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Prospecting for lunar Helium-3 with a radio-frequency atomic magnetometer

I. K. Kominis, C. Kosmas

TL;DR

This paper addresses the challenge of prospecting for lunar He-3 by proposing a direct, in-situ measurement method using a radio-frequency atomic magnetometer to detect the dipolar magnetic field from thermally polarized He-3 spins in regolith. The approach combines regolith heating, pre-polarization in a strong field, and a compact rf-sensor in a lower holding field to enable detection of He-3 at around 5 ppb within about 5 minutes using a small, lightweight setup. The key contribution is a quantitative prospecting framework showing that a 200 g sample and a magnetometer with ~1 fT/√Hz sensitivity can achieve this detection threshold, with total apparatus mass <5 kg, volume ~1 L, and power around 1 kW. The practical impact is a low-cost, deployable instrument suitable for rover-mounted prospecting campaigns that could substantially improve the economic feasibility of lunar He-3 mining by identifying high-abundance regions.

Abstract

Mining $^3{\rm He}$ from lunar regolith has attracted significant interest in recent years due to the scarcity of $^3{\rm He}$ on Earth and its diverse applications, from cryogenics and medical imaging, to nuclear physics and future nuclear fusion. Given the stringent technical and economic challenges of mining lunar $^3{\rm He}$, precise prospecting is essential. Here we propose a prospecting methodology based on a radio-frequency atomic magnetometer, which can detect the dipolar magnetic field of thermally polarized $^3{\rm He}$ spins. With a 200 g regolith sample and an rf-magnetometer with sensitivity $1~{\rm fT/\sqrt{Hz}}$ we can detect $^3{\rm He}$ with abundance 5 ppb within a measurement time of just 5 min. The associated apparatus is lightweight and significantly more cost-effective than alternative measurement techniques. The proposed prospecting method is readily deployable and could substantially improve the technical and economic feasibility of mining lunar $^3{\rm He}$.

Prospecting for lunar Helium-3 with a radio-frequency atomic magnetometer

TL;DR

This paper addresses the challenge of prospecting for lunar He-3 by proposing a direct, in-situ measurement method using a radio-frequency atomic magnetometer to detect the dipolar magnetic field from thermally polarized He-3 spins in regolith. The approach combines regolith heating, pre-polarization in a strong field, and a compact rf-sensor in a lower holding field to enable detection of He-3 at around 5 ppb within about 5 minutes using a small, lightweight setup. The key contribution is a quantitative prospecting framework showing that a 200 g sample and a magnetometer with ~1 fT/√Hz sensitivity can achieve this detection threshold, with total apparatus mass <5 kg, volume ~1 L, and power around 1 kW. The practical impact is a low-cost, deployable instrument suitable for rover-mounted prospecting campaigns that could substantially improve the economic feasibility of lunar He-3 mining by identifying high-abundance regions.

Abstract

Mining from lunar regolith has attracted significant interest in recent years due to the scarcity of on Earth and its diverse applications, from cryogenics and medical imaging, to nuclear physics and future nuclear fusion. Given the stringent technical and economic challenges of mining lunar , precise prospecting is essential. Here we propose a prospecting methodology based on a radio-frequency atomic magnetometer, which can detect the dipolar magnetic field of thermally polarized spins. With a 200 g regolith sample and an rf-magnetometer with sensitivity we can detect with abundance 5 ppb within a measurement time of just 5 min. The associated apparatus is lightweight and significantly more cost-effective than alternative measurement techniques. The proposed prospecting method is readily deployable and could substantially improve the technical and economic feasibility of mining lunar .

Paper Structure

This paper contains 7 sections, 4 equations, 1 figure, 1 table.

Figures (1)

  • Figure 1: Schematic apparatus for measuring the abundance of $^3{\rm He}$ in regolith. Components are not drawn to scale. A regolith sample of mass $m_{\rm s}={\rm 200~g}$ is heated, and the extracted gases flow through a cold trap at $T_p=100~{\rm K}$. Then follows a polarizing magnetifc field $B_p=1~{\rm T}$, where $^3{\rm He}$ is thermally spin-polarized by flowing through a porous material designed to match diffusion time with longitudinal spin-relaxation time. Finally, the gas enters the measurement cell inside a smaller and homogeneous holding magnetic field $B_h=10~{\rm G}$. A free induction decay is induced, and the resulting oscillating magnetic dipolar field produced by $^3{\rm He}$ spins is detected by the radio-frequency magnetometer.