are correct
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Zenith
North Celestial Pole
Altitude
Polaris
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Right ascension
Declination
Meridian
North and South Celestial Pole
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It is a "pulsing" star, a Cepheid variable
Travels the path of the Sun Along the celestial sphere
Stays nearly in the same spot above the northern horizon year-round while the other stars circle around it
~434 light-years from Earth
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Some names will change throughout the centuries of astronomy
Of the retrograde motion of the stars
Precession of the Earth's axis will point away from its current position
The gradual slowing of Earth's rotation
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Climate change
The speed of rotation of Earth's axis
Earth's bulge at its equator
Gravitational attraction of the Moon and Sun
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The Sun intersects the Tropic of Cancer
When the ecliptic intersects the celestial equator in March
The Sun intersects the Tropic of Capricorn
When the ecliptic intersects the celestial equator in September
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Spring and Autumn equinox
Winter Solstice
Summer Solstice
New years day
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The Sun intersects the Tropic of Cancer
When the ecliptic intersects the celestial equator in March
The Sun intersects the Tropic of Capricorn
When the ecliptic intersects the celestial equator in September
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Zero hours is the same as 24 hours in right ascension
Zero hours right ascension is located at the autum equinox
Zero hours right ascension is located at the vernal equinox
Right acsension is measured in hours minutes and seconds
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The slower rotation speed of Earth during winter will cause day and night time length to increase
The orbit speed of Earth during summer will increase, because Earth is approaching the aphelion of its orbit, causing longer solar days
The tidal bulge of the Earth combined with the liquid iron core slows down the rotation speed
The orbit speed of Earth during summer will decrease, because Earth is approaching the aphelion of its orbit, causing shorter solar days
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Subsolar point
Equinox
Solstice
None of the answers
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True north
Magnetic north
Celestial north
Pacific Ocean plate
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Spring Equinox
Winter Solstice
Summer Solstice
Autumal Equinox
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Ecliptic
Ecliptic plane
Celestial equator
Aphelion and perihelion
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Celestial equator
Meridian
Zenith
Horizon
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