Relativity visualized

Space Time Travel

Does an extremely fast object look shortened?

fast lichtschnelle Stäbe laengs
Fig. 1: Watching rulers at rest and in motion. Left: approaching at 70% of the speed of light, middle: at rest, right: receding at 70% of the speed of light. All rulers have the same length when measured at rest, a length measurement of the moving rulers gives 71% of the rest length.
Rulers (0.7 c), MPEG1 320×240 (823 kB), MPEG1 640×480 (2.0 MB)
fast lichtschnelle Stäbe quer
Fig. 2: The same scene as in Fig.  1, here seen from the side. The rulers at the back move to the left hand side, the ones in front to the right hand side, the ones in the middle are at rest.
Rulers (0.7 c), MPEG1 320×240 (790 kB), MPEG1 640×480 (1.8 MB)

Suppose we had space ships at our disposal that could reach nearly the speed of light - would a flying space ship look shortened? Should we expect that the faster they go, the shorter they look? It turns out that things are a little more complicated. This was first pointed out by Anton Lampa in 1924 [1]. A computer simulation illustrates Lampa's calculations (Fig. 1): The Rulers that approach us at high speed (left, 70% of the speed of light) look much longer than the rulers that move away from us at the same velocity (right). They even look longer than the rulers at rest (middle). It must be understood that all the rulers have the same length when measured at rest, exactly the width of a square on the checquered platform. In Fig. 2 we view the same scene from the side. All moving rulers appear shortened!

In order to understand the apparent shape of the moving rulers one must examine in some detail how this image is produced. The image of any object is generated by light that comes from the object and reaches the observer's eye or camera. The light has covered the distance between the object and the camera with finite, albeit very high velocity. Since some points on the object's surface are farther away from the camera than others, the light has travelled for a longer or shorter time, depending on its point of origin.

When the camera is triggered, it registers light that arrives at precisely this instant, simultaneously. This light has been emitted over a certain period, earlier or later according to its transit time. But during this period the object was in motion. Fig. 3 illustrates the consequences. Light which reaches the camera at a certain instant has been emitted by the approaching ruler over a period of time and the emission points therefore cover a region which is longer than the ruler itself; the ruler appears elongated. The elongation due to the light travel times even outweighs the relativistic length contraction: on approaching the camera, the ruler appears to be longer than at rest.

Conversely, when the ruler moves away from the camera, the light travel times let it appear shortened over and above the relativistic length contraction.

Only in the special case of motion exactly perpendicular to the line of sight, the light travel times from both ends of the ruler are the same and the length that we see is the length that we would measure. This is the case in the center of Fig. 2 as can be clearly seen by comparing the ruler length with the width of the background squares.

Stab längs Skizze
Abb. 3: A ruler approaches the camera at 90% of the speed of light. At this velocity its length is contracted to 44% of its rest length (see also the inset which shows the rest length of the ruler). Among all the light rays that reach the camera simultaneously, the ray coming from the far end of the ruler has been emitted first (a), the ray from the near end last (b). All the other emission points lie in between, on a line that is longer than the ruler itself (c, drawn in grey). Thin solid lines mark the distance already covered by the light ray, dotted lines indicate the remainder of the light path.
Rod (0.9 c), MPEG1 320×240 (604 kB), MPEG1 640×480 (1.5 MB)
 
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Authors: Ute Kraus, Date: July 14, 2005
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All contents copyright (C) 2001-2016 Ute Kraus, Corvin Zahn. All rights reserved. For more information see Copyright.