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Fixed misspelled "ecliptic" in documentation.
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@@ -2053,7 +2053,7 @@ Moon visible from the Earth. It is caused by the imperfect tidal locking
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of the Moon's fixed rotation rate, compared to its variable angular speed
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of orbit around the Earth.
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This function calculates a pair of perpendicular libration angles,
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one representing rotation of the Moon in eclitpic longitude `elon`, the other
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one representing rotation of the Moon in ecliptic longitude `elon`, the other
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in ecliptic latitude `elat`, both relative to the Moon's mean Earth-facing position.
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This function also returns the geocentric position of the Moon
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expressed in ecliptic longitude `mlon`, ecliptic latitude `mlat`, the
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@@ -9779,7 +9779,7 @@ def Libration(time):
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of orbit around the Earth.
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This function calculates a pair of perpendicular libration angles,
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one representing rotation of the Moon in eclitpic longitude `elon`, the other
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one representing rotation of the Moon in ecliptic longitude `elon`, the other
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in ecliptic latitude `elat`, both relative to the Moon's mean Earth-facing position.
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This function also returns the geocentric position of the Moon
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