While it is not feasible to send a probe to K2-18, the technological improvements over the last sixty years provides optimism future technological advancements here on Earth and for nearby space telescopes will compensate for this.
I will use three test cases.
(1) The astronomer Martin Schmidt's discovery of the mysterious object 3C-273 in 1963 where the spectral lines for hydrogen were found to the extremely redshifted.
(2) sjastro (status rank amateur astronomer) spectrum of 3C-273 using very modest equipment outperformed the technology astronomers had in 1963.
(3) JWST spectrum of the galaxy GN-z11 which is 13.1 billion light years distant, by comparison 3C-273 is 2.4 billion light years.
Case (1).
View attachment 363893These poor astronomers from the 1960s relied on a very noisy spectra and calculated the redshift with a comparison laboratory hydrogen spectrum.
Case (2)
The software converted the spectrum into an emission intensity vs wavelength graph and automatically found and identified the redshifted lines.
The difficulty was finding the object in the first place which was identified in the inset image as under its alternate name PGC 41121.
While Schmidt used the largest telescope at the time the 200 inch Hale telescope, the spectrum lines taken with a 10 inch telescope are far more identifiable as a CCD was used unlike the photographic emulsions of the time which suffered from reciprocity failure.
Case (3)
The extreme faintness of GN-z11 puts it way beyond the range anything Martin Schmidt or sjastro could with their respective equipment.
Finally some technological data for the three cases using AI to gather and analyse.