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Terminology

Lunar Crater Radio Telescope

Illustration — Lunar Crater Radio Telescope 3D conceptual design • Illustration — Concept of operations for building LCRT The Lunar Crater Radio Telescope (LCRT) is a proposal by the NASA Institute for Advanced Concepts (NIAC) to create an ultra-long-wavelength (that is, wavelengths greater than 10 m, corresponding to frequencies below 30 MHz) radio telescope inside a lunar crater on the far side of the Moon. 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. 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.

Also recorded as LCRT

Lunar Crater Radio Telescope

Lunar Crater Radio Telescope illustration.

Saptarshi Bandyopadhyay · Public domain

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Illustration — Lunar Crater Radio Telescope 3D conceptual design • Illustration — Concept of operations for building LCRT The Lunar Crater Radio Telescope (LCRT) is a proposal by the NASA Institute for Advanced Concepts (NIAC) to create an ultra-long-wavelength (that is, wavelengths greater than 10 m, corresponding to frequencies below 30 MHz) radio telescope inside a lunar crater on the far side of the Moon. 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. 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.

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wikidata · Q89864671 · wikipedia · Lunar Crater Radio Telescope

In this article

  1. 01Origins and development
  2. 02Archives and collections
  3. 03Notes, references and evidence

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