It does! This loss of energy is usually officially termed a cosmological redshift, and it’s an interesting combination of the way that light moves through space, and the nature of our Universe’s expansion.
Light behaves both as a particle and as a wave. Depending on the situation, it can be easier to talk about photons the light particle, or light waves- for travelling the vast distances of space, either works. However, light’s energy is very tightly tied to one of its more wave-like properties - its wavelength. Wavelength measures the distances between peaks, and can be used to measure the distances between ocean waves, or it can be used to very precisely measure the color of light reaching your eyes or a camera. The shorter the wavelength of light, the bluer the color. The bluer the light, the more energy it has, and things like gamma rays and X-rays have more energy still than anything our eyes can detect.
So let’s imagine that we have a space three feet long, and a flexible spring, almost three feet long. To reach from one edge of our space to the other, we’ll have to stretch the spring a little, but the distance between the coils won’t be very large. If we started to extend the spring, and suddenly found that our space had doubled in size, we’d have to stretch the spring much further, and the distance between coils would be much greater.
This is fundamentally what happens to light, as it travels through an expanding universe. The universe as a whole is expanding, meaning that the space between many galaxies is increasing. As light travels away from a galaxy, the Universe is continually expanding, meaning that the distance the light needs to travel is continually increasing as well. As space stretches out underneath a beam of light, its wavelength increases, and its energy decreases. Measuring this loss of energy is one of the main ways that distance is now measured in the Universe. This metric works well because we have a good sense (from other measurements) of how fast the Universe has been expanding, and what the energy loss should be for light which began its journey at an earlier time.
However, a trillion kilometers, on an astronomical standard, is still relatively small. A trillion kilometers is roughly a tenth of a light year (about five weeks of light travel time). This distance is sufficiently small that a more useful unit is the astronomical unit (au) which measures the distance between the Earth and the Sun. A trillion kilometers is about 10,000 au. On the scale of our solar system, this would stretch from the Sun to not quite out into the Oort cloud. This distance would put you way past Pluto, which orbits our sun at around 40 au from the Sun, and well past any hypothetical Planet 9, which is supposed to hang out around 200 au from the Sun.
As distant as these measures are, this measures only our very closest cosmic neighborhood, and in this regime, space is not expanding. Everything within our Galaxy is bound gravitationally to each other much more tightly than the expansion of the Universe can pull apart. The expansion is not so rapid that it is able to shear the Galaxy apart. Light’s loss of energy really only comes into play at much larger scales, far beyond the nearest galaxies.
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