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Artemis: Why Are We Really Going Back to the Moon?

Science Vs · Wendy Zukerman — Angel Abbud-Madrid, Nicolle Zellner, Gregg Hallinan · April 9, 2026 · Original

Most important take away

The popular justifications for returning to the Moon — mining rare earths or helium-3, and using it as a “launching pad” to Mars — largely don’t hold up under scrutiny. The strongest real reasons are training for a future Mars mission and doing unique science (especially a far-side radio telescope that could peer into the universe’s Dark Ages and hunt for life on exoplanets), with national prestige still driving most of the political momentum.

Summary

Key themes

  • A new space race, not just science. With Artemis II circling the Moon and China, India, Japan, South Korea and dozens of new space agencies joining in, going back to the Moon is being framed by leaders (including President Trump) as a way to keep the U.S. “winning” in space. Much of the current push is political prestige, echoing the Apollo-era U.S.–Soviet rivalry.
  • The “lunar gold rush” is mostly hype. Rare earth elements (terbium, neodymium, dysprosium, yttrium, etc.) do exist on the Moon, but they aren’t actually rare on Earth — China just dominates current mining. On the Moon they’re diluted in regolith; Angel Abbud-Madrid compares it to collecting rainwater in Death Valley versus Seattle. Not worth it with today’s info.
  • Helium-3 is a bet on technology that doesn’t exist. Helium-3 could in theory fuel clean nuclear fusion (220 lbs could power Dallas for a year with only helium as “waste”), but we haven’t cracked controlled fusion. Investing in lunar mining for it now is premature.
  • The Moon as training ground, not launch pad. You don’t need the Moon to reach Mars (SpaceX plans to go direct), but NASA’s plan uses it as a “Catskills before Mount Everest” — a place to rehearse long-duration life support, fix broken toilets, test sleeping bags, deal with corrosive moon dust, and learn to live off the land before committing to a 6+ month Mars trip.
  • Water is the real lunar resource. If astronauts can find and extract water on the Moon, it provides drinking water and can be split into hydrogen and oxygen for rocket fuel — effectively a “gas station” that lets future missions escape Earth’s gravity well more cheaply.
  • The best scientific case is the far-side telescope. Caltech’s Gregg Hallinan is building FARSIDE (Farside Array for Radio Science Investigations of the Dark Ages and Exoplanets) — a ~10 km-wide radio telescope on the Moon’s far side, shielded from Earth’s radio noise and atmosphere. It could detect faint hydrogen radio signals from the cosmic Dark Ages (the billion-year gap after the Big Bang before stars formed) and search for magnetospheres around exoplanets as a biosignature.
  • Prestige projects still pay dividends. Even if motivated by a “pissing contest,” Apollo produced smaller computers, GPS, and memory foam, plus transformative views of Earth. Artemis is likely to do the same — the science and perspective shifts are real byproducts of geopolitical ambition.

Actionable insights

  • Don’t buy the lunar-mining narrative at face value. Rare earths and helium-3 are not near-term economic justifications; investment in terrestrial rare-earth recycling and fusion R&D is a better use of money today.
  • Judge Artemis on long-term capability, not single milestones. The value isn’t in one crewed landing but in the infrastructure (water extraction, dust mitigation, habitats) that makes Mars and deeper exploration feasible.
  • Watch the far-side science missions. Radio astronomy from the lunar far side is a genuinely unique capability — arguably the single scientific payoff that can’t be replicated anywhere else.
  • Expect geopolitical framing to dominate headlines. When officials talk about “winning” the Moon, read it as prestige and positioning; the actual deliverables worth tracking are water discovery, reusable lunar infrastructure, and science instruments.
  • Take the Earth-overview moments seriously. Imagery and firsthand awe from crews (Artemis II already producing “Moon Joy”) historically shift public attitudes about climate and fragility — a soft but real dividend of going back.

Chapter Summaries

  • Artemis II and Moon Joy. Four astronauts are flying around the Moon on Artemis II, farther than any humans have been. Global audiences (and host Wendy Zukerman) are moved by the imagery; in two years NASA aims to land people on the Moon for the first time in 50+ years.
  • Grandma’s question: why are we doing this? A flashback to 1969 via researcher Angel Abbud-Madrid frames the core question. Apollo was a Cold War contest; now a new race is on with China, India, and many others, and U.S. leaders openly cite “winning” as a reason to return.
  • The lunar gold rush — rare earths. Moon rocks do contain rare earth elements used in phones, EVs, and solar panels. But they’re not actually rare on Earth, and on the Moon they’re thinly distributed. Abbud-Madrid says it’s not currently worth going after them.
  • Helium-3 and fusion. Helium-3 is abundant on the Moon and could theoretically fuel clean fusion with only helium as waste. The catch: controlled fusion doesn’t work yet. Claims of staking lunar helium-3 are speculative; money is better spent elsewhere now.
  • Moon as stepping stone to Mars. Physicist Nicolle Zellner explains the Moon isn’t a literal launch pad but a training ground — closer (days vs. months), forgiving enough to learn long-duration life support. Artemis II has already revealed problems (broken toilet fixed by “space plumber” Christina Koch, too-warm sleeping bags).
  • Living on the Moon: dust and water. Future lunar bases must handle abrasive moon dust (Apollo astronauts described it blinding them and getting into everything) and find local water. Water can be split into hydrogen/oxygen for rocket fuel, creating a literal gas station above Earth’s gravity well.
  • The far-side telescope (FARSIDE). Caltech’s Gregg Hallinan wants a ~10 km radio array on the Moon’s far side to hear faint hydrogen signals from the Dark Ages — the gap between the Big Bang and the first stars — and to detect magnetospheres around exoplanets as a life indicator. Earth’s atmosphere blocks these signals, making the lunar far side uniquely suited.
  • Prestige projects, real payoffs. Hallinan argues Apollo began as a pissing contest but delivered profound science, technology spinoffs (GPS, smaller computers, memory foam), and a new view of Earth. Artemis will likely do the same — and the emotional “Earth as fragile oasis” moments may matter as much as the hardware.