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Astronomy
THE EARTH-MOON-SUN SYSTEM
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Turning, or spinning, of a body on its axis
Rotation
Motion of a body, such as a planet or moon, along a path around some point in space
Revolution
Method of determining eclipses
Stonehenge
Very slow motion
Precession
Highest point in the sky
Zenith
When the sun has reached its zenith
Noon
Time interval from one noon to the next, which averages about 24 hours
Mean solar day
Time it takes for Earth to make one complete rotation (360 degrees)
Sidereal day
Direction to the sun, changes by almost what degree each day?
1 or One
Period of 23 hours, 56 minutes, and 4 seconds
Sidereal day
Average distance of Earth from the sun
150 million kilometers
Earth is closest to the sun
Perihelion
Perihelion occurs about what year?
January 3
Earth is farthest from the sun
Aphelion
Aphelion occurs about what year?
July 4
The apparent annual path of the sun against the backdrop of the celestial sphere
Ecliptic
The imaginary plane that connects Earth’s orbit with the celestial sphere
Plane
of the
ecliptic
Earth’s axis of rotation is tilted about
23.5
degrees
Earth has one natural satellite
Moon
Moon orbits Earth within a period of about
one month
The moon’s orbit is
elliptical
, its distance to Earth varies by about what percent?
6%
The moon is closest to Earth
Perigee
The moon is farthest from Earth
Apogee
Result of the motion of the moon and the sunlight that is reflected from its surface
Lunar phases
The cycle of the moon through its phases requires 29½ days, a time span
Synodic month
Apparent period of the moon’s revolution around Earth and not the true period, which takes only 27⅓ days
Sidereal month
Moon rotates on its axis only once every?
27⅓ days
Occurs during new-moon phases. When the moon moves in a line directly between Earth and the sun, it casts a dark shadow on Earth
Solar eclipse
Occurs during full-moon phases. The moon is eclipsed when it moves
within Earth’s shadow.
Lunar eclipse
During most
full-moon
phases, the shadow of Earth misses the moon
During a
new-moon
or
full-moon
phase, the moon’s orbit must cross the plane of the ecliptic for an eclipse to take place
Earth’s circular shadow can be seen moving slowly across the disk of the full moon
Total lunar eclipse
Moon is completely within Earth’s shadow, but it is still visible as a coppery disk
Totally
eclipsed
Long-wavelength light
Red
A total eclipse of the moon can last up to how many hours?
Four
See the moon slowly block the sun from view and the sky darken
Total solar eclipse
Total solar eclipses
Umbra
Partial eclipse
Penumbra