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54 Cards in this Set
- Front
- Back
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Constellation is Latin for
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Group of Stars
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There are __ recognized constellations
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88
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3 famous constellations:
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Orion
Ursa Major - the big dipper Ursa Minor - the little dipper |
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Name for "The North Star"
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Polaris
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It is always easiest to learn constellations by understanding their
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relative positions.
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Diurnal Motion:
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the rotation of the earth, this causes the stars to change during a night.
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Stars rise in the ____ and set in the ____.
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East, West
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________ is a star CLUSTER
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Pleiades
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_____ is a CONSTELLATION
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Orion
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Due to a __ degree tip of the earth's axis in respect to the sun, the sun doesn't follow the Celestial Equator
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23
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The path troughout the year is called the ________
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Ecliptic
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The ecliptic crosses the celestial equator at two points in the sky called the ______ and ________ equinox.
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Vernal and Autumnal Equinox (Mar. 21 and Sept. 21)
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The sun is above the Celestial Equator for ____ the year and below it during the other ____.
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Half, Half.
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The day the sun is the highest in the northern sky is called the ______ solstice
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Summer (June 21)
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The day the sun is the lowest is called the ______ solstace
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Winter (Dec 21)
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Summer officially starts on the summer ________.
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Solstice.
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Why is it warmer in the summer?
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In summer, the light is more direct.
In winter, the light is more spread out. |
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RA =
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Right ascension
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RA is measured about the Celestial Equator in units of _____, _______, and _______.
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Hours, minutes and seconds.
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There are __ hours around the sky.
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24
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The zero point is defined as the ______ equinox.
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Vernal
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Declination is measured in _______, _______, and _______.
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DEGREES, minutes and seconds.
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We measure the _____ above or below the Celestial Equator.
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ANGLE
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The celestial poles are at __ degrees N and S.
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90
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We can note the direction as either N or S, or by + or - T/F
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T
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The wobble and gravitational pull of the sun and moon on the earth causes the celestial poles and celestial equator to slowly change positions, this is called the:
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Precession of the Equinox.
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T/F - the Polaris was always the north star, and will continue to be so in the future.
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F
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The wobble has a period of __,___ years.
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26,000
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The Zenith:
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The point directly over your head
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The Meridian
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A line running through the zenith from the north to the south, this line is used to define sidereal (or Star) time.
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Solar Time means
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The time we base off of our watches
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Star time
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The time it takes the stars to go from due south to due south.
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Our current calendar system is the
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Gregorian Calendar
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If the moon passes throught eshadow of the earth it is a _____ Eclipse
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Lunar
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If the shadow of the moon moves across the earth's surface, it is _____ eclipse.
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Solar
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Umbra
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The shadow of the moon on the earth
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Penumbra
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The shadow outside the Umbra (less intense)
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The wobble has a period of __,___ years.
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26,000
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The Zenith:
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The point directly over your head
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The Meridian
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A line running through the zenith from the north to the south, this line is used to define sidereal (or Star) time.
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Solar Time means
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The time we base off of our watches
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Star time
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The time it takes the stars to go from due south to due south.
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Our current calendar system is the
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Gregorian Calendar
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If the moon passes throught eshadow of the earth it is a _____ Eclipse
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Lunar
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If the shadow of the moon moves across the earth's surface, it is _____ eclipse.
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Solar
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Umbra
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The shadow of the moon on the earth
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Penumbra
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The shadow outside the Umbra (less intense)
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There are 3 types of eclipses
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Total Solar
Partial Solar Annular Eclipse |
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Total Solar Eclipse
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Moon fully blocks the visible solar surface
You must be in the umbra to observe the solar atmosphere |
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Partial solar eclipse
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Only part of the sun is blocked
You must be in the penumbra to observe a partial eclipse |
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Annular Eclipse
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The moon is at apogee (furthest from the earth)
THe moon is not large enought to cover the solar disk at this distance The moon leaves a ring of the visible solar survace observable. |
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Why don't we see an eclipse every month?
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The moon doesn't orbit in the Earth-Sun plane, the orbit is tipped 5 degrees to that plane.
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The intersection of the earth's orbit is called the
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Line of Nodes
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Eclipses occur when line of nodes is closely lined up with the
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Earth-Sun orbital plane
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