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This engineering image represents a total of 32 hours of exposure time at several overlapping pointings of the Guider 2 channel. The observations were not optimized for detection of faint objects, but nevertheless the image captures extremely faint objects and is, for now, the deepest image of the infrared sky.
The unfiltered wavelength response of the guider, from 0.6 to 5 micrometers, helps provide this extreme sensitivity. The image is mono-chromatic and is displayed in false color with white-yellow-orange-red representing the progression from brightest to dimmest. The bright star (at 9.3 magnitude) on the right hand edge is 2MASS 16235798+2826079.
There are only a handful of stars in this image β distinguished by their diffraction spikes. The rest of the objects are thousands of faint galaxies, some in the nearby universe, but many, many more in the distant universe. Credit: NASA, CSA, and FGS team.
blogs.nasa.gov...
originally posted by: gspat
Can't wait for pics of the moon.
originally posted by: coamanach
Looks like a Hubble picture, but with the name Webb sticked to it.
I mean... I would have picked an iconic picture of Hubble, and shown what Webb can offer, by showing the same region, but with groovy details.
originally posted by: Soylent Green Is People
originally posted by: gspat
Can't wait for pics of the moon.
It might (technically) be able to image the moon, but it will never look that general direction.
Looking back at the moon would mean looking back toward the direction of the sun, and Webb does not want to do that. It will keep itself pointed away from the general direction of the sun (and hence the Moon) throughout its operational life.
Besides, the power of Webb does not come from high magnification. It comes from being able to detect infrared radiation with great sensitivity. The reason infrared was chosen for Webb is that it's target are mostly extremely distant objects -- such as distant galaxies.
The visible light that was emitted from those galaxies have travel so far while those galaxies are moving away from us (due to expansion of the universe) that the visible light wavelengths have become red-shifted to become infrared. So if we want to see that visible light that was emitted from those galaxies so many years ago, then we need to look in the infrared.
Webb's infrared can be used for other things, but looking at the Moon would almost certainly be better done from more powerful ground-based telescopes or (to avoid atmospheric distortion) from Lunar orbit -- like the Lunar Reconnaissance Orbiter, or LRO.
The LRO cameras have pictures of the moon with (in many cases) 30 cm resolution, which means LRO camera images are able to see a basketball-sized object on the Moon. That's better than Webb would be able to do. The link to the LRO camera images I posted above is zoomable, and allows you to see those basket-ball sized objects