Online Astronomy eText: Galaxies and the Universe
Light-Travel Times and Cosmic Distances
(work in progress)

A gamma-ray burst which occurred "13 billion light-years away" from the Earth
(Gemini Observatory/NSF/AURA, D. Fox & A. Cucchiara (Penn State U.), and E. Berger (Harvard Univ.), apod090429)

     The object inside the circle is GRB 090423, the earliest supernova explosion observed as of April 23, 2009. The explosive death of a massive star caused a gamma-ray burst which was aimed almost directly at the Solar System, allowing it to be easily visible, despite its light having traveled 13 billion light-years to reach us. Given estimates of the age of the Universe in the range of 13.6 billion years, the supernova occurred only a little over 600 million years after the Big Bang, placing it in (almost certainly) the first generation of massive stars to live and die.

      When you read, as in the caption above, that an object is 13 billion light years away, and seen as it was only 600 million years after the Big Bang, what does that mean? How is it possible for that object to have gotten so far away in such a short time, when everything presumably started off very close together?
      The answer to these questions lies in what we mean when we say that something is 13 billion light years away. In general, such an object was not 13 billion light years away when the light by which we see it left it, nor is it that far away now. What it means is that it took 13 billion light years for the light by which we see it to get here.
      For a correct understanding of what is going on, we need to refer to relativity theory, which is beyond the scope of this discussion. (Later versions of this page will refer to such relativistic 'corrections' for the benefit of those who would like to see them, but this discussion relies only on a 'common-sense' approach, for the benefit of those who just want to understand the basic idea.)
      Saying that we see something 13 billion years away, only 600 million years after the formation of the Universe, means that the author of such a statement is using a value of 13.6 billion years as the time since the Universe began. But because of the expansion of the Universe, when we see an object of that sort, so far out in space that it is seen at nearly the beginning of the Universe, the space between us and the object would have been expanding away from us at 13/13.6 or 96% of the speed of light. Any given part of the space between here and there would have been expanding (in all directions) at a relatively slow rate, but with the very large distance between us and the object in question, the total expansion of the space between here and there would have added up to that huge value.
      Now according to Einstein's Theory of Special Relativity, light always travels through 'local' space (the space it is currently passing through) at the speed of light. But that does not mean that it is moving toward us at that rate, as we have to take into account the expansion of the space between us and that local space, which in this example is 96% of the speed of light. As a result, even though the light emitted by the burster would have been traveling toward us at the speed of light when it left the dying star (and at every moment since then), its net progress toward us would only have been at 4% the speed of light (the difference between its speed, and the expansion of space). As a result, its forward progress toward us would have been 25 times slower than expected, and it could have taken 13 billion years to get here, even if the object were only 4% as far away as the stated 13 billion light-year distance. In other words, even if the object was only 600 million light years away from us, if it were moving away from us at 96% the speed of light, it would have taken the light 13 billion light years to get here.
      The net result is that when the light from very distant objects left them, they were far closer than the light-travel time from there to here. The exact distance they had requires relativistic corrections, because in the example above, the light is only slowed by 96% in its progress toward us in the more distant portions of its path. As it gets closer to us, the expansion rate of the remaining space between us and it is slower and slower, so the forward motion of the light toward us becomes more nearly equal to the speed of light. But although the actual distance the object had when it emitted the light isn't quite the same as implied above, it is still far less than the light-travel time.
     It should also be noted that during the time the light was approaching us, the remnant of the object was continuing to move away from us, and in the 13 billion years since it emitted the light by which we see it, it has moved much further away than its original distance. In face, in this example, although less than billion light-years from us when it emitted the 13-billion-year-old light beam, it would now be nearly 50 billion light-years away.
     In other words, there are several cosmic distance scales which apply to such a situation. The simplest one to describe, and the one which is therefore generally used, is the time it took the light to get here (in this case, 13 billion years). However, the actual distance the object had when it emitted that light is much less than that value (if it was close to the 'edge' of the observable Universe at that time), and its current distance is much further (and in fact, may be beyond the current 'edge' of the observable Universe, so that we may never get to see it as it is now, no matter how long we wait).
      Finally, as far as how the object could get so far away in so short a time, the simplest sort of calculation (as done above) would place it only about 600 million light years away at the time its light was emitted, 600 million years after the Big Bang, so as long as it was close to the 'edge' of the Observable Universe, moving away from us at nearly the speed of light (due to the Universal expansion), there's no difficulty in imaging how it could get that far away. In addition, current theory proposes that there is a very short time, just under a millionth of a trillionth of a trillionth of a second, in which the Universe expanded far faster than the speed of light (this is referred to as the Inflationary Theory), so that things could have ended up much further away yet, even without nearly light-speed motions, once the initial Inflation ended. But that is another tale, for another page, and another time.

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