Einstein 1920: Space and Time

Reference: Einstein’s 1920 Book

This paper presents Part 1, Chapter 3 from the book RELATIVITY: THE SPECIAL AND GENERAL THEORY by A. EINSTEIN. The contents are from the original publication of this book by Henry Holt and Company, New York (1920).

The paragraphs of the original material (in black) are accompanied by brief comments (in color) based on the present understanding.  Feedback on these comments is appreciated.

The heading below is linked to the original materials.

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Space and Time in Classical Mechanics

“The purpose of mechanics is to describe how bodies change their position in space with time.” I should load my conscience with grave sins against the sacred spirit of lucidity were I to formulate the aims of mechanics in this way, without serious reflection and detailed explanations. Let us proceed to disclose these sins.

It is not clear what is to be understood here by “position” and “space.” I stand at the window of a railway carriage which is travelling uniformly, and drop a stone on the embankment, without throwing it. Then, disregarding the influence of the air resistance, I see the stone descend in a straight line. A pedestrian who observes the misdeed from the footpath notices that the stone falls to earth in a parabolic curve. I now ask: Do the “positions” traversed by the stone lie “in reality” on a straight line or on a parabola? Moreover, what is meant here by motion “in space”? From the considerations of the previous section the answer is self-evident. In the first place, we entirely shun the vague word “space,” of which, we must honestly acknowledge, we cannot form the slightest conception, and we replace it by “motion relative to a practically rigid body of reference.” The positions relative to the body of reference (railway carriage or embankment) have already been defined in detail in the preceding section. If instead of “body of reference” we insert “system of co-ordinates,” which is a useful idea for mathematical description, we are in a position to say: The stone traverses a straight line relative to a system of co-ordinates rigidly attached to the carriage, but relative to a system of co-ordinates rigidly attached to the ground (embankment) it describes a parabola. With the aid of this example it is clearly seen that there is no such thing as an independently existing trajectory (lit. “path-curve”1), but only a trajectory relative to a particular body of reference.

1 That is, a curve along which the body moves.

Einstein is pointing out that we see trajectory of a body relative to another body only and not independently.

In order to have a complete description of the motion, we must specify how the body alters its position with time; i.e. for every point on the trajectory it must be stated at what time the body is situated there. These data must be supplemented by such a definition of time that, in virtue of this definition, these time-values can be regarded essentially as magnitudes (results of measurements) capable of observation. If we take our stand on the ground of classical mechanics, we can satisfy this requirement for our illustration in the following manner. We imagine two clocks of identical construction; the man at the railway-carriage window is holding one of them, and the man on the footpath the other. Each of the observers determines the position on his own reference-body occupied by the stone at each tick of the clock he is holding in his hand. In this connection we have not taken account of the inaccuracy involved by the finiteness of the velocity of propagation of light. With this and with a second difficulty prevailing here we shall have to deal in detail later.

Just like space co-ordinates, each reference body must have its own time co-ordinates as well to complete the picture of motion.

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FINAL COMMENTS

Einstein notices that a reference system should provide not only its unique space co-ordinates but also its unique time co-ordinate. Time co-ordinate enters the picture because the reference bodies are themselves moving. The problem in classical mechanics has been that it has not been able to figure out a way to measure space and time in absolute co-ordinates.

But there may be a way if we look at time as endurance of change and inertia as resistance to change. The lesser is the inertia the more rapidly the changes shall occur. A reference body shall move faster on its own if its inertia decreases. This is actually observed when we compare the material domain to the field domain. The material domain has high inertia and low velocity, whereas, the field domain has low inertia and high velocity. If inertia could be measured in absolute terms, velocity may also be measured in absolute terms. This will allow absolute co-ordinates to be assigned to space and time.

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