Well, we could have a bar showing a unit of angles we know how big it is. Peak sensitivities in nm for what is shown in the RGB channels. Hard to quite brightness in meaningful units, but we sort-of know how a galaxy is supposed to look.
The general public doesn’t know enough about the details of infrared astronomy to make use of that information. That’s why it’s at the bottom of the page.
My favourite joke from this was that it proves the monkeys and typewriters theory: give the universe 13bn years and it will eventually replicate a frame from a low-budget animation…
Yes! Based on the image data, can the actual locations of the gravitational lens “distorted” galaxies be determined and thereby be shown “correctly”, however simply in some graphic?
Yep. I agree: the average punter may not know much about infrared astronomy. They will probably not know that the pictures they are see are not what they would see if the Webb had an eyepiece. But they won’t ever question what they are shown if we don’t provide a bit of extra information. And that might lead to a more general understanding. And us nerds want to share.
This isn’t BoingBoing’s fault - everyone does it. We get pictures from Mars Orbiter showing blue patches and I don’t know how much they have dicked with the colours. Or colour enhanced pictures from Mercury or the Moon.
I actually find the diffraction spikes helpful - they are only visible about very bright objects, which are probably foreground stars. It would be weird if they weren’t there.