Where to mine 3He, on Earth or the Moon? Photo of the back and dark side of the moon, taken by NASA as the moon passed in between the spacecraft and Earth.
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Helium-3 – Should we go to the Moon to get it, or to Australia?

Gold Hydrogen recently announced the presence of elevated levels of helium-3 isotopes in its Ramsay prospect in South Australia. But what is helium-3 and why could this be an interesting find?

Helium has two stable iso­topes: Helium-4 (4He), which makes up 99.9998% of helium on Earth, and helium-3 (3He), present in absolute trace amounts. Whereas 4He forms continuously as a result of alpha par­ticle release during radioactive de­cay of uranium and thorium, 3He is slowly dissipating since its formation when the Earth came into existence. Due to its extreme rarity and unique properties, the 3He price is 140,000 times higher than the already high 4He price, amounting to USD 70.8 million/MCF.

What can Helium-3 be used for?

3He can be used as a clean, efficient fuel for nuclear fusion. A 1 GW fu­sion plant would require up to 100 kg of 3He on an annual basis to generate clean energy with zero to minimal ra­dioactive waste.

Where to get 3He?

Currently, the 3He available on the market is produced from tritium (3H) decay. Tritium is formed as a byprod­uct in nuclear reactors and aging nu­clear weapons. Tritium is a highly controlled material, and its production is not scalable enough to meet rising 3He demands. Therefore, mining 3He might be an easier solution.

The largest known source of 3He is the Moon, with its soils containing 3He thanks to exposure to solar wind for billions of years. Several compa­nies from the USA, Russia and China, are seriously looking into mining 3He from lunar regolith. However, average concentrations on the Moon are still low; 0.007g 3He per m3 of regolith.

Of course, lunar exploration is in its infancy and more prolific areas are bound to be discovered, but a decent terrestrial source that is much cheaper to mine will easily be able to compete. Hence, Gold Hydrogen had gas sam­ples from the Ramsay prospect tested for helium isotopic composition. One sample contained a concentration of 901 ppt (part per trillion) 3He, sig­nificantly elevated compared to the 7.2 ppt 3He in atmosphere, while the other samples were more in the atmos­pheric range.

The 3He/4He ratios of most sam­ples indicate that helium is generat­ed in the felsic crystalline basement by radioactive decay of uranium and thorium. Only the most enriched samples may have a component of intrusive mantle rocks, bringing pri­mordial 3He towards the surface. In other words, as of yet it does not look convincing that Gold Hydrogen is tapping a large 3He mantle source on the Yorke Peninsula of South Austral­ia. However, if large volumes of heli­um can be produced from the Ramsay prospect, combined with the high 3He price, this could still prove to be a novel and lucrative enterprise.

Source: Helium-3 Confirmed at Ramsay Project 

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