The reason for building the LCRT on the far side of the Moon would be to avoid interference faced by radio telescopes on the Earth's surface.[2] The Moon would block many sources of radio interference originating on Earth, and would avoid the problems that come from Earth's ionosphere at long radio wavelengths.[3]
If completed, the telescope would have a structural diameter of 1.3 km, and the reflector would be 350m in diameter.[4][5][6] Robotic lift wires and an anchoring system would enable origami deployment of the parabolic reflector.[7]
^Bandyopadhyay, Saptarshi; Lazio, Joseph; Goldsmith, Paul; McGarey, Patrick; Goel, Ashish; Rafizadeh, Ramin; Arya, Manan; Delapierre, Melanie; Chahat, Nacer; Stoica, Adrian; Quadrelli, Marco; Nesnas, Issa; Hallinan, Gregg; Jenks, Kenneth; Wilson, Ronald (9 March 2021). "Lunar Crater Radio Telescope (LCRT) on the Far-Side of the Moon"(PDF). Dropbox. California Institute of Technology. p. 1. Retrieved 18 December 2023.
Cite error: There are <ref group=lower-alpha> tags or {{efn}} templates on this page, but the references will not show without a {{reflist|group=lower-alpha}} template or {{notelist}} template (see the help page).