Originally posted by UncleVanya They mention the lack of a color filter gives 3x the resolution of a typical camera sensor of the same megapixels.
Virtually all astronomical imaging systems use monochromatic sensors. To make color images, or to isolate the light from a particular atom or molecule, color filters (sometimes quite narrowband - a few nm - for spectra lines) are used. A typical camera will have a filter wheel with anywhere from half a dozen or so up to perhaps 20 filters that can be rotated in front of the sensor, in a few seconds.
Originally posted by Michael Piziak Wouldn't it be neat if astronauts could do a space walk out to the Hubble, and give it a modern upgrade to the camera/sensor - ?
Not sure if you are kidding or not - but there have been several missions to repair/replace/upgrade Hubble cameras. (My wife is a Co-PI on one of these: STIS - Space Telescope Imaging Spectrograph, which went up in the 90s). The system is designed so that complete camera assemblies (about the size of a telephone booth - that's an anachronistic reference! Have you used a telephone booth lately!?) can be pulled out and replaced with another module. We lowly earthling DSLR users have interchangeable lens, whereas Hubble pretty much has a fixed lens (mirror!) and they change the camera as desired. Actually, HST has several "cameras" available at any one time which can be selected by a secondary mirror, as do all big earth-based telescopes, too. Typically, 3 or 4 instruments can be selected on a few minutes notice. Instruments can be swapped out during the daytime when it is time to put in a new camera (or whatever).
Once the Webb telescope is launched, there will be NO repair/servicing missions. Its orbit is such that it will be a million miles or so from earth, unlike Hubble in its few hundred mile high orbit.
Originally posted by Mooncatt Newer terrestrial telescopes are being developed with larger and flexible mirrors. They work by flexing the mirrors in a way that counteracts and cancels out those distortion waves by shining lasers into the atmosphere and creating artificial stars to track how the atmosphere is bending the light waves.
Actually,it is the (much smaller!) secondary mirrors which will be flexed, at rates around hundreds of times per second - you can't wiggle a multi-meter piece of glass that fast!