TOM JONES

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Back to the Moon: Why Send Humans There?

May 21, 2026 By TOM JONES 1 Comment

(Eighth in a series)

To summarize, there are at least three good reasons to go back to the Moon: It’s close. It’s interesting. And it’s useful.

These are traits that NASA has recognized, and the Congress and several presidents have chosen space policies to reap the benefits of those attributes for the nation. In the process of returning to the Moon, those traits will help expand the technical, scientific and economic abilities of the United States.

Why employ human explorers to derive value from the Moon? We could return to the moon with robots; in fact, we are doing so now—the Firefly “Blue Ghost” lander touched down in Mare Crisium in March 2025, carrying ten science experiments. Of late, the Chinese have joined the robotic exploration of the moon with landers, rovers, and even a sample return mission from the far side: Chang’e 6 in June 2024. NASA is stepping up its own pace by partnering with commercial companies for delivery of NASA and industry experiments to the Moon. Some probes will visit the Moon’s equatorial regions, others those attractive areas near the South Pole, trying to assess the ice resources in those shadowed, supercooled craters. Robots are key to paving the way for a human return.

Shadow of the Blue Ghost lander on the surface of Mare Crisium in March 2025 (Firefly Aerospace)

But in the late 2020s, humans still retain some advantages over robots. Humans are skilled and versatile explorers, as demonstrated during Apollo and through centuries of terrestrial voyages of discovery. Humans respond to and react quickly to sudden opportunity. We are flexible and calm enough to respond effectively to emergency situations. We don’t have to write a new software routine—and upload it to our brains–to respond promptly to and exploit a new discovery.

We are adaptable creatures: during Apollo, all the lunar landing astronauts—save one—were test pilots. Yet their ability to learn geology field exploration techniques, to observe, and to recognize surprising geologic phenomena on the Moon delivered a rich scientific return during the six successful landings.

In October 2007, astronaut Scott Parazynski of the STS-120 crew prepares to install the jerry-built “cufflinks” to stitch the torn P6 solar array panels together. (NASA)

A good example of human adaptability in space exploration was the performance of the STS-120 crew on an ISS construction mission in 2007. As the STS-120 crew commanded the unfurling of the solar array on the relocated P6 truss, frayed guide wires caused some of the accordion-like panels to tear apart. No existing robot—then or now–would have been able to invent and implement a fix that would repair the torn array and complete its deployment. But the crew, aided by their space station colleagues and inventive advice from Mission Control, used spare materials in the station and on the shuttle to create wire-and-sheet-metal “cufflinks;” these 18-inch-long stays would link the torn panels together and carry deployment loads. Cufflinks in hand, Scott Parazynski and Doug Wheelock donned spacesuits and went outside. Assisted by their shuttle and station crewmates, the pair clipped out the frayed wire sections and stitched together the array panels without tearing them further. When the team commanded the repaired array to extend, the reinforced panels stretched smoothly out to their full length, restoring the P6 solar array wing in a triumph for the space and ground teams.

The many successful upgrades of the Hubble Space Telescope by shuttle crews, the last one on STS-125 in 2009, are further examples of precision operations and improvisation that are beyond robotic software and hardware. If you want the best chance for success on your space expedition, having humans along really raises the success rate of that enterprise.

In May 2009, astronaut Michael Good, STS-125 mission specialist, rides Atlantis‘ remote manipulator system arm to the exact position needed for further upgrades to Hubble. (NASA, S125-E-009213)

Of course, going back to the Moon exposes the crew to elevated danger compared to low Earth orbit, and a human expedition costs a lot more than sending robots. We must weigh those costs against the benefits. I believe that humans have great advantages over a machine-only campaign to explore the Moon and learn how to exploit its resources.

Returning to the Moon with NASA and our international partners is today a firm national goal. That consensus was absent when I became an astronaut. President George H.W. Bush proposed a lunar return in 1990, but the Congress said no. President George W. Bush, after the Columbia accident in 2003, declared again that the U.S. would return to the Moon by 2020. But the Congress slow-walked his proposal, and his unwillingness to fight for its goals caused it to fizzle out as well: President Obama killed the Constellation Moon-return program in 2010.

Concept for the Constellation “Altair” lunar lander, circa 2009 (NASA)

The Artemis effort to send expeditions back to the Moon aims to explore and exploit the Moon’s commercial potential, just as the Lewis and Clark Expedition of 1804-1806 opened  the American West. Captains Lewis and Clark were ordered west by President Jefferson to explore and assess the transportation routes and commercial value of the Louisiana Purchase. Today, we’re once again dispatching a professional Corps of Discovery to our technological and economic frontier—the Moon—to expand the nation’s economy into cislunar space.

Next: Which Path Back to the Moon?

www.AstronautTomJones.com

Filed Under: blogs, History, Space

Back to the Moon: Tapping Lunar Energy Resources

May 7, 2026 By TOM JONES Leave a Comment

(seventh in a series)

Another invaluable lunar resource is energy. One side of the rotating Moon is always bathed in sunlight. If you’re near the equator, as at the Apollo 11 landing site, the Moon’s rotation would give you two weeks of sunlight and then two weeks of extreme cold and darkness. At the south pole, at the Moon’s rotation axis, the sunlight strikes the surface at a very shallow angle, slanting in from around the compass over the course of 28 days.

There are elevated spots near the lunar poles where the low-angle sunlight produces nearly continuous illumination. For example, at the circular crater called Shackleton, the oblique sunlight lights up part of the elevated rim, with the sun shining about 90 percent of the time. Thus, near the pole, you could set up a solar panel and produce power nearly all the time—a much better situation than at the equator, where one must store enough electricity to last through two weeks of darkness.

Shoemaker Crater sits nearly at the lunar south pole. Its rim stays nearly continuously illuminated by the slanting rays of the Sun. (ESA Smart 1)

A video here shows the varying illumination over the course of a single lunar month; much of the high terrain at crater rims remains sunlit for more than three weeks out of a month.

In this map of the lunar South Pole (below), the brighter tones show the greatest illumination over the course of a whole year (2026). The darker tones mean that sunlight is much reduced. But notice the bright rim of Shackleton, which is bathed in nearly continuous solar energy. Here on Earth, a rooftop solar panel will produce no electricity for roughly 12 hours out of 24. At Shackleton, you’d enjoy nearly round-the-clock illumination and power. Elevated crater rims, as at Shackleton, would be a very good spot to set up solar panels to power a base or operate a refinery turning water ice into fuel and life support gases.

Illumination map of the lunar South Pole. The shades of gray depict the amount of sunlight received during 2024–white represents greater illumination, and black means no illumination. The floors of many of the craters receive no sunlight at all — they’re permanently shadowed. Conversely, a small number of high spots on mountains and crater rims are in persistent sunshine. (NASA Goddard)

The Moon’s polar resources, then, include water ice and sunlight, two attractive  ingredients located close together at the sunlit rims and the adjoining shadowed crater interiors. As discussed earlier, the Moon’s familiar minerals can be used right away as construction materials: bricks, panels, walls, or radiation shielding. But down the road, the Moon’s more exotic elements and compounds are of interest.

The regolith contains elements like iron, very easy to separate. By dragging a magnet through the dirt, you’ll retrieve a lot of native iron carried in by meteorite impact. Thorium, a radioactive element, is an attractive fuel for nuclear fission reactors, enabling the fission process to make more fuel than it consumes. We might imagine the prospect in this century of importing reactor fuel to Earth from the Moon.

Another promising nuclear fuel is He-3, helium three, a rare isotope of helium. Its use in fusion reactors would enable a cleaner fusion reaction and moderate reactor temperatures. Advocates have proposed sifting and mildly heating the Moon’s regolith at large scale to extract enough helium-three to fuel those future nuclear fusion reactors, generating electricity here at home. Another He-3 application is as a coolant to chill quantum computing chips to temperatures near absolute zero, where they are fastest and most efficient.

Earth’s crust contains little He-3, and any of this light helium released from Earth rocks was able over the past four and a half billion years to largely escape from Earth’s atmosphere. In Earth’s mantle, the ratio of He-3 to He-4 (the most common He isotope) is only about 20 parts per million, and that extracted from crustal natural gas is some 70 to 240 parts per billion (roughly a thousand times lower). But on the Moon, He-3 is continually implanted into the regolith’s upper few meters by the solar wind. It’s present at a concentration in sunlit regions at up to 15 parts per billion—still not very plentiful.

Yet with current prices of about $20 million per kilogram, companies like Interlune see lunar helium-three as an attractive natural resource, one justifying a mining operation that would eventually sift a million tons of regolith to recover tens of kilograms of the isotope annually for return to Earth.

Concept for an Interlune Helium-3 mining operation. (Interlune)

The value of lunar He-3 depends on demand from quantum computing, and our ability to design practical fusion reactors—none exist today. Commercial fusion reactors always seem to be 20 years in the future.

That horizon reminds me of my astronaut career, during which a return to the Moon has always seemed 20 years in the future, too. But the Japanese and Chinese have also indicated interest in exploring the economics of eventually extracting helium-three from the Moon. If the mining and extraction process proves profitable, and we do manage to create fusion reactors to use helium-three, our energy supply problems are over. No more worries about carbon emissions, no more worries about mining fossil fuels, and a much-reduced nuclear waste challenge. Fusion would be a limitless energy source. But the promise of He-3 is many years from being realized.  

Next: Why Send Humans Back to the Moon?

www.AstronautTomJones.com

Filed Under: blogs, news, Space

Back to the Moon: A Useful World

May 1, 2026 By TOM JONES Leave a Comment

(sixth in a series)

The third reason for going back to the Moon is that it is useful. Water is the first of the resources on the moon we will tap—it’s like gold in space because of its scarcity outside Earth’s hydrosphere and atmosphere. If we can tap the Moon’s natural water, we can supply astronauts with drinking water, and they can breathe the oxygen released from water when electrolyzed. By storing hydrogen and oxygen from the Moon’s water, we will stockpile rocket fuel for lifting off the surface or filling the propellant tanks of craft headed outward into the solar system.

James Vaughan concept art for a solar-powered lunar ice mine in a shadowed polar crater. (Vaughan)

Water is present on the arid Moon today because the floors of many craters at its poles are in near-perpetual darkness, protected from the slanting sunlight by the raised crater rims. The shadowed floors of these craters radiate their heat directly to space and thus get very cold: below minus 300 degrees Fahrenheit. And as comet ice and water-rich asteroids have struck the Moon, their violent impacts vaporized rocks, liberated the water and created an ephemeral temporary lunar atmosphere, including that water vapor. Water molecules then migrated to and got stuck in those polar cold traps–the molecules condense onto the surface. That 4 billion years of accumulated impact water, along with implanted hydrogen from the solar wind, comprises a reservoir estimated at hundreds of millions of tons.

Blue highlights on the image show the distribution of surface ice at the moon’s south pole (left) and north pole (right), detected by NASA’s Moon Mineralogy Mapper instrument. (NASA)

In this image of the polar regions of the moon, the light blue dots show water ice deposits—the hydrogen, actually—detected from orbit by satellites. Water ice, when melted, can be broken down further by electricity into oxygen and hydrogen. Those elements are a powerful rocket fuel combination—hydrogen as the fuel and oxygen as the oxidizer. The next steps are to characterize in what form these water deposits exist inside the dark craters, and then test processes that can liberate the water for use in an outpost.

Let’s not forget the Moon’s dirt. The lunar soil has very useful properties that explorers can use to advantage. The Moon’s soils can be used as construction materials like bricks, panels, walls, or radiation shielding, moved and shaped by bulldozers or compressed into molds. Using a lawn-mower-sized microwave transmitter, a lunar paver can sinter the moon’s regolith, fusing the tiny iron particles mixed up in that dirt into a hard pavement. A robot paver could lay down a dust-free landing pad or a roadway for a cargo delivery rover.

Researchers from the Northwestern University in the US have demonstrated the ability to 3D-print structures with simulants of Martian and lunar dust. (NorthWestern University)

Here is a Northwestern University image of some simple tools, resembling Legos, made by a 3D printer from simulated lunar dust (the gray material) and simulated Mars regolith (in orange). This 3D printing technology (using a biopolymer binder) is getting better and more advanced every year. Another idea is to extract native iron from lunar regolith using electromagnets; with that iron, a small steel mill can produce beams, wires, struts, and structures for habitats and industrial mechanisms.  

After we build the first key elements of a lunar outpost, the moon’s more exotic elements and compounds are of interest. Blue Origin is conducting research aimed at using solar or nuclear energy to melt and electrolyze lunar regolith, liberating oxygen from the melt and extracting various metals like titanium, iron, and aluminum. The company’s Blue Alchemist project aims to transform regolith into solar power systems, breathable oxygen, propellant-grade oxygen for refueling, metals, and construction materials. Tests of the regolith melt process are underway in the company’s labs.

Blue Alchemy, a Blue Origin project, aims to use melted lunar regolith to extract silicon for Moon-produced solar panels and protective glass coatings. (Blue Origin)

Next: The Moon’s Useful Energy Resources

www.AstronautTomJones.com

Filed Under: blogs, news, Space

Back to the Moon: The Right Lunar Orbit

February 11, 2026 By TOM JONES 2 Comments

(third in a series)

As the Moon circles the Earth and both bodies make their way around the sun, we’d like to maintain near-constant communication between astronauts and their home planet. During Apollo, astronaut landings were restricted to the lunar near-side, in direct line-of-sight radio communication with Earth. Back then, the command module pilot would be out of touch for half of every orbit—an hour–as he circled the lunar farside. One way around that outage is a large, looping orbit called a near-rectilinear halo orbit (NRHO). That orbit has some favorable characteristics at the Moon. Its orbital plane around the Moon is nearly perpendicular to a line from Earth, and rarely carries a craft behind the Moon, so direct communications are nearly always possible. (Putting comm relay satellites in lunar orbit could also eliminate blockages and their communication problems.)

An example of an NRHO (WestEastSpace)

The NRHO is a big, loopy orbit, with an orbital period of about a week. At perilune the orbit is very close to the moon, while most of the orbit out to apolune and back gives one an excellent view of the moon and the distant Earth. From the halo orbit, we can with very little rocket energy drop down to an orbit favorable for landing, or just as easily rocket back to Earth.

The NRHO contrasts with Apollo’s low, equatorial orbit. Apollo orbited only about 60 miles above the moon, circling once every 2 hours. But that orbit severely limited where the Apollo spacecraft could take its astronauts, and it was quickly perturbed by the moon’s lumpy gravity field. The NRHO offers a well-behaved orbit that allows good communications back to Earth and is in sunshine nearly all the time (for power generation). It won’t carry us behind the moon and cut us off for long periods. And the orbit gives us access to orbits to access the surface at nearly any time and to nearly any place on the moon that we would like to go, not limited to sites near the equatorial plane at which the Apollo missions were targeted.

Exploded view of Orion spacecraft. Service module propellant tanks and main engine visible at left and lower right.

However, the NRHO has some drawbacks. An Artemis lander must use fuel to maneuver into a near-rectilinear halo orbit to meet Orion, and then use still more fuel to drop into a lower orbit for approach to landing. Further, a lander aborting from the Moon’s surface in an emergency might take as long as three and a half days to reach an Orion waiting in the NRHO. Unfortunately, Orion’s propulsion system, housed in its European-built service module, doesn’t have enough fuel to drop the spacecraft into a low lunar orbit to rescue a crew. Due to lift limitations of the SLS booster, Orion has just enough propellant to break out of its NRHO when it’s time for an Earth return. The pros and cons of an NRHO vs. a different, lower lunar orbit are worth further examination.

Nevertheless, reason number one for going back to the moon is that it’s accessible, and we should take advantage of that attribute, no matter what orbit we finally choose.

Next: The Moon is Interesting

www.AstronautTomJones.com

Filed Under: blogs, History, Media, news

Back to the Moon: Who Will Get There Soonest?

September 2, 2025 By TOM JONES Leave a Comment


In late August I talked with NewsNation on the accelerating competition between China and the U.S. to return to the Moon. NASA plans to speed up deployment of a lunar surface nuclear reactor, to power an outpost and resource extraction, are a good step forward, but the administration should be strongly supporting the Artemis lunar return missions, with a ~2027 lunar return on Artemis III (a stretch as the effort stands now). All China has to do for a “W” is to duplicate Apollo 11, while we attempt a much more ambitious lunar return with more people, longer stays, and long-term infrastructure. But greater complexity plus static budgets mean “slow.” Perceptions of global tech superiority matter; we need to change that pace–quickly.

My comments here (note–the nuclear commenter in the clip is incorrect; NASA is building a fission reactor):

https://www.youtube.com/watch?v=M0vOF89mLT0

Image mosaic of lunar south pole from Smart 1 orbiter (ESA)

Filed Under: blogs, news, Space

Back to the Moon: Which Nation Will Be There Soonest?

September 2, 2025 By TOM JONES Leave a Comment

In late August I talked with NewsNation on the accelerating competition between China and the U.S. to return to the Moon. NASA plans to speed up deployment of a lunar surface nuclear reactor, to power an outpost and resource extraction, are a good step forward, but the administration should be strongly supporting the Artemis lunar return missions, with a ~2027 lunar return on Artemis III (a stretch as the effort stands now). All China has to do for a “W” is to duplicate Apollo 11, while we attempt a much more ambitious lunar return with more people, longer stays, and long-term infrastructure. But greater complexity plus static budgets mean “slow.” Perceptions of global tech superiority are important; we need to change–quickly.

My comments here (note–the nuclear commenter is incorrect; NASA is building a fission reactor):

www.AstronautTomJones.com

**

Filed Under: blogs, news, Space

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March 26, 2025 By TOM JONES Leave a Comment

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