planetary science

Editor’s note: This story will be updated periodically.

A helicopter just flew on Mars. NASA’s Ingenuity hovered for about 40 seconds above the Red Planet’s surface, marking the first flight of a spacecraft on another planet.

In the wee hours on April 19, the helicopter spun its carbon fiber rotor blades and lifted itself into the thin Martian air. It rose about three meters above the ground, pivoted to look at NASA’s Perseverance rover, took a picture, and settled back down to the ground.

“Goosebumps. It looks just the way we had tested it in our test chambers,” Ingenuity project manager MiMi Aung said in a news briefing after the flight. “Absolutely beautiful flight. I don’t think I can ever stop watching it over and over again.”

As data from the flight started coming in to Ingenuity’s mission control room at NASA’s Jet Propulsion Lab in Pasadena, Calif., at about 6:35 a.m. EDT, a hush fell. And then cheers erupted as Håvard Grip, Ingenuity’s guidance, navigation and control lead, announced: “Confirmed that Ingenuity has performed its first flight, the first flight of a powered aircraft on another planet.”

NASA’s Ingenuity helicopter took this photo of its own shadow while hovering about three meters in the Martian air on April 19.JPL-Caltech/NASA

“It’s amazing, brilliant. Everyone is super excited,” said mechanical engineer and team member Taryn Bailey. “I would say it’s a success.”

The flight, originally scheduled for April 11, was delayed to update the helicopter’s software after a test of the rotor blades showed problems switching from preflight to flight mode. After the reboot, a high-speed spin test April 16 suggested the shift was likely to work, setting the stage for the April 19 flight.

“I never let you celebrate fully. Every time we hit a major milestone I’m like, not yet, not yet,” Aung told the team moments after the flight was confirmed. Now is the moment to celebrate, she said. “Take that moment and after that, let’s get back to work and more flights. Congratulations.”

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Ingenuity lifted into the thin Martian atmosphere for the first time on April 19, proving that flight is possible on another planet. This video was taken by the Perseverance rover, which watched from a safe distance away.

This first-ever flight was a test of the technology; Ingenuity won’t do any science during its mission, set to last 30 Martian days from the moment it separated from the rover, the equivalent of 31 days on Earth. But its success proves that powered flight is possible in Mars’ thin atmosphere. Future aerial vehicles on Mars could help rovers or human astronauts scout safe paths through unfamiliar landscapes, or reach tricky terrain that a rover can’t traverse.

“Technology demonstrations are really important for all of us,” said Thomas Zurbuchen, associate administrator for NASA’s Science Mission Directorate. “It’s taking a tool we haven’t been able to use and putting it in the box of tools we have available for all of our missions at Mars.”

Ingenuity’s flight was the culmination of more than seven years of imagining, building, testing and hoping for the flight team.

“That is what building first-of-a-kind systems and flight experiments are all about: design, test, learn from the design, adjust the design, test, repeat until success,” Aung said in a news briefing on April 9.

Aung and her team began testing early prototypes of a Mars helicopter in a 7.62-meter-wide test chamber at JPL in 2014. It wasn’t a given that flying on Mars would even be possible, Aung said. “It’s challenging for many different reasons.”

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Before it hitched a ride to Mars on the rover Perseverance, Ingenuity underwent extensive testing in a Mars simulator on Earth. Its engineers experimented with early prototypes and later with Ingenuity itself. These tests convinced the team that the craft could fly in Mars’ thin atmosphere.

Even though Mars’ gravity is only about one-third of Earth’s, the air’s density is about 1 percent that at sea level on Earth. It’s difficult for the helicopter’s blades to push against that thin air hard enough to get off the ground.

Another way to think about it is that the air is thinner on Mars than it is at three times the height of Mount Everest, Ingenuity engineer Amelia Quon of JPL said in the news briefing. “We don’t generally fly things that high,” Quon said. “There were some people who doubted we could generate enough lift to fly in that thin Martian atmosphere.”

So Quon and her team put the helicopter through a battery of tests over the course of five years. “My job … was to make Mars on Earth, and enough of it that we could actually fly our helicopter in it,” Quon said. The Mars simulation chamber could be emptied of Earth air and pumped full of carbon dioxide at Mars-like densities. Some versions of the helicopter were suspended from the ceiling to simulate Mars’ lower gravity. And wind speeds up to 30 meters per second were simulated by a bank of about 900 computer fans blowing at the helicopter.

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The final version of Ingenuity is light, about 1.8 kilograms. Its blades are longer (about 1.2 meters wingspan) and rotate faster (about 2,400 rotations per minute) than a similar vehicle would need to be able to fly on Earth. By the time the helicopter hitched a ride to Mars with the Perseverance rover in July 2020, the engineers were confident the helicopter could fly and remain in control at Mars (SN: 7/30/20).

Perseverance landed in a region called Jezero crater on February 18 (SN: 2/22/21). The helicopter was folded up beneath Perseverance’s belly under a protective shield until March 21.

Over  the next few weeks, Perseverance drove around to find a flat spot for Ingenuity to launch. Then Ingenuity slowly unfolded itself and was finally lowered gently to the ground beneath Perseverance on April 3. The rover drove away quickly to get Ingenuity out of its shadow and allow the helicopter to charge its batteries with its solar panel, giving it enough power to survive the freezing Martian night. 

Ingenuity arrived on Mars folded up under the Perseverance rover in a protective shield the size of a pizza box. After landing, Perseverance dropped the shield and slowly lowered Ingenuity to the ground, then drove away.JPL-Caltech/NASA

On April 8 and 9, Ingenuity unfolded its rotor blades and tested their ability to spin in preparation to take to the air. After trouble-shooting the software problem and retesting the rotor blades April 16, the flight got a green light for April 19. It was scheduled for roughly 3:30 a.m. Eastern Daylight Time on April 19, which corresponds to 12:30 p.m. Mars time, in the early afternoon. That gave the craft’s solar panel enough time to charge up its batteries for the flight. It was also a time when Perseverance’s weather sensors, called MEDA, suggested the average wind speed would be about six meters per second.

NASA’s Ingenuity helicopter tested its spinning rotor blades on April 8, a week and a half before taking flight in the thin Martian air for the first time.JPL-Caltech/NASA

Ingenuity had to pilot itself through the flight. That’s partly because of the communication delay — Mars is far enough from Earth that light signals take about 15 minutes to travel between the two planets. But it’s also because Mars’ thin air makes the helicopter difficult to steer. “Things happen too quickly for a human pilot to react to it,” Quon said.

Perseverance filmed the flight from about 65 meters away, at a spot named Van Zyl Overlook. Ingenuity also filmed the flight from its own perspective, with two sets of cameras: Its downward facing navigation cameras capturing the view below it in black and white, and its color cameras scanning the horizon.

Over several days, NASA’s Perseverance rover gently lowered the Ingenuity helicopter to the ground and then took this selfie with it on April 6 from about four meters away. The rover then drove off to a safe distance of 65 meters to get ready to watch Ingenuity’s first flight.MSSS/JPL-Caltech/NASA

Now that this first flight went well, the team hopes to take up to four more flights over the course of Ingenuity’s mission, possibly starting as soon as April 22. Each will be a little bit more daring and riskier, Aung said. “We are going to continually push all the way to the limit of this rotorcraft.” And each one will be a nail-biter: Just one bad landing could end things immediately. Ingenuity has no way to right itself after a fall.

That may be the way the mission ends, Aung admitted in the April 19 news briefing. “Ultimately, we expect the helicopter will meet its limit,” she said. Even if it eventually  wipes out in a crash, the engineering team will learn valuable information from how the helicopter eventually fails.

At the end of Ingenuity’s mission, Perseverance will drive off, leaving the little helicopter that could behind, and continue its own mission: to search for signs of past life in Jezero crater, and to store rocks for a future mission to return to Earth. More

Whether they’re made of methane on Saturn’s moon Titan or iron on the exoplanet WASP 76b, alien raindrops behave similarly across the Milky Way. They are always close to the same size, regardless of the liquid they’re made of or the atmosphere they fall in, according to the first generalized physical model of alien rain.

“You can get raindrops out of lots of things,” says planetary scientist Kaitlyn Loftus of Harvard University, who published new equations for what happens to a falling raindrop after it has left a cloud in the April Journal of Geophysical Research: Planets. Previous studies have looked at rain in specific cases, like the water cycle on Earth or methane rain on Saturn’s moon Titan (SN: 3/12/15). But this is the first study to consider rain made from any liquid.

“They are proposing something that can be applied to any planet,” says astronomer Tristan Guillot of the Observatory of the Côte d’Azur in Nice, France. “That’s really cool, because this is something that’s needed, really, to understand what’s going on” in the atmospheres of other worlds.

Comprehending how clouds and precipitation form are important for grasping another world’s climate. Cloud cover can either heat or cool a planet’s surface, and raindrops help transport chemical elements and energy around the atmosphere.

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Clouds are complicated (SN: 3/5/21). Despite lots of data on earthly clouds, scientists don’t really understand how they grow and evolve.

Raindrops, though, are governed by a few simple physical laws. Falling droplets of liquid tend to default to similar shapes, regardless of the properties of the liquid. The rate at which that droplet evaporates is set by its surface area.

“This is basically fluid mechanics and thermodynamics, which we understand very well,” Loftus says.

She and Harvard planetary scientist Robin Wordsworth considered rain in a variety of different forms, including water on early Earth, ancient Mars and a gaseous exoplanet called K2 18b that may host clouds of water vapor (SN: 9/11/19). The pair also considered Titan’s methane rain, ammonia “mushballs” on Jupiter and iron rain on the ultrahot gas giant exoplanet WASP 76b (SN: 3/11/20). “All these different condensables behave similarly, [because] they’re governed by similar equations,” she says.

The team found that worlds with higher gravity tend to produce smaller raindrops. Still, all the raindrops studied fall within a fairly narrow size range, from about a tenth of a millimeter to a few millimeters in radius. Much bigger than that, and raindrops break apart as they fall, Loftus and Wordsworth found. Much smaller, and they’ll evaporate before hitting the ground (for planets that have a solid surface), keeping their moisture in the atmosphere.

Eventually the researchers would like to extend the study to solid precipitation like snowflakes and hail, although the math there will be more complicated. “That adage that every snowflake is unique is true,” Loftus says.

The work is a first step toward understanding precipitation in general, says astronomer Björn Benneke of the University of Montreal, who discovered water vapor in the atmosphere of K2 18b but was not involved in the new study. “That’s what we are all striving for,” he says. “To develop a kind of global understanding of how atmospheres and planets work, and not just be completely Earth-centric.” More

As our planet orbits the sun, it swoops through clouds of extraterrestrial dust — and several thousand metric tons of that material actually reaches Earth’s surface every year, new research suggests.

During three summers in Antarctica over the past two decades, researchers collected more than 2,000 micrometeorites from three snow pits that they’d dug. Extrapolating from this meager sample to the rest of the world, tiny pebbles from space account for a whopping 5,200 metric tons of weight gain each year, researchers report in the April 15 Earth and Planetary Science Letters.

Much of Antarctica is the perfect repository for micrometeorites because there’s no liquid water to dissolve or otherwise destroy them, says Jean Duprat, a cosmochemist at Sorbonne University in Paris (SN: 5/29/20). Nevertheless, collecting the samples was no easy chore.

First, Duprat and colleagues had to dig down two meters or more to reach layers of snow deposited before 1995, the year when researchers set up a field station at an inland site dubbed Dome C. Then they used ultraclean tools to collect hundreds of kilograms of snow, melt it and sieve the tiny treasures from the frigid water.

To hunt for micrometeorites that have fallen to Antarctica in recent decades, researchers dig trenches (pictured) to collect snow that is later melted and then sieved for the space dust.J. Duprat, C. Engrand, CNRS Photothèque

In all, the team found 808 spherules that had partially melted as they blazed through Earth’s atmosphere and another 1,280 micrometeorites that showed no such damage. The particles ranged in size from 30 to 350 micrometers across and all together weigh mere fractions of a gram. But the micrometeorites were all found within three areas totaling just a few square meters, the merest fraction of Earth’s surface. Assuming that particles of space dust are just as likely to fall in Antarctica as anywhere else let the team estimate how much dust fell over the entire planet.

The team’s findings “are a wonderful complement to previous studies,” says Susan Taylor, a geologist at the Cold Regions Research and Engineering Laboratory in Hanover, N.H., who was not involved in the new study. That’s because Duprat and colleagues found a lot of the small stuff that would have dissolved elsewhere, she notes.

About 80 percent of the micrometeorites originate from comets that spend much of their orbits closer to the sun than Jupiter, the researchers estimate. Much of the rest probably derive from collisions of objects in the asteroid belt. All together, these tiny particles deliver somewhere between 20 and 100 metric tons of carbon to Earth each year, Duprat and colleagues suggest, and could have been an important source of carbon-rich compounds such as amino acids early in Earth’s history (SN: 12/4/20). More

Seventeen tiny particles recovered from a flat-topped mountain in eastern Antarctica suggest that a space rock shattered low in the atmosphere over the ice-smothered continent about 430,000 years ago.

The nickel- and magnesium-rich bits were sifted from more than 6 kilograms of loose sediments collected atop the 2,500-meter-tall summit of Walnumfjellet, says Matthias van Ginneken, a cosmochemist at the University of Kent in England. Their exotic chemistry doesn’t match Earth rocks, but it does match the proportions of elements seen in a type of meteorite called a carbonaceous chondrite, van Ginneken and his colleagues report March 31 in Science Advances.

Most of the particles range in size from 0.1 to 0.3 millimeters across, and more than half consist of spherules that are fused together into odd-shaped globs. The elemental mix in the spherules closely matches that of particles found at two other far-flung sites in Antarctica— one more than 2,750 kilometers away — which suggests that all of the materials originated in the same event. Because the other particles were found in ice cores and dated to about 430,000 years ago, the team presumes that the newly found particles from Walnumfjellet fell then too.  

The chemistry of nickel- and magnesium-rich spherules (pictured) found on a mountaintop in Antarctica match that of a certain type of stony meteorites.Scott Peterson/micro-meteorites.com

The chemistry of nickel- and magnesium-rich spherules (pictured) found on a mountaintop in Antarctica match that of a certain type of stony meteorites.Scott Peterson/micro-meteorites.com

The meteor that broke up over Antarctica was between 100 to 150 meters across, the team’s simulations suggest, and probably burst at low altitude. Blast waves may have pummeled a 100,000-square-kilometer area of the ice sheet, the team estimates. The explosion left no crater, but peak temperatures where the plume of hot gases reached Earth’s surface would have hit 5,000° Celsius and may have melted up to a few centimeters of ice. A similar airburst over a densely populated area today would result in millions of casualties and severely damage an area hundreds of kilometers across (SN: 5/2/17). More

This is what it looks like to land on Mars.
NASA’s Perseverance rover took this video on February 18 as a jetpack lowered it onto the Red Planet’s surface.
“It gives me goosebumps every time I see it,” said engineer David Gruel of NASA’s Jet Propulsion Laboratory in Pasadena, Calif., at a news briefing on February 22.
The movie begins with the rover’s parachute opening above it as the rover and its landing gear enter the Martian atmosphere. Seconds later, a camera on the rover’s underside shows the heat shield falling toward the ground. If you look carefully, you can see one of the springs that pushed the heat shield off the rover came loose, said NASA engineer Allen Chen, the rover’s entry, descent and landing lead.
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NASA’s Perseverance rover captured video of its own landing using a set of cameras on the back of the entry vehicle, the sky crane and the rover itself.
“There’s no danger to the spacecraft here, but it’s something we didn’t expect, and wouldn’t have seen” without the videos, he said.
The rover filmed the ground coming closer and closer, getting glimpses of a river delta, craters, ripples and fractured terrain. Cameras on the top and bottom of the rover captured clouds of dust billowing as the rover’s jetpack, the sky crane, lowered it down to the ground on three cables. A camera on the sky crane showed the rover swinging slightly as it descended. Finally, the sky crane disconnected the cables and flew away, leaving Perseverance to begin its mission.
“It’s hard to express how emotional it was and how exciting it was to everybody” to see the movie for the first time, said deputy project manager Matt Wallace. “Every time we got something, people were overjoyed, giddy. They were like kids in a candy store.”
The movie looks so much like animations of the sky crane landing technique that NASA had released in the past that it almost doesn’t look real, says imaging scientist Justin Maki. “I can attest to, it’s real,” he says. “It’s stunning and it’s real.”

The rover also captured audio from the surface of the Red Planet for the first time, including a gust of Martian wind.
Perseverance landed in an ancient lakebed called Jezero crater, about two kilometers from what looks like an ancient river delta feeding into the crater (SN: 2/18/21). The rover’s primary mission is to search for signs of past life and to cache rock samples for a future mission to return to Earth.
The first images Perseverance sent back from Mars showed its wheels on a flat expanse. The ground is strewn with rocks that are shot through with holes, said deputy project scientist Katie Stack Morgan in a news briefing on February 19.
“Depending on the origins of the rocks, these holes could mean different things,” she said. The science team thinks the holes could be from gases escaping volcanic rock as lava cooled, or from fluid moving through the rock and dissolving it away. “Both would be equally exciting for the team.”

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All eyes are on Mars — and all ears, too. When NASA’s Perseverance rover touches down on the Red Planet on February 18, the landing will be recorded with sight, sound and maybe even touch.
The rover will cap off a month of Mars arrivals from space agencies around the world (SN: 7/30/20). Perseverance joins Hope, the first interplanetary mission from the United Arab Emirates, which successfully entered Mars orbit on February 9; and Tianwen-1, China’s first Mars mission, which arrived on February 10 and will deploy a rover to the Martian surface in May.
NASA will broadcast Perseverance’s landing on YouTube starting at 2:15 p.m. EST. The actual moment of touchdown is expected at approximately 3:55 p.m. EST. Perseverance is designed to explore an ancient river delta called Jezero crater, searching for signs of ancient life and collecting rocks for a future mission to return to Earth (SN: 7/28/20).
The rover will use the landing system pioneered by its predecessor, Curiosity, which has been exploring Mars since 2012 (SN: 8/6/12). But in a first for Mars touchdowns, this rover will record its own landing with dedicated cameras and a microphone.
As the craft carrying Perseverance zooms through the thin Martian atmosphere, three cameras will look up at the parachute slowing it down from supersonic speeds. When a rocket-powered “sky crane” platform lowers the rover to the ground, a fourth camera on the platform will record the rover’s descent. Another camera on the rover will look back up at the platform, and a sixth camera will look at the ground.
Perseverance will use the “sky crane” landing system pioneered by its predecessor, Curiosity. The landing involves dangling the rover from a floating platform on cables and touching down directly on its wheels.JPL-Caltech/NASA
Perseverance will use the “sky crane” landing system pioneered by its predecessor, Curiosity. The landing involves dangling the rover from a floating platform on cables and touching down directly on its wheels.JPL-Caltech/NASA
“The goal is to see the video and the action of getting from high up in the atmosphere down to the surface,” says engineer David Gruel of NASA’s Jet Propulsion Laboratory in Pasadena, who was the engineering lead for that six-camera system, called EDL-Cam. He hopes every engineer on the team has an image of the rover hanging below the descent stage as their computer desktop background six months from now.
Because it will take more than 11 minutes for signals to travel between Earth and Mars, the cameras won’t stream the landing movie in real time. And after Perseverance lands, engineers will be focused on making sure the rover is healthy and able to collect science data, so the landing videos won’t be among the first data sent back. Gruel expects to be able to share what the rover saw four days after landing, on February 22.

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Perseverance will also carry microphones to record first-ever audio of a Mars landing. Unlike the landing cameras, the microphones will continue to work after touchdown, hopefully helping the engineering team keep track of the rover’s health. Motors sound different when they get clogged with dust, for instance, Gruel says. The team will hear the sound of the rover’s wheels crunching across the Martian surface, and maybe the sound of the wind blowing.
“Are we going to hear a dust devil? What might a dust devil sound like? Could we hear rocks rolling down a hill?” Gruel asks. “You never know what we might stumble onto.”
Sound will add a way to share Mars with people who have trouble seeing, Gruel notes. “It might appeal to a whole other element of the population who might not have been able to experience past missions the same way,” he says.
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Watch NASA’s live coverage of the Perseverance landing here starting at 2:15 p.m. EST.
Elsewhere on Mars, the InSight lander will be listening to the landing too (SN: 2/24/20). The lander’s seismometer may be able to feel vibrations when two tungsten weights that Perseverance carried to Mars for stability smack into the ground before the rover lands, geophysicist Benjamin Fernando of the University of Oxford and colleagues report in a paper posted December 3 to eartharxiv.org and submitted to JGR Planets.
“No one’s ever tried to do this before,” Fernando says.
The ground will move by at most 0.1 nanometers per second, Fernando and colleagues calculated. “It’s incredibly small,” he says. “But the seismometer is also incredibly sensitive.”
The team may be able to catch that tiny signal because they know exactly when and where the impact will happen. If the lander does pick up the signal, it will tell scientists something about how fast seismic waves travel through the ground, a clue to the details of Mars’ interior structure. And even if they don’t feel anything, that will put limits on the waves’ speed. “It still teaches us something,” Fernando says.
The InSight team hopes to also feel vibrations from Tianwen-1 when its rover touches down in May. “Detecting one would be great,” Fernando says. “Detecting two would be like, amazing.” More

Amino acids in a meteorite — Science News, December 5, 1970
[Researchers] present evidence for the presence of amino acids of possible extraterrestrial origin in a meteorite that fell near Murchison, Victoria, Australia, Sept. 28, 1969.… If over the course of time their finding becomes accepted … it would demonstrate that amino acids, the basic building blocks of proteins, can be and have been formed outside the Earth.
Update
Scientists confirmed in 1971 that the Murchison meteorite contained amino acids, primarily glycine, and that those organic compounds likely came from outer space (SN: 3/20/71, p. 195). In the decades since, amino acids and other chemical precursors to life have been uncovered in other fallen space rocks. Recent discoveries include compounds called nucleobases and sugars that are key components of DNA and RNA. The amino acid glycine even has been spotted in outer space in the atmosphere of comet 67P/Churyumov-Gerasimenko. Such findings bolster the idea that life could exist elsewhere in the universe. More

For the first time in almost half a century, scientists are going to get their hands on new moon rocks.
The Chinese space agency’s Chang’e-5 spacecraft, which landed on the moon around 10:15 a.m. EST December 1, will scoop up lunar soil from a never-before-visited region and bring it back to Earth a few weeks later. Those samples could provide details about an era of lunar history not touched upon by previous moon missions.
“We’ve been talking since the Apollo era about going back and collecting more samples from a different region,” says planetary scientist Jessica Barnes of the University of Arizona in Tucson, who works with lunar samples from the American and Soviet Union missions of the 1960s and 1970s. “It’s finally happening.”
Chang’e-5, the latest in a series of missions named for the Chinese moon goddess (SN: 11/11/18), took off from the China National Space Administration’s launch site in the South China Sea on November 23 and landed in volcanic flatlands on the northwest region of the moon’s nearside.

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The lander, equipped with a scoop and a drill, will collect about two kilograms of soil and small rocks, possibly from as deep as two meters below the moon’s surface, says planetary scientist Long Xiao of China University of Geosciences in Wuhan.
The spacecraft has to work fast. With no internal heating mechanism, it has no defenses against the extremely cold lunar night, which can reach –170° Celsius. The entire mission has to fit within one lunar day, about 14 Earth days.
After the lander collects the sample, a small rocket will bring the lander and the sample back to the orbiter perhaps as early as December 3, although the Chinese space agency has not released the official schedule.
Once in orbit, the moon material will be packaged into a return capsule and sent back to Earth. The capsule is expected to land in the Inner Mongolia region by December 17.
The last time new lunar samples were sent back to Earth was 1976, with the end of the Soviet Union’s Luna program. Between those missions and NASA’s Apollo missions, scientists on Earth have about 380 kilograms of moon material to study (SN: 7/15/19). “Perhaps for a long time people thought, been there, done that, when it comes to the moon,” Barnes says.
Two kilograms of new stuff might not sound like much next to what’s already in hand. But Chang’e-5 is returning samples from an entirely unexplored region. The landing site is in the Mons Rümker region in the northwest region of the nearside of the moon. Like the Apollo and Luna landing sites, Rümker is flat. “The engineering consideration is first, to be safe,” Xiao says.

All the Apollo and Luna missions visited ancient volcanic plains, where the rocks are between 3 billion and 4 billion years old. Rümker’s volcanic rocks are much younger, around 1.3 billion to 1.4 billion years old. In the ‘60s, scientists didn’t think the moon was still volcanically active that late. More recent studies from lunar orbit and from telescopes have suggested a more complicated volcanic past.
“With these new samples, we potentially add another pinpoint in our geologic history of the moon,” says Barnes. “We’ll get an idea of, what was the volcanic history like on the moon a billion years ago? That’s something we don’t have access to in the returned samples we already have.”
The Rümker region is also rich in potassium, rare-Earth elements and phosphorous, often called KREEP elements. Those elements were some of the last to crystalize out of the magma ocean that covered the young moon and can help reveal details of how that process happened. It’s an “exotic flavor” of material, says Barnes. “It’s a really different area, geochemically, to the rest of the moon.”
One of the biggest challenges for the mission will be drilling that material. The drill can’t change direction once it’s deployed, so it has to attempt to drill through anything directly below it. If the drill hits a large rock, it could fail. So the Chang’e-5 team is hoping for fine, loose soil, Long says.
Once the sample is back on Earth, it will be stored and cataloged at a curation center in Beijing. Then it will be distributed for scientists to do research.
“You can’t breathe easy on these types of missions until the samples are back and are safe in the curation place where they’re going to be held,” Barnes says.
The Chinese space agency plans to share samples with international scientists. A 2011 congressional rule makes it difficult for U.S. scientists to collaborate directly with China, so it’s unclear who will get to work with the rocks. But the discoveries that the new samples will enable go beyond international borders.
“It doesn’t matter who’s doing it,” says Barnes. “The whole world should be behind this mission and this endeavor. It’s a piece of history.” More