Humans Will Again Set Foot on the Moon; This Time, They'll Have UArizona Science in Tow
UArizona scientists mapped the moon for the Apollo missions. Now, as NASA astronauts prepare to return to the moon, two of the three instruments they'll bring have UArizona ties.Humans Will Again Set Foot on the Moon; This Time, They'll Have UArizona Science in Tow
×
NASA and University Communications - April 12, 2024
University of Arizona Lunar and Planetary Laboratory researchers will have a hand in two of the three instruments NASA selected for deployment on the lunar surface by Artemis III astronauts.
Once installed near the moon's South Pole, the instruments will collect valuable scientific data about the lunar environment, the lunar interior and how to sustain a long-duration human presence on the moon, which will help prepare NASA to send astronauts to Mars.
The instruments were specifically chosen because of their unique installation requirements that necessitate deployment by humans during moonwalks, a NASA press release explained. All three payloads were selected for further development towards flight on Artemis III, which is targeted to launch in 2026. Final manifesting decisions about the mission will be determined at a later date. Members of these payload teams will become members of NASA's Artemis III science team.
Artemis III, the first mission to return astronauts to the surface of the moon in more than 50 years, will explore the south polar region of the moon. Several proposed landing regions for the mission are located amid some of the oldest parts of the moon. Together with the permanently shadowed regions, they provide the opportunity to learn about the history of the moon through previously unstudied lunar materials.
Mapping moonquakes
Dani DellaGiustina, assistant professor of planetary sciences in the UArizona Lunar and Planetary Laboratory, is working as part of the team to design and build two seismometers for the Lunar Environment Monitoring Station, or LEMS. One will be tuned to detect deep moonquakes and the other to detect shallow moonquakes.
"I am stoked because I have been working for years to develop seismic instruments not just for the moon, but also for asteroids and other bodies like Europa," DellaGiustina said. "So, to see one of them make it to the next step, which is flight opportunity, is really exciting."
LEMS is led by Mehdi Benna from the University of Maryland, Baltimore County. NASA Goddard will build and operate LEMS. DellaGiustina is a co-investigator along with Hop Bailey, a UArizona Space Institute program manager, and Angela Marusiak, an assistant research professor of planetary sciences. Veronica Bray, associate research professor in planetary sciences, is assisting with science operations.
LEMS is a compact, autonomous seismometer suite designed to carry out continuous, long-term monitoring of ground motion from moonquakes, in the lunar south polar region. The instrument will characterize the regional structure of the moon's crust and mantle, which will add valuable information to lunar formation and evolution models. LEMS is intended to operate on the lunar surface from three months up to two years and may become a key station in a future global lunar geophysical network.
Moonquakes have a few sources, including the same gravitational tug between the moon and Earth that causes ocean tides. Also, in the same way that houses creak as temperatures rise, the moon trembles as it expands and contracts in response to dramatic temperature swings.
"The big difference between the Earth and the moon is the moon does not have plate tectonics. There is some evidence of faults on the moon, however," Marusiak said. "One of our goals is to figure out if those faults are active and how active they are, and if they could cause a risk for the astronauts or their habitats."
Lastly, the researchers also anticipate that LEMS will detect meteor impacts.
Treasures beneath the surface
Erik Asphaug, professor of planetary sciences in the UArizona Lunar and Planetary Laboratory, is a collaborator on the Lunar Dielectric Analyzer, or LDA, which will reveal what lies a meter deep in the moon's regolith, which is airless soil.
"As a child of the Apollo era, I find it amazing to be part of this adventure to put an instrument on the moon," Asphaug said. "I've always been a big fan of radio and radar techniques to find out what's inside of things. I'm most excited to see if the regolith near the south pole has active frost."
LDA will measure how the moon's regolith responds to an electric field, which depends on porosity and the presence of volatiles – substances that evaporate – especially ice. It will gather essential information about the structure of the moon's subsurface and monitor whether volatiles migrate as the LDA goes in and out of shadow.
Hideaki "Hirdy" Miyamoto – a University of Tokyo professor, Planetary Science Institute affiliated scientist and adjunct professor at the University of Adelaide – leads the LDA, which is supported by the Japan Aerospace Exploration Agency.
"Different materials propagate radio signals at different speeds," Asphaug said, "so when you send a signal and measure its reflection, its speed tells you about composition and porosity. This will be important not only for lunar science, but for establishing a permanent human presence on the moon."
With the Artemis campaign, NASA will land the first woman, first person of color and its first international partner astronaut on the moon, and establish long-term exploration for scientific discovery and preparation for human missions to Mars for the benefit of all.
"It is exciting to see a new generation of Lunar and Planetary Laboratory scientists build on our legacy of lunar exploration, dating back to even before Apollo," said Mark Marley, the Lunar and Planetary Laboratory director. "Our first major research program was to map the moon. Now we are helping send instruments to detect what lies beneath that surface."
UA News - Humans Will Again Set Foot on the Moon; This Time, They'll Have UArizona Science in Tow
How Pluto Got Its 'Heart'
The mystery of how Pluto got a giant heart-shaped feature on its surface has finally been solved by an international team of astrophysicists.How Pluto Got Its 'Heart'
×
University Communications - April 14, 2024
Ever since the cameras of NASA's New Horizons mission discovered a large heart-shaped structure on the surface of the dwarf planet Pluto in 2015, this "heart" has puzzled scientists because of its unique shape, geological composition and elevation. Scientists from the University of Bern in Switzerland and the University of Arizona used numerical simulations to investigate the origins of Sputnik Planitia, the western teardrop-shaped part of Pluto's heart surface feature.
According to their research, Pluto's early history was marked by a cataclysmic event that formed Sputnik Planitia: a collision with a planetary body a little over 400 miles in diameter, roughly the size of Arizona from north to south. The team’s findings, published in Nature Astronomy, also suggest that the inner structure of Pluto is different from what was previously assumed, indicating that there is no subsurface ocean.
"The formation of Sputnik Planitia provides a critical window into the earliest periods of Pluto's history," said Adeene Denton, a planetary scientist at the UArizona Lunar and Planetary Laboratory who co-authored the paper. "By expanding our investigation to include more unusual formation scenarios, we've learned some totally new possibilities for Pluto's evolution, which could apply to other Kuiper Belt objects as well."
A divided heart
The heart, also known as the Tombaugh Regio, captured the public's attention immediately upon its discovery. But it also immediately caught the interest of scientists because it is covered in a high-albedo material that reflects more light than its surroundings, creating its whiter color. However, the heart is not composed of a single element. Sputnik Planitia covers an area of approximately 750 by 1,250 miles, equivalent to a quarter of Europe or the United States. What is striking, however, is that this region is roughly 2.5 miles lower in elevation than most of Pluto's surface.
"While the vast majority of Pluto's surface consists of methane ice and its derivatives covering a water-ice crust, the Planitia is predominantly filled with nitrogen ice, which most likely accumulated quickly after the impact due to the lower altitude," said the lead author of the study, Harry Ballantyne, a research associate at Bern. The eastern part of the heart is also covered by a similar but much thinner layer of nitrogen ice, the origin of which is still unclear to scientists, but is probably related to Sputnik Planitia.
An oblique impact
The elongated shape of Sputnik Planitia and its location at the equator strongly suggest that the impact was not a direct head-on collision but rather an oblique one, according to Martin Jutzi of the University of Bern, who initiated the study. Like several others around the world, the team used Smoothed Particle Hydrodynamics simulation software to digitally re-create such impacts, varying both the composition of Pluto and its impactor, as well as the velocity and angle of the impactor. These simulations confirmed the scientists' suspicions about the oblique angle of impact and determined the composition of the impactor.
"Pluto's core is so cold that the rocks remained very hard and did not melt despite the heat of the impact, and thanks to the angle of impact and the low velocity, the core of the impactor did not sink into Pluto's core, but remained intact as a splat on it," Ballantyne said. This core strength and relatively low velocity were key to the success of these simulations: Lower strength would result in a very symmetrical leftover surface feature that does not look like the teardrop shape observed by NASA's New Horizons probe during its fly-by of Pluto in 2015.
"We are used to thinking of planetary collisions as incredibly intense events where you can ignore the details except for things like energy, momentum and density," said Lunar and Planetary Laboratory professor and study co-author Erik Asphaug, whose team has collaborated with its Swiss colleagues since 2011, exploring the idea of planetary "splats" to explain, for instance, features on the far side of Earth's moon. "In the distant solar system, velocities are so much slower than closer to the sun, and solid ice is strong, so you have to be much more precise in your calculations. That's where the fun starts."
No subsurface ocean on Pluto
The current study sheds new light on Pluto's internal structure as well. In fact, a giant impact like the one simulated is much more likely to have occurred very early in Pluto's history than during more recent times. However, this poses a problem: A giant depression like Sputnik Planitia is expected to slowly drift toward the pole of the dwarf planet over time due to the laws of physics, since it is less massive than its surroundings. Yet it has remained near the equator. The previous theorized explanation invoked a subsurface liquid water ocean, similar to several other planetary bodies in the outer solar system. According to this hypothesis, Pluto's icy crust would be thinner in the Sputnik Planitia region, causing the ocean to bulge upward, and since liquid water is denser than ice, causing a mass surplus that induces migration toward the equator.
The new study offers an alternative perspective, according to the authors, pointing to simulations in which all of Pluto's primordial mantle is excavated by the impact, and as the impactor's core material splats onto Pluto's core, it creates a local mass excess that can explain the migration toward the equator without a subsurface ocean, or at most a very thin one.
Denton, who already has embarked on a research project to estimate the speed of this migration, said this novel and creative origin hypothesis for Pluto's heart-shaped feature may lead to a better understanding of the dwarf planet's origin.
UA News - How Pluto Got Its 'Heart'
How the Moon Turned Itself Inside Out
More than 50 years ago, Apollo astronauts brought basaltic lava rocks back from the moon with surprisingly high concentrations of titanium. Later, satellite observations found that these titanium-rich volcanic rocks are primarily located on the moon's nearside - but how and why they got there has remained a mystery – until now.How the Moon Turned Itself Inside Out
×
By Daniel Stolte, University Communications - April 8, 2024
About 4.5 billion years ago, a small planet smashed into the young Earth, flinging molten rock into space. Slowly, the debris coalesced, cooled and solidified, forming our moon. This scenario of how the Earth's moon came to be is the one largely agreed upon by most scientists. But the details of how exactly that happened are "more of a choose-your-own adventure novel," according to researchers in the University of Arizona Lunar and Planetary Laboratory who published a paper in Nature Geoscience. The findings offer important insights into the evolution of the lunar interior, and potentially for planets such as the Earth or Mars.
Most of what is known about the origin of the moon comes from analyses of rock samples, collected by Apollo astronauts more than 50 years ago, combined with theoretical models. The samples of basaltic lava rocks brought back from the moon showed surprisingly high concentrations of titanium. Later satellite observations found that these titanium-rich volcanic rocks are primarily located on the moon's nearside, but how and why they got there has remained a mystery – until now.
Because the moon formed fast and hot, it was likely covered by a global magma ocean. As the molten rock gradually cooled and solidified, it formed the moon's mantle and the bright crust we see when we look up at a full moon at night. But deeper below the surface, the young moon was wildly out of equilibrium. Models suggest that the last dregs of the magma ocean crystallized into dense minerals including ilmenite, a mineral containing titanium and iron.

Schematic illustration with a gravity gradient map of the lunar nearside and a cross-section showing two ilmenite-bearing cumulate downwellings from lunar mantle overturn.
Adrien Broquet/University of Arizona & Audrey Lasbordes
"Because these heavy minerals are denser than the mantle underneath, it creates a gravitational instability, and you would expect this layer to sink deeper into the moon's interior," said Weigang Liang, who led the research as part of his doctoral work at LPL.
Somehow, in the millennia that followed, that dense material did sink into the interior, mixed with the mantle, melted and returned to the surface as titanium-rich lava flows that we see on the surface today.
"Our moon literally turned itself inside out," said co-author and LPL associate professor Jeff Andrews-Hanna. "But there has been little physical evidence to shed light on the exact sequence of events during this critical phase of lunar history, and there is a lot of disagreement in the details of what went down – literally."
Did this material sink as it formed a little at a time, or all at once after the moon had fully solidified? Did it sink into the interior globally and then rise up on the near side, or did it migrate to the near side and then sink? Did it sink in one big blob, or several smaller blobs?
"Without evidence, you can pick your favorite model. Each model holds profound implications for the geologic evolution of our moon," said co-lead author Adrien Broquet of the German Aerospace Center in Berlin, who did the work during his time as a postdoctoral research associate at LPL.
In a previous study, led by Nan Zhang at Peking University in Beijing, who is also a co-author on the latest paper, models predicted that the dense layer of titanium-rich material beneath the crust first migrated to the near side of the moon, possibly triggered by a giant impact on the far side, and then sunk into the interior in a network of sheetlike slabs, cascading into the lunar interior almost like waterfalls. But when that material sank, it left behind a small remnant in a geometric pattern of intersecting linear bodies of dense titanium-rich material beneath the crust.
"When we saw those model predictions, it was like a lightbulb went on," said Andrews-Hanna, "because we see the exact same pattern when we look at subtle variations in the moon’s gravity field, revealing a network of dense material lurking below the crust."
In the new study, the authors compared simulations of a sinking ilmenite-rich layer to a set of linear gravity anomalies detected by NASA's GRAIL mission, whose two spacecraft orbited the moon between 2011 and 2012, measuring tiny variations in its gravitational pull. These linear anomalies surround a vast dark region of the lunar near side covered by volcanic flows known as mare (Latin for "sea").

The lunar near side with its dark regions, or “mare,” covered by titanium-rich volcanic flows (center) makes up the moon’s familiar sight from Earth (left). The mare region is surrounded by a polygonal pattern of linear gravity anomalies (blue in image on the right) interpreted to be the vestiges of dense material that sank into the interior. Their presence provides the first physical evidence for the nature of the global mantle overturn more than 4 billion years ago.
Adrien Broquet/University of Arizona
The authors found that the gravity signatures measured by the GRAIL mission are consistent with ilmenite layer simulations, and that the gravity field can be used to map out the distribution of the ilmenite remnants left after the sinking of the majority of the dense layer.
"Our analyses show that the models and data are telling one remarkably consistent story," Liang said. "Ilmenite materials migrated to the near side and sunk into the interior in sheetlike cascades, leaving behind a vestige that causes anomalies in the moon's gravity field, as seen by GRAIL."
The team's observations also constrain the timing of this event: The linear gravity anomalies are interrupted by the largest and oldest impact basins on the near side and therefore must have formed earlier. Based on these cross-cutting relationships, the authors suggest that the ilmenite-rich layer sank prior to 4.22 billion years ago, which is consistent with it contributing to later volcanism seen on the lunar surface.
"Analyzing these variations in the moon's gravity field allowed us to peek under the moon's surface and see what lies beneath," said Broquet, who worked with Liang to show that the anomalies in the moon’s gravitational field match what would be expected for the zones of dense titanium-rich material predicted by computer simulation models of lunar overturn.
Lopsided moon
While the detection of lunar gravity anomalies provides evidence for the sinking of a dense layer in the moon’s interior and allows for a more precise estimate of how and when this event occurred, what we see on the surface of the moon adds even more intrigue to the story, according to the research team.
"The moon is fundamentally lopsided in every respect," Andrews-Hanna said, explaining that the near side facing the Earth, and particularly the dark region known as Oceanus Procellarum region, is lower in elevation, has a thinner crust, is largely covered in lava flows, and has high concentrations of typically rare elements like titanium and thorium. The far side differs in each of these respects. Somehow, the overturn of the lunar mantle is thought to be related to the unique structure and history of the near side Procellarum region. But the details of that overturn have been a matter of considerable debate among scientists.
"Our work connects the dots between the geophysical evidence for the interior structure of the moon and computer models of its evolution," Liang added.
"For the first time we have physical evidence showing us what was happening in the moon’s interior during this critical stage in its evolution, and that's really exciting," Andrews-Hanna said. "It turns out that the moon’s earliest history is written below the surface, and it just took the right combination of models and data to unveil that story."
"The vestiges of early lunar evolution are present below the crust today, which is mesmerizing," Broquet said. "Future missions, such as with a seismic network, would allow a better investigation of the geometry of these structures."
Liang added: "When the Artemis astronauts eventually land on the moon to begin a new era of human exploration, we will have a very different understanding of our neighbor than we did when the Apollo astronauts first set foot on it."
UA News - How the Moon Turned Itself Inside Out
Teams Behind OSIRIS-REx Win Prestigious Aviation Award
The team behind the University of Arizona-led NASA mission to sample the asteroid Bennu joins the ranks of the Apollo 11 crew and Orville Wright to earn the Robert J. Collier Trophy.Teams Behind OSIRIS-REx Win Prestigious Aviation Award
×
By Mikayla Mace Kelley, University Communications - March 26, 2024
The University of Arizona, NASA and Lockheed Martin have won the Robert J. Collier Trophy for their work on the OSIRIS-REx mission that returned a sample of the asteroid Bennu last fall.
The National Aeronautic Association, which gives the award every year, made the announcement Tuesday. The Collier Trophy, awarded since 1911, is one of the most prestigious honors in aviation, recognizing the "performance, efficiency and safety of air or space vehicles."
In earning the trophy, the OSIRIS-REx team joins ranks that include the team behind the James Webb Space Telescope and the crew of NASA's Apollo 11 mission, as well as legendary aviators such as Orville Wright and Chuck Yeager. The list of Collier recipients represents a timeline of the most groundbreaking aviation achievements that created today's aerospace industry.
"It's an awesome crowd to be affiliated with," said Dante Lauretta, OSIRIS-REx principal investigator and a Regents Professor of planetary sciences at the UArizona Lunar and Planetary Laboratory. "It hammers home the magnitude of the accomplishment. I always understood we were doing something important, but it shows the recognition the country and world is bestowing upon us."
The OSIRIS-REx spacecraft delivered 4.29 ounces, or 121.6 grams, of rocks and dust from the near-Earth asteroid Bennu on Sept. 24. The delivery, shot back to Earth in a capsule to scientists waiting in the Utah desert, was a first in U.S. history, and the largest sample returned since the Apollo missions.
The sample delivery went according to plan thanks to the massive effort of hundreds of people who remotely directed the spacecraft's seven-year journey to Bennu and back, starting with launch on Sept. 8, 2016. The team guided it to arrival at Bennu on Dec. 3, 2018, followed by the search for a safe sample-collection site in 2019 and 2020, sample collection on Oct. 20, 2020, and the return trip home starting on May 10, 2021. During the asteroid encounter, the team set new Guinness World Records for smallest object orbited and closest orbit achieved by a spacecraft.
Initial studies of the Bennu sample in October showed evidence of water-bearing minerals and high carbon content, indicating the building blocks of life might be found in the rock. A sample of the asteroid is available for the public to see at the UArizona's Alfie Norville Gem & Mineral Museum.
"I have been avidly following the progress of OSIRIS-REx ever since I came to the University of Arizona, and it was such an incredible moment to witness the delivery of the asteroid sample," said University of Arizona President Robert C. Robbins. "I am proud to see the outstanding achievements of the OSIRIS-REx team recognized with the Robert J. Collier Trophy.
The work this team has done to advance the knowledge of our solar system and its origin is awe-inspiring, and the Collier Trophy is richly deserved." "The award really focuses on accomplishments within the last year," Lauretta said. "The entry, descent, and landing of the sample return capsule in the fall allowed the Air Force to test and calibrate sensors for other incoming hazards."
The mission also provided unprecedented insight into potentially hazardous near-Earth asteroids like Bennu through the science team's characterization of the Yarkovsky effect, a small amount of thrust generated by heat from the sun being radiated off an asteroid's surface. The team also developed a natural feature tracking system, which is onboard software for targeting the sample site and hazard avoidance during sample collection. As a result, OSIRIS-REx became the first mission to fly image-based guidance in deep space.
UArizona-led science and operations teams supported the spacecraft navigators at NASA Goddard Space Flight Center, KinetX and Lockheed Martin in achieving these successes.
Ultimately, the mission wrapped on time and exceeded the mission sample requirement laid out by NASA, Lauretta said.
UA News - Teams Behind OSIRIS-REx Win Prestigious Aviation Award
Loathed By Scientists, Loved By Nature: Sulfur and The Origin Of Life
A University of Arizona-led study shines a spotlight on sulfur, a chemical element that, while all familiar, has proved surprisingly resistant to scientific efforts in probing its role in the origin of life.Loathed By Scientists, Loved By Nature: Sulfur and The Origin Of Life
×
By Daniel Stolte, University Communications - March 13, 2024
Many artists have tried to depict what Earth might have looked like billions of years ago, before life made its appearance. Many scenes trade snow-covered mountains for lava-gushing volcanoes and blue skies for lightning bolts pummeling what's below from a hazy sky.
But what did early Earth actually look like? This question has been the subject of intense scientific research for decades.
A publication led by Sukrit Ranjan, an assistant professor in the University of Arizona's Lunar and Planetary Laboratory, shines a spotlight on sulfur, a chemical element that, while all familiar, has proved surprisingly resistant to scientific efforts in probing its role in the origin of life.
"Our picture of early Earth is pretty fuzzy," said Ranjan, who explores sulfur concentrations in early Earth's waters and atmosphere. The same processes that make our planet habitable – liquid water and plate tectonics – constantly destroy the rocks that hold Earth's geologic record, he argues. "It's great for us because it recycles nutrients that would otherwise be locked up in Earth's crust, but it's terrible for geologists in the sense that it removes the messengers."
Published in the journal AGU Advances in December, Ranjan's paper was selected as an editor's highlight, in recognition of "experiments that were extremely difficult to perform but provide constraints for ongoing laboratory prebiotic chemistry experiments."
At the core of efforts to pull back the curtain on the emergence of life on Earth has been a concept known as the "RNA world," Ranjan said, referring to ribonucleic acid, a class of molecules that are present in every living cell and crucial to life as we know it.
The RNA world hypothesis is based on an interesting feature of modern biology, which is that of the four major categories of biomolecules – amino acids, carbohydrates, lipids and nucleic acids – RNA is the only one that can perform the role of an enzyme and the storage and replication of genetic information, by making copies of itself, all by itself. There’s just one problem: It's really hard to make.
"For about 50 years, people have tried to figure out how to make RNA without enzymes, which is how biology does it," Ranjan said, explaining that it wasn't until the last five years that researchers figured out non-enzymatic pathways to make RNA.
"If we can get RNA, then on the far horizon we see a pathway to get everything else going," he said. "And this begs the question: Was this molecule actually available earlier in any quantities whatsoever? And this is actually a major open question."
Recently, scientists have completed a half-century quest to make RNA molecules without biological enzymes, a huge step forward to demonstrating the RNA world. However, these chemical pathways all rely on a critical sulfur molecule, called sulfite. By studying rock samples from some of Earth's oldest rocks, scientists know there was plenty of sulfur to go around on the early, prebiotic Earth. But how much of it was in the atmosphere? How much of it ended up in water? And how much of it ended up as RNA-producing sulfite? Those are the questions Ranjan and his team set out to answer.
"Once it's in the water, what happens to it? Does it stick around for a long time, or does it go away quickly?" he said. "For modern Earth we know the answer – sulfite loves to oxidize, or react with oxygen, so it'll go away super-fast."
By contrast, as geological evidence indicates, there was very little oxygen in early Earth's atmosphere, which could have allowed sulfite to accumulate and last much longer. However, even in the absence of oxygen, sulfite is very reactive, and many reactions could have scrubbed it from the early Earth environment.
One such reaction is known as disproportionation, a process by which several sulfites react with each other, turning them into sulfate, and elemental sulfur, which are not useful for origin-of-life chemistry. But how fast is this process? Would it have allowed for sufficient quantities of sulfites to build up to kickstart life?
"No one has actually looked into this in depth outside of other contexts, mainly wastewater management," Ranjan said.
His team then set out to investigate this problem under various conditions, an effort that took five years from designing the experiments to publishing the results.
"Of all the atoms that stock the prebiotic shipyard, including carbon, hydrogen, nitrogen, oxygen, phosphorus and sulfur, sulfur is perhaps the thorniest," wrote Sonny Harman of NASA's Ames Research Center, in a viewpoint article accompanying the publication. Because of its eagerness to enter into chemical reactions, "sulfur compounds tend to be more unstable, posing hazards to lab personnel and equipment, clogging up instrumentation and gumming up experiments."
A lab tech's nightmare
In their setup, Ranjan and his co-authors dissolved sulfite in water at various levels of acidity or alkalinity, locked it into a container under an oxygen-free atmosphere and let it "age," as Ranjan put it. Every week, the team measured the concentrations of various sulfites with ultraviolet light. At the end of the experiment, they subjected them to a suite of analyses, all geared toward answering a relatively simple question, he said: "Just how much of this original molecule is left, and what did it turn into?"
Sulfites, it turned out, disproportionate much slower than what conventional wisdom held. Earlier studies, for example, had floated the idea of a sulfur haze engulfing the early Earth, but Ranjan's team found that sulfites break down under ultraviolet light more quickly than expected. In the absence of an ozone layer during Earth's early days, this process, known as photolysis, would have quickly purged sulfur compounds from the atmosphere and the water, albeit not quite as efficiently as the abundant oxygen in today's world.
While it's plausible that slow disproportionation could have allowed sulfites to accumulate, photolysis would have made that very unlikely except in certain environments such as shallow water pools, shaded from UV radiation, particularly if fed by surface runoff to provide mineral shields. Examples include underground pools or closed basin carbonate lakes, drainage-less depressions where sediments accumulate but water can only leave by evaporation.
"Think bodies of water like the Great Salt Lake in Utah or Mono Lake in California," Ranjan said, adding that hydrothermal environments are emerging as hot candidates for life's first appearance. Here, groundwater carrying dissolved minerals comes into contact with heat from volcanic activity, creating unique micro-environments that offer "safe spaces" for chemical process that could not occur elsewhere.
Such places can be found at mid-ocean ridges in the deep sea, but also on land, Ranjan said.
"A modern-day example of this is Yellowstone National Park, where we find pools that accumulate lots of sulfite, despite the oxygen," he said, "and that can happen just because the sulfite is continually being replenished by volcanic outgassing."
The study provides opportunities to test the hypothesis of sulfite availability in the evolution of the first molecules of life experimentally, the authors point out. Ranjan said one field of research in particular has him excited – phylogenetic microbiology, which uses genome analysis to reconstruct the blueprints of sulfur-using microorganisms believed to represent the oldest phyla on Earth.
There is evidence that these bacteria gain energy by reducing highly oxidized forms of sulfur to less oxidized ones. Intriguingly, Ranjan pointed out, they depend on a fairly complex enzyme machinery for the first step, reducing sulfate, sulfur's abundant "modern" form, to sulfite, suggesting these enzymes are the product of a long evolutionary process. In contrast, only one enzyme is involved in the conversion from sulfite – the proposed key ingredient in "prebiotic puddle environments" – to sulfide.
"If true, this implies that sulfite was present in the natural environment in at least some water bodies, similar to what we argue here," he said. "Geologists are just now turning to this. Can we use ancient rocks to test if they're rich in sulfite? We don't know the answer yet. This is still cutting-edge science."
UA News - Loathed By Scientists, Loved By Nature: Sulfur and The Origin Of Life
A Pebble Scooped from an Asteroid is now on Display at UArizona Museum
Tucson’s Alfie Norville Gem & Mineral Museum is one of only three places in the world where the public can see a piece of the asteroid Bennu, collected during NASA's LPL-led OSIRIS-REx mission.A Pebble Scooped from an Asteroid is now on Display at UArizona Museum
×
It might not be the heftiest or flashiest stone on display at the University of Arizona's Alfie Norville Gem & Mineral Museum, but it certainly is its most unique, if not downright alien: a piece from an asteroid in space, brought to Earth by NASA's UArizona-led OSIRIS-REx mission in September.
After seven years in space and over 4 billion miles traveled, it touched down in a remote area of the Utah desert, tucked safely inside a capsule protecting the sample from the harsh conditions in space and the rough ride through Earth's atmosphere.
The museum is one of only three places in the world to display an extraterrestrial rock sample collected in space, other than the moon. The other two samples from asteroid Bennu available for public viewing are at Space Center Houston in Texas and the Smithsonian National Museum of Natural History in Washington, D.C. Sample curation specialists at NASA's Johnson Space Center in Houston carefully selected the specimen suitable for public display, and visitors can check it out as of today.
Canister open.jpeg
The spacecraft's sample canister with the lid open, inside a glovebox at NASA's Johnson Space Center in Houston. In all, OSIRIS-REx brought 121.6 grams (4.29 ounces) of material to Earth on Sept. 24. NASA/Johnson Space Center"What's so special about the Bennu sample is that it was collected directly at the asteroid, in space, and that's something that we really try to help our visitors understand," said the museum's director, Violetta Wolf, explaining that while many are familiar with seeing meteorites on display, it is important to realize that those are very different.
While meteorites come from space, too, by the time they reach the ground, they have been in contact with all sorts of Earthly influences – during their fall, they are exposed to extreme heat, altering their appearance as well as possibly their structure and chemical makeup. Then they smack into the ground, sometimes digging into the soil. By the time they are found and collected, they have been exposed to the air, water, microbes and who knows what.
"To have something that actually has never been in contact with our atmosphere or anything else on our planet, is exceptional and incredibly rare," Wolf said. "We only have two pieces in the museum like that, and that's the lunar sample and now the sample from Bennu."
In all, OSIRIS-REx brought 121.6 grams (4.29 ounces) of material to Earth on Sept. 24. Of that amount, UArizona scientists received 200 milligrams (approximately 7 thousandths of an ounce) of asteroid material for scientific study. Initial analyses indicate the samples contain plentiful amounts of water locked up in minerals like clays and are also rich in carbon, nitrogen, sulfur and phosphorus.
Bigger than the sand-size science samples that are currently being analyzed at the university, the specimen that NASA allocated for public display in Tucson is a small, dark pebble with well-defined structure and texture. It will go on display next to a moon rock brought to Earth by astronauts of the Apollo 15 mission.
"It's not huge, of course, but for a sample of this significance, it's actually pretty large," Wolf said, adding that the roughly pinky-nail-size display specimen is actually larger than expected.
"You can actually see it's a small pebble, very dark, almost black," she said. "It almost seems like something that you would shake out your shoe after a long hike. If you look closely, you can see some different textures in it, some different colors."
Educational samples are specifically portioned out to recognize the importance of not just the scientific research, but the potential to inspire and encourage future scientists, Wolf said.
The specimen is tucked inside a clear container held by a metal casing to protect it from mechanical damage. A protective nitrogen atmosphere protects it from being exposure to air and prevents chemical alteration.
"NASA's approach to scientific research is that it has to also benefit the public through interpretation and getting young people excited about careers in science and space-related research and technology," Wolf said. "Putting it in its display case really was a humbling moment – recognizing what just passed through our hands."
And while that small piece of asteroid Bennu will sit in its case, shielded from Earth's ever-changing environment, its story has only just begun. As OSIRIS-REx scientists are beginning to probe the stuff left over from the formation of the solar system about 4.6 billion years ago, they will make countless discoveries, and with each one, a little bit more will be known about the display sample.
"This is not a 'one and done' kind of exhibit," Wolf said. "We're going to keep adding more information as we learn. Having this on display is a huge milestone, but there's still so much to come."
As new analytic technologies become available and new papers are being published, researchers such as Dante Lauretta, the mission's principal investigator at the UArizona Lunar and Planetary Laboratory, will share those insights with the public, and Wolf and her team already look forward to updating the information on the display to share them with the public.
"Having this asteroid sample on display is a testament to the incredible achievements of the OSIRIS-REx mission and the dedication of the team behind it," Lauretta said. "It's a tangible reminder of humanity's ability to explore the cosmos and unravel the mysteries of our universe."
James Webb Space Telescope Captures the End of Planet Formation
We know that there is nearly 100 times more gas than solids present when planets form. But today we see only a fraction of that gas in the solar system (stored within gas giant planets like Jupiter). So, when and how did the remaining gas leave the system? New research featuring LPL graduate student Naman Bajaj as lead author seeks to answer this exact question.James Webb Space Telescope Captures the End of Planet Formation
×
Scientists believe that planetary systems like our solar system contain more rocky objects than gas-rich ones. Around our sun, these include the inner planets – Mercury, Venus, Earth and Mars – the asteroid belt and the Kuiper belt objects such as Pluto.
Jupiter, Saturn, Uranus and Neptune, on the other hand, contain mostly gas. But scientists also have known for a long time that planet-forming disks start out with 100 times more mass in gas than solids, which leads to a pressing question: When and how does most of the gas leave a nascent planetary system?
A new study led by Naman Bajaj at the University of Arizona Lunar and Planetary Laboratory, published in the Astronomical Journal, provides answers. Using the James Webb Space Telescope, or JWST, the team obtained images from such a nascent planetary system – also known as a circumstellar disk – in the process of actively dispersing its gas into surrounding space.
"Knowing when the gas disperses is important as it gives us a better idea of how much time gaseous planets have to consume the gas from their surroundings," said Bajaj, a second-year doctoral student at UArizona's Lunar and Planetary Laboratory. "With unprecedented glimpses into these disks surrounding young stars, the birthplaces of planets, JWST helps us uncover how planets form."
During the very early stages of planetary system formation, planets coalesce in a spinning disk of gas and tiny dust around the young star, according to Bajaj. These particles clump together, building up into bigger and bigger chunks called planetesimals. Over time, these planetesimals collide and stick together, eventually forming planets. The type, size and location of planets that form depend on the amount of material available and how long it remains in the disk.
"So, in short, the outcome of planet formation depends on the evolution and dispersal of the disk," Bajaj said.
At the heart of this discovery is the observation of T Cha, a young star – relative to the sun, which is about 4.6 billion years old – enveloped by an eroding circumstellar disk notable for a vast dust gap, spanning approximately 30 astronomical units, or au, with one au being the average distance between the Earth and the sun.
Bajaj and his team were able, for the first time, to image the disk wind, as the gas is referred to when it slowly leaves the planet-forming disk. The astronomers took advantage of the telescope's sensitivity to light emitted by an atom when high-energy radiation – for example, in starlight – strips one or more electrons from its nucleus. This is known as ionization, and the light emitted in the process can be used as a sort of chemical "fingerprint" – in the case of the T Cha system, tracing two noble gases, neon and argon. The observations also mark the first time a double ionization of argon has been detected in a planet-forming disk, the team writes in the paper.
"The neon signature in our images tells us that the disk wind is coming from an extended region away from the disk," Bajaj said. "These winds could be driven either by high-energy photons – essentially the light streaming from the star – or by the magnetic field that weaves through the planet-forming disk."
In an effort to differentiate between the two, the same group, this time led by Andrew Sellek, a postdoctoral researcher at Leiden University in the Netherlands, performed simulations of the dispersal driven by stellar photons, the intense light streaming from the young star. They compared these simulations to the actual observations and found dispersal by high-energy stellar photons can explain the observations, and hence cannot be excluded as a possibility. That study concluded that the amount of gas dispersing from the T Cha disk every year is equivalent to that of Earth's moon. These results will be published in a companion paper, currently under review with the Astronomical Journal.
While neon signatures had been detected in many other astronomical objects, they weren't known to originate in low-mass planet-forming disks until first discovered in 2007 with JWST's predecessor, NASA's Spitzer Space Telescope, by Ilaria Pascucci, a professor at LPL who soon identified them as a tracer of disk winds. Those early findings transformed research efforts focused on understanding gas dispersal from circumstellar disks. Pascucci is the principal investigator on the most recent observing project and a co-author on the publications reported here.
"Our discovery of spatially resolved neon emission – and the first detection of double ionized argon – using the James Webb Space Telescope could become the next step towards transforming our understanding of how gas clears out of a planet-forming disk," Pascucci said. "These insights will help us get a better idea of the history and impact on our own solar system."
In addition, the group has also discovered that the inner disk of T Cha is evolving on very short timescales of decades; they found that the spectrum observed by JWST differs from the earlier spectrum detected by Spitzer. According to Chengyan Xie, a second-year doctoral student at LPL who leads this in-progress work, this mismatch could be explained by a small, asymmetric disk inside of T Cha that has lost some of its mass in the short 17 years that have elapsed between the two observations.
"Along with the other studies, this also hints that the disk of T Cha is at the end of its evolution," Xie said. "We might be able to witness the dispersal of all the dust mass in T Cha's inner disk within our lifetime."
Co-authors on the publications include Uma Gorti with the SETI Institute, Richard Alexander with the University of Leicester, Jane Morrison and Andras Gaspar with the UArizona's Steward Observatory, Cathie Clarke with the University of Cambridge, Giulia Ballabio with Imperial College London, and Dingshan Deng with the Lunar and Planetary Laboratory.
NASA's OSIRIS-REx Curation Team Clears Hurdle to Access Remaining Bennu Sample
Before this milestone, the curation team already had collected more than the 60 grams required to declare the mission a success.NASA's OSIRIS-REx Curation Team Clears Hurdle to Access Remaining Bennu Sample
×
NASA Johnson Space Center and University Communications - January 11, 2024
NASA's Johnson Space Center curation team members have successfully removed the two fasteners from the sampler head that had prevented the remainder of OSIRIS-REx's asteroid Bennu sample material from being accessed.
Steps now are underway to complete the disassembly of the Touch-and-Go Sample Acquisition Mechanism, or TAGSAM, head to reveal the rest of the rocks and dust delivered by NASA's first asteroid sample return mission. The mission, which launched in 2016 and spent the next seven years traveling to Bennu and imaging the asteroid before collecting the sample, returned the sample to Earth on Sept. 24.
The sample is thought to contain the leftovers from the formation of the solar system 4.5 billion years ago.
"Finally having the TAGSAM head open and full access to the returned Bennu samples is a monumental achievement that reflects the unwavering dedication and ingenuity of our team," said the mission's principal investigator, Dante Lauretta, Regents Professor at the University of Arizona Lunar and Planetary Laboratory. "This success reaffirms the significance of OSIRIS-REx and our commitment to advancing our understanding of the cosmos. We eagerly anticipate the next chapter as we share these precious samples with the global scientific community and continue our journey of discovery."
The remainder of the bulk sample will be fully visible after a few additional disassembly steps, at which point image specialists will take ultra-high-resolution pictures of the sample while it is still inside the TAGSAM head. This portion of the sample will then be removed and weighed, and the team will be able to determine the total mass of Bennu material captured by the mission.
"Our engineers and scientists have worked tirelessly behind the scenes for months to not only process the more than 70 grams of material we were able to access previously, but also design, develop and test new tools that allowed us to move past this hurdle," said Eileen Stansbery, division chief for Astromaterials Research and Exploration Science at Johnson. "The innovation and dedication of this team has been remarkable. We are all excited to see the remaining treasure OSIRIS-REx holds."
Curation processors paused disassembly of the TAGSAM head hardware in mid-October after they discovered that two of the 35 fasteners could not be removed with the tools approved for use inside the OSIRIS-REx glovebox. In response, two new multi-part tools were designed and fabricated to support further disassembly of the TAGSAM head. These tools include newly custom-fabricated bits made from a specific grade of surgical, non-magnetic stainless steel – the hardest metal approved for use in the pristine curation gloveboxes.
"In addition to the design challenge of being limited to curation-approved materials to protect the scientific value of the asteroid sample, these new tools also needed to function within the tightly confined space of the glovebox, limiting their height, weight and potential arc movement," said Nicole Lunning, OSIRIS-REx curator at Johnson. "The curation team showed impressive resilience and did incredible work to get these stubborn fasteners off the TAGSAM head so we can continue disassembly. We are overjoyed with the success."
Prior to the successful removal, the team at Johnson tested the new tools and removal procedures in a rehearsal lab. After each successful test, engineers increased the assembly torque values – or twisting force – and repeated the testing procedures until the team was confident the new tools would be able to remove the fasteners while minimizing the risk of any potential damage to the TAGSAM head or any contamination of the sample within.
Despite not being able to fully disassemble the TAGSAM head, the curation team members had already collected 2.48 ounces, or 70.3 grams, of asteroid material from the sample hardware, surpassing the agency's goal of bringing at least 60 grams to Earth. They have fulfilled all the sample requests received from the OSIRIS-REx science team so far and have hermetically sealed some of the Bennu sample for better preservation over decades, storing some at ambient temperature conditions and others at minus-112 degrees Fahrenheit.
Meanwhile, scientists at UArizona's Kuiper-Arizona Laboratory for Astromaterials Analysis have begun analyzing some of the pristine extraterrestrial material that the mission delivered from Bennu.
Later this spring, the curation team will release a catalog of the OSIRIS-REx samples, which will be available to the global scientific community.
UA News - NASA's OSIRIS-REx Curation Team Clears Hurdle to Access Remaining Bennu Sample
UArizona-led Asteroid Sampling Mission's New Journey: OSIRIS-APEX
Under the leadership of the University of Arizona's Dani Mendoza DellaGiustina, the former OSIRIS-REx spacecraft sets off on a journey to study asteroid Apophis and take advantage of the asteroid's 2029 flyby of Earth.UArizona-led Asteroid Sampling Mission's New Journey: OSIRIS-APEX
×
By University Communications and NASA Goddard Space Flight Center - January 8, 2024
At the end of a long-haul road trip, it might be time to kick up your feet and rest awhile – especially if it was a seven-year, 4-billion-mile journey to bring Earth a sample of asteroid Bennu.
But OSIRIS-REx, the NASA mission that accomplished this feat in September, is already well on its way – with a new name – to explore a new destination, this time under the leadership of Dani Mendoza DellaGiustina, an assistant professor at the University of Arizona's Lunar and Planetary Laboratory who previously served as the deputy principal investigator of OSIRIS-REx.
When OSIRIS-REx left Bennu in May 2021 with a sample aboard, its instruments were in great condition, and it still had a quarter of its fuel left. So instead of shutting down the spacecraft after it delivered the sample, the team proposed to dispatch it on a bonus mission to asteroid Apophis, with an expected arrival in April 2029. NASA agreed, and OSIRIS-APEX (Origins, Spectral Interpretation, Resource Identification, and Security – Apophis Explorer) was born.
A rare opportunity at Apophis
After considering several destinations, including Venus and various comets, NASA chose to send the spacecraft to Apophis, an "S-type" asteroid made of silicate materials and nickel-iron – a fair bit different from the carbon-rich, "C-type" Bennu.
The intrigue of Apophis is its exceptionally close approach of our planet on April 13, 2029. Although Apophis will not hit Earth during this encounter or in the foreseeable future, the pass in 2029 will bring the asteroid within 20,000 miles (32,000 kilometers) of the surface – closer than some satellites, and close enough that it could be visible to the naked eye in the Eastern Hemisphere.
Apophis' close encounter with Earth will change the asteroid’s orbit and the length of its 30.6-hour day. The encounter also may cause quakes and landslides on the asteroid's surface that could churn up material and uncover what lies beneath.
"The close approach is a great natural experiment," DellaGiustina said. "We know that tidal forces and the accumulation of rubble pile material are foundational processes that could play a role in planet formation. They could inform how we got from debris in the early solar system to full-blown planets."
OSIRIS-APEX mission principal investigator Dani DellaGiustina.Chris Richards/University Communications
Scientists estimate that asteroids of Apophis' size, about 367 yards (or 340 meters) across, come this close to Earth only once every 7,500 years.
"OSIRIS-APEX will study Apophis immediately after such a pass, allowing us to see how its surface changes by interacting with Earth's gravity," said Amy Simon, the mission's project scientist based at NASA's Goddard Space Flight Center in Greenbelt, Maryland.
Apophis represents more than just the opportunity to learn more about how solar systems and planets form: As it happens, most of the known potentially hazardous asteroids – those whose orbits come within 4.6 million miles of Earth – are also S-types. What the team learns about Apophis can inform planetary defense research, a top priority for NASA.
OSIRIS-APEX: Travel itinerary
By April 2, 2029 – around two weeks before Apophis' close encounter with Earth – OSIRIS-APEX's cameras will begin taking images of the asteroid as the spacecraft catches up to it. Apophis will also be closely observed by Earth-based telescopes during this time. But in the hours after the close encounter, Apophis will appear too near the sun in the sky to be observed by ground-based optical telescopes. This means any changes triggered by the close encounter will be best detected by the spacecraft.
OSIRIS-APEX will arrive at the asteroid later in April 2029, and operate in its proximity for about the next 18 months. In addition to studying changes to Apophis caused by its Earth encounter, the spacecraft will conduct many of the same investigations OSIRIS-REx did at Bennu, including using its instrument suite of imagers, spectrometers and a laser altimeter to closely map the surface and analyze its chemical makeup.
As an encore, OSIRIS-APEX will reprise one of OSIRIS-REx's most impressive acts (minus sample collection), dipping within 16 feet of the asteroid's surface and firing its thrusters downward. This maneuver will stir up surface rocks and dust to give scientists a peek at the material that lies below.
Dante Lauretta, principal investigator of the OSIRIS-REx mission, said he is excited about the extended mission as it holds the promise of uncovering new insights into the solar system's formation and planetary defense.
"As we transition from OSIRIS-REx to OSIRIS-APEX, I'm proud to pass the torch to Dani DellaGiustina and the extended mission team," he said. "OSIRIS-APEX carries the legacy of OSIRIS-REx, and I'm eager to see the discoveries it will make. This mission embodies our relentless pursuit of knowledge and the spirit of exploration."
Although the rendezvous with Apophis is more than five years away, the next milestone on its journey is the first of six close sun passes. Those near approaches, along with three gravity assists from Earth, will put OSIRIS-APEX on course to reach Apophis in April 2029.
UArizona-led Asteroid Sampling Mission's New Journey: OSIRIS-APEX - UA News
Sweating The Small Stuff: UArizona Scientists Have Begun To Study Samples From Asteroid Bennu
At the university's Kuiper-Arizona Laboratory for Astromaterials Analysis (K-ALFAA), a suite of instruments allows researchers to study the particles collected by the OSIRIS-REx mission the down to the atomic scale.Sweating The Small Stuff: UArizona Scientists Have Begun To Study Samples From Asteroid Bennu
×
By Daniel Stolte, University Communications - December 20, 2023
Lately, Tom Zega has been watching his caffeine intake before heading to work.
As a co-investigator of NASA's OSIRIS-REx sample analysis team, Zega is one of a small, but growing, number of scientists who have begun to work on analyzing the pristine extraterrestrial material that the University of Arizona-led mission brought back from Bennu, a near-Earth asteroid thought to be a leftover from the formation of the solar system 4.5 billion years ago.
University of Arizona scientists have received 200 milligrams – roughly seven-thousandths of an ounce – of the asteroid Bennu sample for analysis. The small particles pictured here in a concavity slide are observed under an optical microscope. Chris Richards/University Communications
Some particles in the Bennu sample are tiny, barely visible with the unaided eye, and manipulating them requires a very steady hand, said Zega, a professor of planetary science at the UArizona Lunar and Planetary Laboratory.
"I sometimes joke with my students about this – if you've had not enough caffeine or too much, your hand might be somewhat shaky, and the smaller the particle you're working with, the more careful you obviously have to be," he said. Currently, his team at LPL has been allocated about 200 milligrams of sample from Bennu – roughly seven-thousandths of an ounce.
Thanks to the extremely sophisticated equipment at UArizona's Kuiper-Arizona Laboratory for Astromaterials Analysis, they can extract a wealth of information from sample particles down to the nanogram, even picogram level, referring to a billionth or trillionth of a gram, respectively.
The team's main interest lies in how these materials found on the asteroid came to be, and what clues they hold for the origin of the planets, including Earth. A quarter of the sample, which is being curated at NASA's Johnson Space Center in Houston, may be allocated to the members of the mission’s science team, who are spread across the world, while about 70% will be preserved for researchers outside the mission team and for future generations, much like was done with the rocks and soil brought back by the astronauts of the Apollo moon landings, according to Zega.
"NASA preserved a large fraction of those samples for subsequent generations of scientists to look at, and we're still doing groundbreaking science on lunar samples that were brought back in the late 1960s and early 1970s," he said. "Just like the instruments we have now surpass the instruments that they had available at that time, in the future, we'll have instruments that surpass those that we have now."
University of Arizona scientists have received a small portion of the asteroid Bennu sample and analysis has begun in their lab. Here, doctoral student Lucas Smith loads Bennu sample into an electron microscope for analysis. Chris Richards/University Communications
What makes these samples unique and precious is that they were collected at the place they originated, unlike meteorites, which don't make it into the lab until after a long journey to Earth's surface. Meteorites are no longer pristine because they have been exposed to heat during their fall through the atmosphere and weathering on the ground, and they could come from anywhere. They lack, as geologists say, "context."
"With these samples from Bennu, we now have all the contextual information that will enable us to study these materials at the fundamental levels and tell the story of the origins and history of asteroid Bennu," Zega said.
A suite of instruments at the LPL's lab, ranging from optical to electron microscopes allows the team to probe the sample down to the atomic scale, according to Pierre Haenecour, assistant professor of planetary science at LPL and OSIRIS-REx co-investigator.
"We literally can look at single atoms," he said. "We also have a nanoscale secondary ion mass spectrometer, or nanoSIMS for short. It allows us to look at isotopes (different variations of atoms) to understand how each particular component in the sample originated."
Early findings confirm the predictions made about Bennu from the remote survey the OSIRIS-REx spacecraft performed during two years at the asteroid, prior to going in for the sample grab.
As suggested by remote observation of the asteroid, Bennu samples contain copious amounts of water locked up in minerals like clays. The samples are also rich in carbon, nitrogen, sulfur, and phosphorous, according to LPL assistant professor Jessica Barnes, who also is an OSIRIS-REx co-investigator.
"The abundance and isotopic composition of these and other elements will allow us to investigate where in the solar system Bennu’s parent body formed and from which constituents," she said. "The study of organic molecules may help us unravel the chemical processes that turned these simple elements into complex molecules that may have helped start life on Earth and possibly elsewhere."
Training students in cutting-edge science is an important part of the OSIRIS-REx mission. The opportunity to come to the university as a graduate student and spend four or five years working on a sample from a mission as historic as OSIRIS-REx is one that Haenecour said he would have loved.
"It really is a historic opportunity to get involved in and get to do some groundbreaking science," he said.
Discussing sample analysis measurements in the lab: doctoral students Zoë Wilbur, Lucas Smith and Iunn Ong (front to back). Chris Richards/University Communications
Working with samples of such significance comes with a responsibility that everyone takes seriously, Zega said. Getting everything right is important, and much work goes into the actual measurement itself – calibrating the instruments, taking meticulous notes and laying out the entire thought process before beginning the experiments. Some of the analytical techniques consume sample material in the process, and everyone on the sample analysis team is conscious of that, Zega said.
"I'd be lying if I said I didn't feel pressure when I'm working with one of these samples," he said, adding that when he is working in the lab, he tends to not want an audience. "Sometimes, when I have a collaborator in the lab, and we are working together, I tell them, 'I need you to not talk for the next few minutes, because we're in a really critical step here.'"
Per NASA's science requirement, the OSIRIS-REx mission was tasked with bringing 60 grams, or about two ounces, of sample to Earth. With a confirmed sample mass so far of just over 70 grams, and more sample still waiting to be extracted from the sampling head, the mission has already achieved this milestone, Zega said.
"It is very exciting to have samples from Bennu inside our labs, in the same building where the mission was first conceived by the late LPL Director Mike Drake," said Mark Marley, head of the Department of Planetary Sciences and director of LPL. "I am so proud of our faculty, staff and students who have carried his vision to completion."
The sample analysis team comprises about 200 researchers from all over the world, who coordinate the types of measurements and analyses to ensure that they maximize the science they get from the sample. Hundreds of scientific papers describing analyses of the Bennu sample are expected just in the next couple of years.
According to Haenecour, one 10-microgram particle is enough to produce science for years at a time, and the amount of sample already at UArizona is enough to keep students busy for years.
UArizona's Dante Lauretta is the principal investigator for OSIRIS-REx (formally the Origins, Spectral Interpretation, Resource Identification and Security – Regolith Explorer), and he leads the science team and the mission’s science observation planning and data processing. NASA's Goddard Space Flight Center in Greenbelt, Maryland, provides overall mission management. Lockheed Martin Space in Littleton, Colorado, built the spacecraft. Goddard and KinetX Aerospace were responsible for navigating the OSIRIS-REx spacecraft.
Sweating The Small Stuff: UArizona Scientists Have Begun To Study Samples From Asteroid Bennu - UA News
OSIRIS-REx Sample Analysis Begins at the University of Arizona - YouTube Video