Lecture Four

GA 201/1920-04-16/p038 ·1920-04-16 · English MediumMedium alignmentSome paragraph re-numbering between this translation and the German original — the locus may slip by a paragraph or two.
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Before one engages in Astronomy, one must educate oneself in a qualitative sense concerning that which moves in space, concerning the things that are interdependent in space. For one must be quite clear that Sun matter and any other matter—Earth matter for instance—can under no circumstances be brought into a simple relationship; because the matter of the Sun is, in comparison with the matter of the Earth, something absorbing and sucking, while the latter exerts pressure. The motions which express themselves in nutation are motions proceeding from the astral world, and not from anything that can be found in Newton's principles. It is just this Newtonism that has driven us so far into materialism, because it seizes on the uttermost abstractions. It speaks of a force of gravitation. The Sun, it says, attracts the Earth, or the Earth attracts the Moon; a force of attraction exists between these bodies, like some invisible cable. But if really nothing but this force of attraction existed, there would be no cause for the Moon to revolve round the Earth, or the Earth round the Sun; the Moon would simply fall on to the Earth. This would indeed have happened ages ago, if gravitation alone were acting; or the Earth would have fallen into the Sun. It is therefore quite impossible for us to look to gravitation alone for the means of explaining the imagined or actual motions of celestial bodies. So what do they do? Let us see! Here we have a Planet imbued with a constant desire to fall into the Sun—supposing we were to have the law of gravitation alone. But now we will suppose that this planet has at some time or other been given another force, a tangential force. This impetus acts with such and such a power, and the force of gravitation acts at the same time with such and such a power, so that eventually the planet does not fall into the Sun, but has to move along a line resulting from both forces.

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Cite: GA 201/1920-04-16/p038 · edition English