This effort is being planned for the 2025-2035 time frame.Existing ground-based telescopes, and various proposed Extremely Large Telescopes, can exceed the HST in terms of sheer light-gathering power and diffraction limit due to larger mirrors, but other factors affect telescopes.. 
Lẹhin mu iṣẹ sise igba die ni Weimar ni 1703 bi oṣere Fetini, Bach di alamọja ni Neue Kirche ni N' (1703-170).. 