I don't think anyone posted anything here yet about the ESA's Euclid space telescope, which seems strange.

Anyway, it is the latest scientific instrument to join the James Webb telescope and others at the Sun-Earth Lagrange point 2 (L2), which on average is about 1.6 million kilometers (over a million miles) out in space. The L2 point is where the sun's and earth's gravitational forces create a spot where objects parked there always maintain a fixed distance in space from the earth, even while it orbits around the sun.
The Euclid telescope has a 1.2 meter main mirror, which is smaller then the James's Webb mirror, but it does use the same segmented Korsch-style mirror as Webb. It also has VIS and NISP instruments. The VISible camera is for visible light imagery used to measure shapes, while the Near-Infrared Spectrometer and Photometer (NISP camera) is for infrared shots that also measure the light being emitted by celestial objects in various bandwidths. Early test images from the instruments are both clear and detailed.
Euclid's goal is to scan about a third of the sky in six years, which will be far more than the Hubble telescope has done since first being put in to orbit. It will focus mostly on extra-galactic targets up to 10 billion light years away. It will create a 3D map of the universe's large-scale structures, which could help scientists unlock the secrets about dark matter and the earliest eons of the universe.
The ESA doesn't know for sure how long Euclid will last, but it has kept open the possibility of tacking on five years at the end of the primary mission. The Webb telescope will probably still be going strong when it's time for Euclid to call it a night. The perfect launch that it had helped Webb save fuel, boosting its expected life from ten to twenty years.
Below is an early test shot done using the Euclid's main mirror. It lacks the colorization and enhancement that has been shown in photos from the Jame's Webb. Eventually Euclid photo's will also be enhanced once various preliminary testing on the instrument is complete.