Shogo Tachibana greeted asteroid Ryugu with dread.

The cosmochemist with the College of Tokyo had spent 10 years serving to to design a mission to Ryugu’s floor. To the touch down safely, the spacecraft, Hayabusa2, wants to search out broad, flat stretches of fine-grained mud on the asteroid. However on June 27, when Hayabusa2 finally reached its target after a three-and-a-half-year journey (SN On-line: 6/27/18), Tachibana obtained a impolite awakening: Ryugu is roofed in boulders. Huge ones.

“We can’t discover a 100 % secure place to the touch down,” Tachibana says. “It appears to be a really harmful place.”

If Hayabusa2 can cope with the boulders — and another challenges that come up — it can turn into solely the second spacecraft to deliver a chunk of an asteroid again to Earth. And the mission will reply questions that its predecessor couldn’t. The unique Hayabusa mission visited a sand- and rock-covered asteroid referred to as Itokawa in 2005. However Itokawa has the fallacious chemical make-up to handle massive questions concerning the origin of life that Ryugu, which is carbon-rich, is nicely fitted to. And Hayabusa suffered a collection of calamities that prompted it to return to Earth a number of years late, with lower than 2,000 grains of treasured asteroid mud.

Tachibana and colleagues from the Japanese Aerospace Exploration Company, or JAXA, are relying on Haybusa2 to return bits of Ryugu’s floor to Earth in 2020. And if a daring plan to blow a crater into the asteroid works, the spacecraft will get some subsurface grains as nicely.

A sister undertaking from NASA, the OSIRIS-REx mission, arrived at an asteroid called Bennu in December to deliver samples again in 2023 (SN On-line: 12/three/18).

The 2 spacecraft face daunting challenges. The probes should examine objects which have so little gravity that daylight can knock them off their orbits. If the probes handle to select up samples, the spacecraft should maintain the mud pristine in the course of the journey again to Earth. To get probably the most out of the missions, the Japanese and American groups are attempting to work collectively throughout cultural and bureaucratic divides.

New worlds

Ryugu and Bennu are small targets. Ryugu’s polar diameter is about 880 meters and Bennu’s is about 510 meters (left). Each asteroids orbit the solar on trajectories that typically take them comparatively near Earth (proper).

Two small asteroids… …with related orbits

C. Chang

Supply: Univ. of Arizona

However the uncertainties and anxiousness are value it. Asteroids like Ryugu and Bennu are among the many oldest and most intriguing objects within the photo voltaic system. They may maintain the keys to a number of the most urgent planetary questions: What got here earlier than the planets? What are the origins of life? And the way a lot of a menace do asteroids pose to life on Earth in the present day?

In fact, planetary scientists have already got tens of hundreds of asteroid items to check. Such meteorites fall to Earth within the lots of annually, providing researchers loads of materials to slice, grind and study for clues to the photo voltaic system’s historical past.

Dante Lauretta of the College of Arizona in Tucson, the principal investigator of OSIRIS-REx, spent the primary a part of his profession making an attempt to coax meteorites into telling him whether or not molecules crucial for all times — corresponding to nucleic acids, amino acids and phosphorus, that are structural elements of DNA — might have originated inside carbon-rich asteroids like Ryugu or Bennu.

Carbon-rich asteroids are considered largely unchanged since their formation not less than four.6 billion years in the past, which makes them excellent time capsules. Just a few grains of such an asteroid might reveal what the early photo voltaic system was fabricated from.

Distant research of asteroids additionally recommend that the uncooked components for all times, and perhaps even the chemical processes which can be crucial for all times to start, might need been current on carbon-rich asteroids even earlier than the planets had been finished rising.

“We expect an asteroid like this one could have delivered this materials to the floor of the early Earth, offering seeds or constructing blocks of life,” Lauretta says. “If we are able to present the precursors [of life] began earlier than the planet, I feel the likelihood that there’s life elsewhere within the photo voltaic system goes approach up.”

Learning meteorites to discover this notion falls brief on two fronts, nonetheless: It’s laborious to inform the place they arrive from, and so they’re contaminated. As quickly as an area rock hits Earth’s ambiance, it begins accumulating indicators of Earth life. Subsequently, any intriguing natural compounds in a meteorite could possibly be from Earth, not native to the asteroid. There’s no method to inform.

“We wanted samples of a carbon-rich asteroid to actually reply the questions I used to be into,” Lauretta says.

A uncommon breed

Of greater than 500,000 asteroids within the photo voltaic system, Ryugu and Bennu are two of solely 5 with the correct orbits, sizes and compositions for a sample-return mission.  

Supply: Univ. of Arizona

Break me off a chunk

Attending to the origins of the photo voltaic system, and perhaps life’s beginnings, makes bringing clear, rigorously chosen samples to earthly labs essential. However spacecraft can’t simply dig in with a shovel. There’s no grabbing a rock with a claw like in an arcade recreation. The asteroids are so tiny — Ryugu is about 880 meters from pole to pole and Bennu is about 510 meters — and their gravity is so weak that reaching out and grabbing one thing might push the spacecraft off target with the asteroid.

So as an alternative of scooping or grabbing, the spacecraft will attain out with proboscis-like tubes, both touching down briefly or hovering above the floor. This difficult endeavor has been tried solely as soon as earlier than — and it was virtually a catastrophe.

Drop and dodge

To pattern Ryugu beneath the floor, Hayabusa2 will launch a projectile to blast open a crater, then take a lap across the asteroid to keep away from injury. The spacecraft will then come near the brand new gap within the floor and shoot a small bullet from its sampling horn. The bullet will splash on the floor, sending mud and sand right into a catcher within the higher a part of the horn.  

Supply: JAXA

The primary Hayabusa spacecraft was supposed to make use of its three response wheels to stabilize itself because it hovered close to Itokawa’s floor, stretched out a group tube to the touch the floor and fired a small bullet down the tube to fire up mud particles. These mud grains would float up the tube right into a sterile chamber for storage on the journey again to Earth.

Nearly every thing went fallacious. Earlier than Hayabusa even obtained to the asteroid, the largest photo voltaic flare ever recorded broken the spacecraft’s photo voltaic panels and one in all its engines, slowing down the spacecraft and delaying its asteroid rendezvous by three months.

As soon as at Itokawa, two of the craft’s response wheels failed, making it laborious for the craft to maintain a fair keel. A companion rover launched by Hayabusa that was meant to land on Itokawa’s floor and measure the asteroid’s composition missed its mark and floated into house. The dust-stirring bullet didn’t fireplace, so it was initially unclear if the craft obtained any samples in any respect. And all 4 of the probe’s engines failed one after the other on the return journey, forcing Hayabusa to take a prolonged detour residence.

“It had a number of severe issues,” says JAXA’s Makoto Yoshikawa, a mission supervisor on each Hayabusa and Hayabusa2.

For all of Hayabusa’s calamities, the mission’s story had a contented ending. Towards all odds, the spacecraft returned to Earth in 2010 (SN On-line: 6/14/10), having grabbed 1,534 grains of Itokawa.

Planners of the brand new mission realized from the unique mission’s mishaps. Hayabusa2 has 4 response wheels, souped-up engines and a beefier communication system that may ship again rather more knowledge to assist scientists plan the pattern assortment. The gathering tube has tooth at its mouth to carry pebbles into the tube even when the bullet doesn’t fireplace. And in September, Hayabusa2 successfully dropped three small landers on Ryugu’s floor to collect knowledge on the asteroid’s composition, temperature and magnetic properties (SN On-line: 9/24/18).

With related warning, when OSIRIS-REx goes in to collect a pattern from Bennu, it can contact the asteroid solely briefly. “It’s like 5 seconds of contact,” Lauretta says. “Get the pattern after which get out of there.”

<img src="knowledge:picture/png;base64,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" data-echo="https://www.sciencenews.org/websites/default/information/2019/01/011919_LG_sample-return_inline4_730.jpg" alt class="caption" title="KEEP IT CLEAN  OSIRIS-REx’s sampler, referred to as the Contact-and-Go Pattern Acquisition Mechanism, or TAGSAM (photographed in a clear room), has a head on an arm that extends. ~~ Lockheed Martin”><img src="https://www.sciencenews.org/websites/default/information/2019/01/011919_LG_sample-return_inline4_730.jpg" alt class="caption" title="KEEP IT CLEAN  OSIRIS-REx’s sampler, referred to as the Contact-and-Go Pattern Acquisition Mechanism, or TAGSAM (photographed in a clear room), has a head on an arm that extends. ~~ Lockheed Martin”>

The spacecraft’s Contact-And-Go Pattern Acquisition Mechanism, TAGSAM, has a nitrogen jet on the finish of a robotic arm. When the arm touches Bennu’s floor, it can launch a burst of nitrogen gasoline to ruffle the floor simply sufficient to blow particles into the pattern collector. As a bonus, the pattern collector’s head is roofed in chrome steel Velcro-like pads that may decide up floor mud on contact.

The remote-reach technique avoids the trouble of anchoring to the asteroid, however presents its personal drawback: Nobody is aware of how fine-grained mud behaves when blown round in low gravity. That open query worries engineers. “What truly occurs once you contact the floor of an asteroid is an unknown space of physics,” Lauretta says. “I feel [the surface] goes to be like a fluid. It’s a very alien panorama.”

[embedded content]

IN AND OUT  TAGSAM’s arm permits floor contact with out the spacecraft touchdown on the asteroid. Throughout 5 seconds of contact, a jet of nitrogen gasoline will agitate Bennu’s floor to loosen mud for assortment. Floor contact pads may even accumulate fine-grained materials. As soon as assortment is finished, the TAGSAM head will transfer right into a capsule the place it’s protected against contamination in the course of the journey again to Earth.

The highway to Ryugu

When Hayabusa returned, planetary scientist Michelle Thompson of Purdue College in West Lafayette, Ind., studied the Itokawa grains. Having such a restricted provide compelled scientists to get probably the most out of the samples. The primary chapter of Thompson’s Ph.D. dissertation was written a few single Itokawa particle that measured 50 micrometers throughout.

“We nonetheless obtained some superb science out of these particles,” she says. These grains proved that a lot of the meteorites on Earth come from stony, carbon-poor asteroids like Itokawa, not carbon-bearing ones like Ryugu and Bennu (SN On-line: eight/25/11). “Within the context of [Hayabusa’s] issues, it’s unbelievable the quantity of knowledge that got here out of that mission,” Thompson says.

Whereas Hayabusa was floundering in house in 2006, Yoshikawa’s group was already suggesting that JAXA fly a follow-up mission. By then, Yoshikawa had set his sights on an much more engaging asteroid, Ryugu.

JAXA despatched a spacecraft to Itokawa as a result of it was simple to succeed in, not as a result of it was scientifically particular. However as a carbon-rich asteroid, Ryugu is believed to encompass probably the most historic, pristine materials within the photo voltaic system.

Ryugu’s title even references a time capsule from a Japanese folktale, during which the hero Urashima Taro retrieves a field from a dragon-guarded fort referred to as Ryugu on the backside of the ocean. When the hero returns to the floor, he finds that 300 years have handed. When he opens the field, he turns into an previous man, as a result of the field contained all of that elapsed time.

Yoshikawa and his colleagues proposed the mission yearly and had been rebuffed every time — till Hayabusa got here residence in 2010.

The spacecraft’s return was lauded in Japan, Yoshikawa says. “Japanese folks had been very shocked to see that Hayabusa actually got here to the Earth.” An editorial within the Japan Times deemed the spacecraft a “excessive achiever,” and referred to as for extra funding for JAXA and house analysis.

In Might 2011, the Japanese authorities authorised the Hayabusa2 mission. Tachibana, Yoshikawa and the remainder of the JAXA group aimed for the following launch window, in 2014.

Pleasant competitors

Like Hayabusa2, OSIRIS-REx was rejected a number of occasions earlier than NASA chosen it for flight, additionally in Might 2011. Due to Bennu’s orbit, the following launch alternative to succeed in the asteroid wasn’t till September 2016. That two-year hole between JAXA’s and NASA’s launches impressed some pleasant competitors between the groups.

Years within the making

The Hayabusa2 and OSIRIS-REx missions grew up virtually concurrently on reverse sides of the world. The shut timing of the Japanese and U.S. missions means the 2 can study from one another.

Aspect-by-side missions

Might 10, 1999: Ryugu found

September 11, 1999: Bennu found

Might 2011: Hayabusa2 and OSIRIS-REx are formally authorised

December three, 2014: Hayabusa2 launches

September eight, 2016: OSIRIS-REx launches

June 27, 2018: Hayabusa2 arrives at Ryugu

December three, 2018: OSIRIS-REx arrives at Bennu

Late 2020: Hayabusa2 returns samples to Earth

September 24, 2023: OSIRIS-REx returns samples to Earth

Hayabusa2: DLR (CC BY 3.0); OSIRIS-REx: Conceptual Picture Lab/NASA’s Goddard Area Flight Middle

“In fact, we’re good mates and we need to have a great relation,” Tachibana says. “However on the identical time we’re rivals.” OSIRIS-REx is larger than Hayabusa2 and plans to gather as much as 20,000 occasions as a lot asteroid mud — as much as two kilograms, within the best-case situation, in contrast with Hayabusa2’s complete of 100 milligrams. To compete, Hayabusa2’s group got down to do every thing first, Tachibana says.

“They had been involved we had been going to overshadow them,” Lauretta says. The primary few conferences between the groups had been tense, he remembers. However each teams felt it was finest to work collectively.

“That is the primary time since Apollo … that two sample-return missions are going to the identical form of goal,” Tachibana says. “The U.S. and the Soviet Union couldn’t discuss to one another.” It was the center of the Chilly Struggle. “This time we are able to discuss to one another.”

In November 2014, NASA and JAXA signed a memorandum promising to share knowledge, software program and samples. JAXA will give 10 % of its Ryugu pattern to NASA, and NASA will give zero.5 % of the bigger Bennu pattern to JAXA.

Nonetheless, the 2 house companies don’t align on every thing. “Hayabusa2 and OSIRIS-REx have fully totally different philosophies of sampling,” says cosmochemist Keiko Nakamura-Messenger of NASA’s Johnson Area Middle in Houston. She oversees the pattern website choice for OSIRIS-REx and shall be in command of storing the samples.

Take the mission timelines: OSIRIS-REx will spend greater than a 12 months mapping Bennu intimately. Its suite of science devices, together with three cameras, a laser altimeter and three spectrometers, will work out the asteroid’s composition all around the floor earlier than the group chooses the mission’s sole sampling website.

Hayabusa2 scientists, then again, chose the first of three sampling sites in August, lower than two months after the spacecraft arrived at Ryugu (SN On-line: eight/23/18). Initially the group deliberate to take its first pattern in October, however the boulders proved so tough that sampling was pushed to February 2019 on the earliest.

Hayabusa2 will pattern three websites to seize as a lot of the asteroid’s mineral range as potential. One of many samples will come from inside a several-meter-wide crater that doesn’t but exist. The spacecraft will create the outlet by firing a two-kilogram copper projectile on the asteroid, then conceal on the opposite facet of Ryugu to keep away from particles when the projectile hits. The goal is to see if the asteroid’s inside is totally different from the floor.

It’s laborious to think about NASA approving such a loopy maneuver, says Nakamura-Messenger, who grew up in Japan. It’s too dangerous. “The NASA approach, the American approach, is: The success price must be actually excessive,” she says. However she’s rooting for Hayabusa2’s daring strikes.

“In my coronary heart, I’m Japanese,” she says. “Subsequently, I’m like, ‘Go for it!’ ”

Valuable mud

Hayabusa2 goals to collect zero.1 grams of mud from Ryugu, the burden of about three grains of rice. OSIRIS-REx will attempt to rise up to 2,000 grams of Bennu’s floor, concerning the weight of a small Chihuahua.

C. Chang

Certain for Bennu

Nonetheless, Ryugu’s shock boulder discipline made Lauretta, Nakamura-Messenger and the remainder of the OSIRIS-REx group nervous about Bennu.

“I’ve been mendacity awake at evening anticipating Bennu,” Lauretta says. “It’s fascinating and scary abruptly.”

Becoming with NASA’s cautious strategy, the OSIRIS-REx group knew much more about Bennu than JAXA knew about Ryugu earlier than the missions launched. Bennu got here shut sufficient to Earth in 1999, 2005 and 2011 for radio telescopes to map the asteroid’s form (although not shut sufficient to disclose a lot element).

“We compiled probably the most complete database from astronomy for any asteroid within the photo voltaic system,” Lauretta says of the group’s prework on Bennu.

These radio measurements allowed researchers to see how daylight nudges the asteroid on its orbit, a phenomenon referred to as the Yarkovsky impact. As asteroids tumble by house, they take in daylight on one facet and re-emit that power as warmth later, when that facet faces away from the solar. The pressure of that radiating warmth is sufficient to push the asteroid round, making it tough to foretell the asteroid’s orbit over the long run.

The Yarkovsky impact calculation yielded a worrying prediction: Bennu has a 1 in 2,700 likelihood of hitting Earth within the late 22nd century, one of many highest possibilities of any recognized asteroid.

<img src="knowledge:picture/png;base64,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" data-echo="https://www.sciencenews.org/websites/default/information/2019/01/011919_LG_sample-return_inline8_730.jpg" alt class="caption" title="HAZARD MAP OSIRIS-REx took this mosaic picture of Bennu in early December and has seen indicators of liquid water within the asteroid’s previous. ~~ Univ. of Arizona, NASA’s Goddard Area Flight Middle”><img src="https://www.sciencenews.org/websites/default/information/2019/01/011919_LG_sample-return_inline8_730.jpg" alt class="caption" title="HAZARD MAP OSIRIS-REx took this mosaic picture of Bennu in early December and has seen indicators of liquid water within the asteroid’s previous. ~~ Univ. of Arizona, NASA’s Goddard Area Flight Middle”>

That forecast makes OSIRIS-REx’s mission much more pressing. Testing the returned samples will give scientists a greater understanding of how Bennu’s floor materials absorbs and emits warmth. That data will sharpen the researchers’ predictions of the place the asteroid will go, and assist inform future missions to deflect asteroids that come too near Earth.

That’s provided that Bennu is clean sufficient for the spacecraft to get a pattern. The first images taken as OSIRIS-REx approached Bennu on December three didn’t do a lot to quell the group’s fears. With the bare eye, Bennu appears to have about as many boulders as Ryugu, perhaps a little bit fewer, says planetary scientist Kevin Walsh of the Southwest Analysis Institute in Boulder, Colo.

“Even when we persuade ourselves that there’s a website that’s boulder free, there’s nonetheless an opportunity it might change afterward. So we’ll must see,” says Walsh, who introduced an early comparability of Bennu and Ryugu on December 11 at a Washington, D.C., assembly of the American Geophysical Union. “We now have loads of instruments to search out the locations with the least quantity of hazards, even when we are able to’t discover a place that’s fully freed from them.”

That may be a reduction, Nakamura-Messenger says. However each mission to this point has shocked her.

“I don’t make wild guesses anymore,” she says. “Nature is wilder.”


This text seems within the January 19, 2019 concern of Science Information with the headline, “Cosmic collectors: Twin quests goal to seize some asteroid mud and produce it to Earth.”

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