Searching Rudolf Steiner Lectures by GA number (GA0323) Matches
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Query was: distance
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 Title: Astronomy Course: Lecture I
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 mechanics. They calculate distances, movements and forces.
 Title: Astronomy Course: Lecture II
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 element, simply the distance from the center of the Earth in
 Title: Astronomy Course: Lecture III
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 the mean distance from the central body). This Law, you see,
 distances.” Here then you have the Newtonian Law of
 inverse proportion to the squares of their distances apart.
 attraction decrease with the squares of the distances”,
 Title: Astronomy Course: Lecture VI
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 begin to get some notion of the great distance which men at
 not be uninteresting to compare how great is the distance
 Title: Astronomy Course: Lecture IX
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 of its distances (a + b) from the two foci remains constant.
 distances of any one of its points from two fixed points, the
 difference of the distances of any point of the
 in regard to its distances from A and B, and establish the condition
 that the two distances AM and BM multiplied together should
 and the distance AB, 2a. If we take the midpoint between a
 of a point whose distance from a fixed point remains
 its distances from two fixed points maintain a constant
 is somewhere in the infinite distance, as one says. Following
 according to the distance between B and M. But there is a
 infinite distance to the right and left. If we were to
 Title: Astronomy Course: Lecture X
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 surface, far way at some indeterminate distance
 a sphere surrounding the Earth at an indeterminate distance.
 the distance between them 2a; then any point of the curve
 to whether a, that is, half the distance between the foci, is
 equations to determine the distances of M from A and B.
 Title: Astronomy Course: Lecture XIII
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 the Earth in her movement, is to the distance of the fixed
 Title: Astronomy Course: Lecture XIV
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 certain distance from myself, the onlooker. Over it all I put
 we now call the distance of the Moon (I must not say, of the
 Title: Astronomy Course: Lecture XV
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 measured distances from two fixed points, and so that the
 quotient of the two distances is constant. This was our other
 I go out into infinite distances, makes its appearance
 Title: Astronomy Course: Lecture XVIII
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 is arriving there from some great distance and then making
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