I wonder if a future evolution of space telescopes will be some kind of interferometric (obviously extremely hard for IR or visible light, but easier for radio and microwaves) swarm of cheap semi-disposible telescopes than one enormous one.
Then you can add to the swarm, upgrade elements, and retire failed elements without having to eat a multi-billion helping of humble pie.
And rather than have a fearsomely complex integrated sunshield, you could have a similar swarm of simpler satellites that provide a large cool area at L2, and then the observers just need to handle their own heat.
I suppose this could be described as microservices...in spaaaaace. Draw what parallels you will from that!
[1]: https://www.life-space-mission.com/ [2]: https://lisa.nasa.gov/
The image this article is about is mostly in the optical (MUSE only goes from 465nm to 930nm; and the synthetic filters used in the MUSE image [4] seem to be quite close to the used HST filters).
> And really only in the near-infrared, as past 5 microns, we can't really see through the atmosphere.
Not quite true [1] (at least if only considering absorption), it's just that the background becomes more and more of a problem (both continuum and narrow emission lines), and one has less nicely defined windows of transmission and lots of strongly variable absorption lines (picking dry places for the telescopes and selecting nights with low water vapour column densities helps). At the VLT for example there is VISIR [2], which does mid-IR imaging and spectroscopy.
Of course the sensitivty from the ground is much lower than from space or somewhere in between (for example there is SOFIA [3] which is a 2.5m telescope on an airplance) and some bands of interest are indeed absorbed. But there are indeed projects that involve mid-IR observations that can be done from the ground.
[1] https://www.gemini.edu/sciops/telescopes-and-sites/observing... [2] http://www.eso.org/sci/facilities/paranal/instruments/visir/... [3] https://en.wikipedia.org/wiki/Stratospheric_Observatory_for_... [4] https://www.eso.org/public/unitedkingdom/images/eso1824c/
I don't think past 5 microns there's been a lot of science done from the ground (not counting SOFIA). Practically, I think everyone is waiting for JWST. A lot of the interesting molecular lines also get absorbed by the Earth's atmosphere.
is that true? does this mean that we should simply use ground-based 'scopes with adaptive optics?
Is that a lot?
https://en.wikipedia.org/wiki/James_Webb_Space_Telescope [0]
Since the first hominids looked up at the stars, till literally yesterday, mankind had only one fundamental force to observe the universe with: electromagnetic waves, be it light, radio waves or infrared. From today, we have two. The other two remaining fundamental forces do not operate at astronomical scales.
Of course, we had LIGO before yesterday, but for me, the confirmation through electromagnetic wave observations is key. This is an historic day!
[1]: https://www.nasa.gov/feature/goddard/2016/nasas-fermi-telesc...