Comet at 1000 km
blogs.esa.int
blogs.esa.int
There's a possibility all the volatile components have already been burned off by the solar wind (which is what causes the tail). That would make this either a very old, or very small comet. Or one that wasn't that icy to begin with.
The outgassing is mainly a function of the magnitude of the solar radiation (which varies quite a bit) and the cross section of the comet, so it's doubly variable and may outgas really far from the Sun if the conditions are right.
This comet's aphelion is around Jupiter, and comets have been observed with tails (from telescopes, not naked eyes! :P) at that distance. This comet probably is too small though.
See my other comment for a better explanation of why the tail wouldn't be visible in this image.
Here's a cool image of Comet Humason that was taken while it was near Jupiter in the 60s, it's pretty epic, one of the most awesome comets I came across in my studies, this image is from an obscure journal that I can't find now, but I found the image on a forum :P
http://foro.tiempo.com/index.php?action=dlattach;topic=12940...
Besides that, the comet tail is formed from the outgassing from the Sun-facing surface of the comet and then wrapped up in the magnetic field of the solar wind, so the bright stuff you see in the sky is usually something like 10 thousand (or more) kilometers away from the actual nucleus, the bright part you usually see from Earth around comet is the coma (nebulous gas) not the solid surface of the comet, with the tail extending out many hundreds of thousands of kilometers behind it, though technically the tail will extend as far as the solar wind carries it once it's entrained in it :)