Some people like the FSS. Some people hate it. Others adore it, while the rest despise it.
You can't please everyone.
Personally, I'm not, not in love with it. If that makes any sense.
How would I do it? First, I'd look at the underlying technology.
The first necessary thing would be a detector or detectors.
A telescope array that can detect visible, infrared, and ultraviolet light, and other spectra like radio waves, etc...
And with the advent of gravitational interferometers, such as LIGO, a gravitational wave detector (miniaturized) can also get fitted. This can give an idea of where to point the telescope.
Other detectors such as a neutrino detecting tank, particle radiation from the sun, suns, or other bodies, and others can be fitted, but that might make the FSS overly complex.
Let's just start with a multi-spectral telescope, to cover EM radiation, and a gravitational wave interferometer to tell where significant masses exist.
The process would go as such:
You can't please everyone.
Personally, I'm not, not in love with it. If that makes any sense.
How would I do it? First, I'd look at the underlying technology.
The first necessary thing would be a detector or detectors.
A telescope array that can detect visible, infrared, and ultraviolet light, and other spectra like radio waves, etc...
And with the advent of gravitational interferometers, such as LIGO, a gravitational wave detector (miniaturized) can also get fitted. This can give an idea of where to point the telescope.
Other detectors such as a neutrino detecting tank, particle radiation from the sun, suns, or other bodies, and others can be fitted, but that might make the FSS overly complex.
Let's just start with a multi-spectral telescope, to cover EM radiation, and a gravitational wave interferometer to tell where significant masses exist.
The process would go as such:
- Let the interferometer run for a bit so that it can detect and orient where waves originate. This should be an automatic process that is run every time you jump into a system.
- Use the telescope(s) to point at wave sources to get a visual or spectral observation of the gravitational wave source. The longer the telescope is focused on the source the more data you gather until the complete object is resolved. This can also become a multi-crew process to cut down scan time.
Note: The closer you are to an object the more light you can collect (depending on the star's brightness as well), and the faster you can get details about the object.
And because you're only seeing one side of the object you can only gather data for that one side. If you want to get data on the other side, which might be completely different, or give you more information about the object, you have to travel so that you can see the other side of the object. There just is no way of getting around that. Pun not intended. - At a later time, the data can be further processed to discover new findings. You shouldn't have to be in the system to do this. You can be docked at a station or even floating in space.