The Electrical Design of a Membrane Antenna for Lunar-based Low-frequency Radio Telescope

TL;DR

This paper presents the design, simulation, and prototype testing of a lightweight, durable membrane antenna made from polyimide film for lunar low-frequency radio telescopes, capable of detecting cosmic dark age signals.

Contribution

It introduces a novel membrane antenna design optimized for lunar deployment, with high efficiency and broad frequency coverage, suitable for large-scale cosmic observations.

Findings

Efficiency >90% in 12-19 MHz range

Prototype electrical properties match simulations

Omni-directional pattern suitable for cosmic signal detection

Abstract

Detecting primordial fluctuations from the cosmic dark ages requires extremely large low-frequency radio telescope arrays deployed on the far side of the Moon. The antenna of such an array must be lightweight, easily storable and transportable, deployable on a large scale, durable, and capable of good electrical performance. A membrane antenna is an excellent candidate to meet these criteria. We study the design of a low-frequency membrane antenna for a lunar-based low-frequency (<30 MHz) radio telescope constructed from polyimide film widely used in aerospace applications, owing to its excellent dielectric properties and high stability as a substrate material. We first design and optimize an antenna in free space through dipole deformation and coupling principles, then simulate an antenna on the lunar surface with a simple lunar soil model, yielding an efficiency greater than 90% in the range of 12-19 MHz and greater than 10% in the range of 5-35 MHz. The antenna inherits the omni-directional radiation pattern of a simple dipole antenna in the 5-30 MHz frequency band, giving a large field of view and allowing detection of the 21 cm global signal when used alone. A demonstration prototype is constructed, and its measured electrical property is found to be consistent with simulated results using |S11| measurements. This membrane antenna can potentially fulfill the requirements of a lunar low-frequency array, establishing a solid technical foundation for future large-scale arrays for exploring the cosmic dark ages.