Searching Rudolf Steiner Lectures by GA number (GA0323)
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- Title: Astronomy Course: Lecture I
- mechanics. They calculate distances, movements and forces.
- Title: Astronomy Course: Lecture II
- element, simply the distance from the center of the Earth in
- Title: Astronomy Course: Lecture III
- 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
- 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
- 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 mid-point 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
- 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
- the Earth in her movement, is to the distance of the fixed
- Title: Astronomy Course: Lecture XIV
- 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
- 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
- is arriving there from some great distance and then making
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